The Geophysical Institute of Peru (IGP) is recruiting a Postdoctoral Researcher for a 2-year, full-time position within the Directorate of Geospace Sciences (DCG).

Based at the Jicamarca Radio Observatory (JRO) near Lima—home to the world's largest phased-array radar—the researcher will analyze comprehensive radar datasets to advance understanding of lower and upper atmospheric dynamics, ionospheric physics, and space weather coupling.

🔬 Core Responsibilities & Research Scope

Radar Data Analysis: Process and interpret multi-instrument radar observations from Jicamarca's systems to investigate equatorial ionospheric electrodynamics, plasma instabilities, and atmospheric coupling.

Collaboration: Work directly with Dr. Danny Scipión (Director of DCG) and Dr. David Hysell (Cornell University), while building an independent research profile.

Proposals & Output: Publish in top-tier peer-reviewed journals, present at international conferences, and collaborate with IGP scientists to prepare competitive grant proposals for external funding.

📋 Candidate Profile & Qualifications

Education: Ph.D. in Space Physics, Electrical Engineering, or a closely related discipline.

Recency: Ph.D. must have been awarded no earlier than 2023.

Skillset: Strong background in equatorial aeronomy, space weather, or advanced radar signal processing and observation techniques.

📅 Key Details & Application Deadline

Duration: 2 years (Full-time, fixed-term).

Location: Jicamarca Geophysical Observatory, IGP (Lima, Peru).

Application Deadline: October 30, 2026.

📩 How to Apply

Submit your application electronically as a single PDF file addressed to Dr. Hernando Tavera (Head of IGP) via email:

Application Email: postdoc@igp.gob.pe

Inquiries Contact: Dr. Danny Scipión (dscipion@igp.gob.pe)

Required Documents:

Cover Letter: Outlining your interest in the position and detailing your proposed research project.

Curriculum Vitae (CV)

References: Names and contact details of three professional references. 

For more information and how to apply, see the link below:

https://www.igp.gob.pe/convocatorias/postdoctoral2026/ 

The Center for Astrophysics | Harvard & Smithsonian (CfA); a joint collaboration of the Smithsonian Astrophysical Observatory (SAO) and the Harvard College Observatory (HCO), invites applications for its prestigious CfA Postdoctoral Fellowship and Clay Postdoctoral Fellowship programs.

These fellowships provide early-career, independent researchers with access to the extensive facilities, supercomputing networks, scientific staff, and observational resources of the CfA in Cambridge, Massachusetts.

🔬 Research Scope & Opportunities

Domain Focus: Theoretical astrophysics, observational ground- and space-based astronomy, solar & stellar physics, space weather, planetary sciences, and astronomical instrument engineering.

Independence: Fellows operate as independent primary investigators, free to pursue their own research agendas while collaborating with over 800 staff scientists and students across the CfA.

📋 Candidate Profile & Qualifications

Education: Ph.D. in Astrophysics, Astronomy, Physics, Space Physics, or a closely related field (completed prior to the start of the fellowship).

Research Track Record: Demonstrated capability for independent research, strong publication record, and innovative research proposals aligning with or extending CfA facilities and scientific priorities.

📩 How to Apply

Detailed application instructions, specific deadline dates, and submission portals are accessible via the official AAS Job Register postings:

Contact Person: Kathy Reeves (kreeves@cfa.harvard.edu)

See links below:

aas.org/jobregister/ad/94bd2ef3

aas.org/jobregister/ad/3d3c3757

The Radar Interferometry and Geospatial Science Laboratory ('Radar Lab') in the Department of Earth, Environmental, and Planetary Sciences at Washington University in St. Louis (WashU) is seeking a Postdoctoral Research Associate.

Working with Dr. Roger Michaelides, the postdoc will develop novel geodetic imaging techniques to improve surface topography characterization, vegetation canopy estimates, and periglacial landscape change detection. The project is funded primarily through the NASA Surface Topography and Vegetation (STV) Decadal Survey Incubation effort.

🔬 Core Responsibilities & Technical Scope

NASA STV Contribution: Help define science measurement needs and sensor architectures for the NASA STV targeted observable.

Geodetic & Radar Methods: Develop and apply radar remote sensing modalities (InSAR, SAR, radar altimetry, GPR) alongside LiDAR and optical remote sensing.

Arctic Environmental Science: Analyze dynamic surface processes and topographic changes over periglacial and high-latitude landscapes.

📋 Candidate Profile & Qualifications

Education: Ph.D. in Earth Science, Geophysics, Physics, Electrical Engineering, Environmental Engineering, or a related field (completed prior to appointment).

Desired Technical Skills:

Hands-on experience with remote sensing data analysis, particularly SAR and InSAR.

Proficiency in scientific programming.

Demonstrated track record of scientific writing and peer-reviewed publications.

📅 Application & Key Dates

Priority Deadline: Applications received by November 1, 2026 will receive full consideration (position remains open until filled).

Location: Danforth Campus, Washington University in St. Louis, MO.

📩 How to Apply

Submit your application package online via the WashU Workday Portal (Req ID: JR97129). Required application materials include:

Letter of Application

Curriculum Vitae (CV) including publications and employment history

Contact information for up to 3 references

Primary Contact: Dr. Roger Michaelides (applicants are encouraged to reach out directly to discuss the role).

See link below for Application: . 

https://sites.wustl.edu/radar/join-our-group-2/ 

The Space Sciences Laboratory (SSL) at the University of California, Berkeley is inviting applications for a 2-year Postdoctoral Scholar position starting in Spring/Summer 2027.

Working with Dr. L Claire Gasque and Dr. Brian Harding, the scholar will conduct original research across two complementary NASA Living With a Star (LWS) projects focused on magnetosphere-ionosphere-thermosphere (M-I-T) coupling.

🔬 Core Research & Responsibilities

Research Focus: Examine how ionospheric currents and electric fields affect conductivity, chemistry, and energy deposition, using optical phenomena like enhanced aurora, Strong Thermal Emission Velocity Enhancement (STEVE), and the picket fence.

Observational Analysis: Analyze ground-based optical data from networks such as TREx, alongside satellite measurements from missions like Swarm and DMSP.

Computational Modeling: Apply kinetic, chemical, and electrodynamic models to simulate M-I-T coupling under extreme driving, construct synthetic optical observations, and perform model-data comparisons.

Software & Mentorship: Develop open-source Python analysis tools and participate in mentoring undergraduate/graduate researchers (e.g., via the SSL ASSURE summer REU program).

📋 Candidate Profile & Qualifications

Basic Qualifications: Ph.D. (or enrollment in a Ph.D. program) at time of application.

Additional Qualifications: Ph.D. completed by start date, with no more than 3 years of post-Ph.D. research experience.

Desirable Skills: Background in Space Physics/Geophysics, experience analyzing optical or satellite datasets, knowledge of kinetic/electrodynamic models, and strong Python programming skills.

📅 Salary, Contract & Application Dates

Position Duration: 2 years (with potential renewal based on performance and funding).

Salary Range: $71,491 to $79,727 (based on UC Postdoc salary scale T23).

First Review Date: August 30, 2026 (11:59 PM PT).

Final Application Deadline: November 15, 2026.

📩 How to Apply

Applications must be submitted through the official UC Berkeley AP Recruit Portal:

Curriculum Vitae (CV)

Cover Letter

Contact information for 2 references

Inquiries: kimking@berkeley.edu 

For more information and application,see link below:

https://aprecruit.berkeley.edu/JPF05510 

The Astrophysics Center at Schmidt Sciences is recruiting the inaugural cohort of approximately five early-career scientists for the Schmidt Observatory System Postdoctoral Fellows program. The positions are based on-site in Baltimore, MD or New York, NY.

Fellows will be embedded within a small, high-impact team working across a coordinated network of ground- and space-based observatories. Multiple facilities are expected to come online over the next 2–3 years, giving fellows direct influence over observatory architecture, performance calibration, and mission-shaping science.

🔬 Core Responsibilities & Areas of Focus

Fellows will take ownership of key problem areas to produce publishable scientific research and enabling capabilities:

System Analysis & Modeling: Translate technical system behavior into quantified scientific impact, develop end-to-end simulations, and contribute to cross-observatory integration and commissioning.

Primary Focus Areas:

AI & Advanced Analysis Tools: AI-driven methods for instrument modeling, systematic error reduction, and user interaction.

Dynamic Observatory Operations: Adaptive observing strategies, scheduling, and real-time multi-facility decision-making.

Spectroscopy & Photometry Performance: End-to-end modeling, precision/stability optimization, and analysis pipeline development.

Coronagraph & High-Contrast Imaging: System-level performance modeling for exoplanet and high-contrast targets.

Time-Domain & Multimessenger Coordination: Optimization of alert handling, broker ecosystems, and transient follow-up strategies.

Future Missions & Design: Trade-space analysis and scientific trade-off evaluations for future mission concepts.

📋 Candidate Profile & Eligibility

Requirements

Education: Ph.D. in Astronomy, Astrophysics, Physics, or a closely related field.

Technical Background: Expertise in relevant domains such as instrumentation, simulation, data systems, observational astronomy, or AI/ML.

Export Control / Citizenship Notice: Requires access to U.S. export-controlled information. Candidates must be a U.S. person (U.S. citizen, permanent resident, legal asylee, or refugee) OR receive explicit U.S. Government authorization.

📅 Contract, Salary & Benefits

Appointment Type: Fixed-term (2-year position with a structured 3rd-year renewal based on performance).

Annual Salary Range: $100,000 – $130,000 / year.

Resource Support: Dedicated funding for travel, conference attendance, publication fees, computing resources, and access to advanced AI tools.

📩 How to Apply

Applications must be submitted directly through the official Schmidt Sciences careers portal.

Applicants are strongly encouraged to highlight one or more preferred Areas of Focus within their cover letter. 

For more information see link below:

https://jobs.lever.co/schmidt-entities/43e857be-8c2d-4e1d-b48c-c10f7c134b32 

The Department of Earth and Environmental Engineering at Columbia University is recruiting a Postdoctoral Researcher to develop AI-enabled approaches for evaluating and optimizing cloud seeding strategies.

Co-advised by Dr. Kara D. Lamb and Prof. Pierre Gentine, the researcher will investigate whether cloud seeding can alter precipitation and mitigate wildfire risk in the Western United States.

🔬 Core Research & Technical Scope

Numerical Modeling: Conduct aerosol-perturbation experiments using 3D Large-Eddy Simulations (LES).

Machine Learning & Optimization: Develop generative optimization, reinforcement learning, and reduced-order models to discover effective weather modification strategies.

Interdisciplinary Focus: Intersect atmospheric modeling, scientific machine learning, precipitation formation, and cloud microphysics.

📋 Candidate Qualifications & Skills

Education & Background: PhD in Atmospheric Science, Cloud Microphysics, Numerical Modeling, Machine Learning, or a closely related field.

Desirable Experience:

High-performance computing (HPC) and Python development.

Large-Eddy Simulations (LES).

Particle- or bin-based microphysics modeling.

📩 How to Apply

To apply, send your CV and Cover Letter directly to the advisors.

Co-Advisors: Dr. Kara D. Lamb and Prof. Pierre Gentine

Institution: Dept. of Earth and Environmental Engineering, Columbia University (New York, NY)

The Space Physics and Astronomy Research Unit within the Faculty of Science at the University of Oulu is recruiting a Postdoctoral Researcher to join the Ionospheric Physics research group.

The successful candidate will work within the newly established Finnish Centre of Excellence in Space Resilience, focusing on global changes in the ionosphere-thermosphere system induced by geomagnetic storms.

🔬 Core Responsibilities & Technical Tasks

Numerical Simulations: Apply existing first-principles global numerical simulations of the near-Earth space environment to analyze the impact of nominal and extreme once-per-century geomagnetic storms on the ionosphere-thermosphere system.

Satellite Data Validation: Compare simulation outputs with thermospheric neutral mass density measurements collected by Low Earth Orbit (LEO) satellites (e.g., Swarm, GRACE, GOCE).

Collaborative Research: Engage with the nationwide Space Resilience Center of Excellence network across the University of Helsinki, Aalto University, FMI, and University of Turku.

📋 Candidate Profile & Skills

Education: Ph.D. in Space Physics or a closely related field, completed prior to the application deadline and within the last 10 years.

Technical Skills: Proficiency in scientific programming (Python or MATLAB) and prior research experience in space physics.

Desirable Assets: Hands-on experience with LEO satellite data, ground-based instruments, or global numerical simulations.

General Competencies: Ability to pursue independent research, strong communication skills, and fluency in English.

📅 Salary, Duration & Key Dates

Contract: 3-year fixed-term position starting October 1, 2026 (or as agreed), subject to a 6-month trial period.

Salary: Standard Demand Level 5 scale for Finnish university research staff, starting at approx. €3,900 per month (gross) plus performance components and ePassi wellness benefits.

Location: Oulu, Finland.

Closing Date: September 1, 2026, at 23:59 Finnish Local Time.

📩 How to Apply

Applications must be submitted via the University of Oulu online recruitment portal (email applications are not accepted).

Ensure your submission is in English and includes:

Cover Letter: Motivation, prior knowledge, research interests, and career trajectory (2–3 pages).

Curriculum Vitae: Formatted following the Finnish Advisory Board on Research Integrity template.

Publication List: Following Research Council of Finland guidelines.

References: Contact details for 2 professional referees.

Academic Contact: Dr. @Heikki Vanhamäki (heikki.vanhamaki@oulu.fi) 

For more information:

https://oulunyliopisto.varbi.com/en/what:job/jobID:950976/ 

The T-2 Group (Nuclear & Particle Physics, Astrophysics and Cosmology) in the Theoretical Division at LANL invites applications for two-year postdoctoral positions in heliophysics starting in Fall 2026.

The positions focus on theoretical, computational, and observational heliophysics, with opportunities to be sponsored for LANL Distinguished Postdoctoral Fellowships (Curie, Feynman, Hoffman, Oppenheimer) or Director’s Fellowships.

🔬 Core Responsibilities & Technical Scope

Candidates across all areas of heliophysics are encouraged to apply, with particular interest in:

Energetic Particles: Particle acceleration/transport, Fokker-Planck diffusion models, solar flares, and Solar Energetic Particles (SEPs).

Computational Plasma Modeling: Particle-in-cell (PIC) simulations, hybrid fluid-particle codes, wave-particle interactions, and wave propagation.

Magnetospheric & Space Weather Physics: Radiation belt dynamics, inner/outer heliospheric modeling, and national security-related space research.

📋 Candidate Profile & Requirements

Education: Ph.D. in Space Physics, Plasma Physics, Astrophysics, or a closely related field obtained within 5 years of application submission (and prior to appointment start).

Requirements: Strong record of peer-reviewed publications, experience in scientific collaborations, and a history of presenting at professional conferences.

Citizenship Restrictions: Due to federal NDAA restrictions, non-green card holders from China, Russia, Iran, and North Korea are prohibited from accessing LANL facilities.

📅 Location, Salary & Key Dates

Location: Fully on-site in Los Alamos, New Mexico.

Contract & Salary: 2-year appointment. Starting base salary for brand-new graduates is $99,500/year, scaling upward with post-PhD experience.

Application Deadline: September 15, 2026 for full consideration (Req. Number: IRC145201).

📩 How to Apply

A complete application package requires:

CV & List of Publications

Research Statement

Contact details for 3 references

Primary Contact: Fan Guo (guofan@lanl.gov)

For more information:

Apply online via lanl.jobs with Req. Number IRC145201 

The South African National Space Agency (SANSA) is recruiting two Postdoctoral Researchers for 3-year contracts within its Space Science Programme in Hermanus, Western Cape.

The positions focus on observational and/or numerical simulation studies of Atmospheric Gravity Waves (AGWs) and Traveling Ionospheric Disturbances (TIDs).

🔬 Core Responsibilities & Tasks

Space Physics Research: Conduct observational and numerical modeling studies on AGW and TID propagation, ionospheric dynamics, and upper-atmospheric coupling.

Data Analysis & R&D: Develop computational pipelines to process space science datasets and solve complex space weather problems.

Capacity Building & Admin: Support national partnerships, participate in outreach/human capacity development, and contribute to scientific dissemination.

📋 Candidate Profile & Skills

Education: Ph.D. in Space Science, Space Physics, or Applied Mathematics.

Experience: Early-career researcher with a emerging publication record from PhD work (at least submitted papers).

Technical Skills: Strong programming skills (preferably Python) with proven data analysis and problem-solving expertise.

Work Style: Ability to work independently and within an international collaborative team.

📅 Contract, Salary & Key Dates

Positions Available: 2

Contract Type: 3-Year Contract

Location: Hermanus, Western Cape, South Africa

Compensation: R400,000 / year

Closing Date: 03 August 2026 (Job Ref: Pdoc001)

📩 How to Apply

Applications must be submitted online via the SANSA / MCI Direct Hire Portal with a detailed CV. 

For more information:

https://sansajobs.mcidirecthire.com/Vacancy 

The Department of Meteorology at Stockholm University (MISU) is recruiting a Postdoctoral Researcher to join Assistant Professor Rachel Atlas’s group.

The project focuses on understanding how large-scale atmospheric processes control intermittent bursts of stratospheric turbulence and evaluating how global climate models (e.g., ICON, IFS, ERA6) represent these dynamics compared to in-situ observations.

🔬 Core Research & Methods

Flexible Scope: Choose an observational, modeling, or combined approach.

Observations: In-situ data from aircraft, sounding rockets, and high-altitude balloons.

Modeling/Reanalysis: km-scale global simulations (ICON, IFS) and ERA6 reanalysis data (no need to run new simulations unless desired).

📋 Candidate Profile

Education: Ph.D. in Meteorology, Atmospheric Sciences, Oceanography, or a related field (ideally completed within the last 3 years).

Technical Skills: Strong scientific programming skills (preferably Python) and an excellent command of English.

📅 Contract, Salary & Key Dates

Duration: Full-time for 2 to 3 years (Start date: January 1, 2027, or earlier by agreement).

Location: Stockholm, Sweden.

Application Deadline: August 14, 2026 (Ref: SU FV-2427-26).

Inquiries: Assistant Prof. Rachel Atlas (rachel.atlas@misu.su.se). 

For more information:

https://su.varbi.com/en/what:job/jobID:952841/ 

The Space Science and Applications Group at LANL is inviting applications for a postdoctoral position blending hands-on hardware development with fundamental space science research. LANL develops and operates instrumentation for major initiatives, including NASA’s IMAP mission, alongside active national security space arrays.

🔬 Core Responsibilities

Hardware Operations: Supporting the development, laboratory calibration, environmental testing, and operations of space plasma instruments and energetic neutral atom (ENA) imagers.

Future Payloads: Contributing to the baseline design of instrumentation for future space missions.

Scientific Research: Investigating heliospheric, magnetospheric, or ionospheric physics, solar wind-plasma interactions, or ENA telemetry.

Data Analysis: Processing space-based measurements, publishing in peer-reviewed journals, and presenting at conferences.

📋 Candidate Profile

Education: A Ph.D. in Space Physics, Physics, Astronomy, Engineering, or a related field completed within the past five years.

Clearance: Ability to obtain a DOE Q clearance (typically requires U.S. citizenship). Note: U.S. citizenship is NOT a requirement to apply.

Desired Assets: Laboratory experience with detectors, vacuum systems, or calibration facilities; experience with computational data analysis, modeling, or simulation.

📅 Location, Salary & Terms

Location & Duration: Fully on-site in Los Alamos, NM. 2-year initial contract with a possible 3rd-year extension.

Compensation: Minimum starting salary of $97,000, scaling upward with post-PhD experience. Strong candidates may eligible for prestigious Laboratory fellowships.

Timeline: Rolling basis review; positions filled as applications are received.

📩 How to Apply

Submit a Cover Letter describing your background, a full CV, and contact details for three professional references directly to senior staff:

Carlos Maldonado: cmaldonado@lanl.gov

Ruth Skoug: rskoug@lanl.gov

For more information:

https://lanl.jobs/search/jobdetails/space-physics-instrumentation-and-data-analysis-postdoctoral-researcher/adfde200-f6ee-4643-a517-928b3cc41381  

An exciting opportunity is available within the School of Physical and Chemical Sciences at Queen Mary University of London (QMUL).

The successful candidate will work on the high-profile UKRI Future Leaders Fellowship (FLF) project: “Exploring New Regions of Space: Fundamentals and Impacts of Astrophysical Plasma Turbulence”.

This highly collaborative initiative features flexible, interlinking projects aimed at bridging the gap between fundamental plasma physics and applied space weather research.

🔬 The Research Scope & Methodology

The project investigates the mechanics of plasma turbulence and the critical role it plays in governing heliospheric and astrophysical systems—including its largely unmapped impacts on space weather. To accommodate a diverse range of technical backgrounds, the project spans multiple methodologies:

Observational Data Analysis: Interrogating cutting-edge datasets from active heliophysics and space physics missions.

Experimental & Numerical Modeling: Engaging with laboratory plasma experiments, theoretical physics frameworks, numerical fluid/kinetic simulations, and predictive space weather modeling.

Interdisciplinary Integration: Team members are encouraged to bring deep expertise in at least one of these areas while actively collaborating across the others.

📋 Candidate Profile

Education: A PhD (or equivalent) in Space Physics, Astrophysical Plasma Physics, Laboratory Plasma Physics, or a closely related discipline.

Core Competencies: A proven track record of conducting and disseminating internationally high-quality, innovative research.

Attributes: Highly motivated, capable of demonstrating strong individual initiative, and committed to successful team collaboration, academic life, and ethical working practices.

📅 What is Offered & Application Requirements

Career Support: The UKRI Future Leaders Fellowship framework provides extensive, dedicated career development support and professional mentoring for all team members.

The Institutional Environment: The Space & Astrophysical Plasmas group is embedded within QMUL's Astronomy Unit, a world-class environment featuring state-of-the-art research facilities following a recent £12M refurbishment.

Application Document: In addition to a standard CV, applicants must upload a Research Statement detailing previous achievements and future research plans (maximum of 2 pages) to the supporting documents section of the portal.

📩 Contact Information

For informal inquiries regarding the scientific scope of the turbulence frameworks, project timelines, or role details, you can contact the Principal Investigator directly:

Contact: Dr. Christopher Chen

Job Title: Reader in Space Plasma Physics

Email: christopher.chen@qmul.ac.uk 

For more information and applications link:

https://qmul-jobs.tal.net/vx/mobile-0/appcentre-ext/brand-4/candidate/so/pm/1/pl/3/opp/9805-Postdoctoral-Research-Associate/en-GB 

Reminder: Deadline is in a few days.

The Rhodes University Centre for Radio Astronomy Techniques & Technologies (RATT), in partnership with SARAO, is seeking a visionary Postdoctoral Fellow to lead the scientific coordination of the Transient Array Radio Telescope (TART) Africa network.

This is more than a research role—it is a leadership opportunity to drive scientific output, foster pan-African collaboration, and build sustainable capacity in radio astronomy across the continent.

🚀 Key Responsibilities

Network Coordination: Lead the scientific exploitation of the TART Africa network.

Community Building: Support and expand collaborations within the African radio astronomy community.

Impact & Outreach: Drive science development initiatives and public outreach programs.

✅ Requirements

Education: PhD in Radio Astronomy or a closely related field.

Network: Proven experience collaborating within the African radio astronomy ecosystem.

Passion: A demonstrated commitment to outreach and scientific capacity building.

📍 Location & 💰 Funding

Host: Rhodes University or SARAO’s Cape Town offices.

Stipend: ZAR 478,826 per year (Tax-free, adjusted annually for inflation).

📅 How to Apply

Deadline: 15 April 2026 (Applications reviewed until the position is filled).

Please submit the following to applications@ratt.center

Full CV & Bibliography.

A brief summary of your research.

Three letters of recommendation (to be sent separately by your referees).

📍 Swedish Institute of Space Physics (IRF), Kiruna, Sweden

📅 Deadline: November 25, 2025

📑 Ref: DNR 2.2.1-363/25

The Swedish Institute of Space Physics (IRF) invites applications for a Postdoctoral Researcher to study space debris and meteoroids using the cutting-edge EISCAT_3D radar system — one of the world’s most advanced tools for space and atmospheric research.

🌌 About the Project:

In collaboration with EISCAT AB, this project focuses on developing methods to:

• Perform 3D measurements of meteoroids and space debris

• Analyze how the ionosphere affects orbital accuracy

• Develop signal analysis and data processing techniques for space situational awareness

• Combine radar data for both ionospheric and space object studies

Your research will directly contribute to global efforts in tracking and mitigating space debris, and results will be shared through international peer-reviewed publications.

🎓 Qualifications:

• PhD in Space Physics, Physics, or related field

• Proficiency in Python, C++, or similar programming languages

• Background in signal processing, inverse modeling, or numerical methods (a plus)

• Excellent English communication skills; Swedish is an advantage

💼 Terms & Benefits:

• 📆 3-year contract (start as soon as possible)

• 💰 Competitive salary (negotiated individually)

• 🌍 International, equality-driven workplace

• 🕒 Flexible hours + 7 weeks vacation

• 💪 Comprehensive healthcare, wellness programs & on-site gym

Join IRF in advancing space situational awareness and atmospheric science from one of Europe’s most northern research hubs.

📩 Apply with:

CV, cover letter, publication list, and two references. 

Exciting news for early-career solar physicists!

Professor Zhenghua Huang and the newly established Solar Physics Group at Nanjing University (Suzhou Campus) are inviting applications for a two-year postdoctoral position in Solar Physics.

This role offers a rare chance to play a core research role in understanding energy and mass coupling processes in the solar atmosphere, combining cutting-edge solar observations with advanced numerical simulations. The successful candidate will work closely with the CHASE mission team and contribute to preparations for the upcoming 2.5-meter solar telescope—placing you at the forefront of modern solar research.

🔬 Research focus

• Solar atmospheric dynamics

• Energy and mass coupling processes

• Solar data analysis and numerical simulations

• Collaboration with major solar missions and telescope teams

📍 Position details

• Location: Suzhou Campus, Nanjing University (China)

• Contract: Full-time, fixed-term (2 years)

• Start date: Negotiable (on or before end of 2026)

• Salary: CNY 20,000 – 24,000/month (gross), depending on experience

• On-campus accommodation: May be available

• Working language: English

🎓 Eligibility

• PhD in Physics, Astrophysics, or a closely related field (completed or near completion)

• No more than 3 years of postdoctoral (or equivalent) research experience

• Strong background in solar data analysis and/or numerical simulations

• Excellent scientific writing and presentation skills in English

📧 How to apply

Please send your CV and any inquiries directly to:

Professor Zhenghua Huang

📩 huangzh@nju.edu.cn 

The Space Science and Applications Group (ISR-1) at Los Alamos National Laboratory (LANL) is inviting applications for postdoctoral researchers in heliospheric physics.

🔬 Core Research Focus

Successful candidates will carry out original research aimed at answering foundational heliophysics questions in Particle Energization, Outer Heliosphere, Broad Heliophysics.

📋 Candidate Profile

Minimum Job Requirements:

A Ph.D. in Space Physics completed within the last five years, or soon to be completed (must be finished by the position start date).

Demonstrated experience in the observational data analysis of space, heliospheric, or magnetospheric physics missions.

Strong scientific programming and coding experience (e.g., Python, IDL, C++).

Communication: A proven track record of publishing in scientific journals and effectively communicating research both orally and in writing.

Desired Qualifications:

Hands-on experience with space plasma or ENA instrumentation and hardware calibration techniques.

Experience utilizing numerical modeling tools for particle detection and instrument simulation (such as SIMION or SRIM).

📅 Appointment Details & Top-Tier Compensation

Location: Fully on-site in Los Alamos, New Mexico.

Duration: 2 years initial appointment, with a possible extension for a 3rd year.

Salary: Highly competitive, scaling with post-PhD experience. The starting salary for a brand-new graduate is $97,000.

Citizenship: U.S. citizenship is NOT a requirement; international researchers are encouraged to apply.

Fellowships: Exceptionally strong candidates may be nominated for prestigious Laboratory Fellowships, which offer additional funding and distinction.

Timeline: Review of applications begins immediately on a rolling basis and will continue until the position is filled.

📩 How to Apply

To receive full consideration, your application package must include:

A Cover Letter detailing your scientific background and relevant mission/data experience.

A full CV / Resume (including a comprehensive publication list).

Contact information for three professional references.

For scientific or technical inquiries about the IMAP instruments and research directions, you can directly reach out to the principal scientists:

Dan Reisenfeld at dreisenfeld@lanl.gov

Ruth Skoug at rskoug@lanl.gov

For more information and applications:

https://lanl.jobs/search/jobdetails/heliospheric-physics-postdoctoral-researcher/f48824a4-bfd0-4ccc-b5e8-1c277dc2f312 

The Department of Mechanical and Aerospace Engineering within the Space Systems Research Group at The University of Manchester (UK) is recruiting a PhD student for the MoRe Spacecraft Framework project ("Towards Modular and Reusable Space System Design").

Supervised by Dr. Manu H. Nair and Dr. Nicholas Crisp, this 3.5-year doctoral project focuses on developing a modular, standardized, and reusable spacecraft design methodology across mechanical, structural, thermal, electrical, payload, and software domains to enable In-Orbit Servicing, Assembly, and Manufacturing (ISAM) and Active Debris Removal (ADR).

🔬 Core Research & Technical Scope

Design Framework & Architectures: Develop the MoRe Spacecraft Framework to standardize subsystem interfaces, allowing spacecraft components to be replaced, upgraded, or reused across missions.

Digital Engineering & MBSE: Combine Model-Based Systems Engineering (MBSE, SysMLv2), MATLAB/Simulink modeling, multi-criteria optimization, and digital engineering toolkits.

Quantitative Figures of Merit: Establish quantitative metrics for modularity, interoperability, maintainability, reusability, sustainability, and lifecycle performance.

Scenario Evaluation: Test and validate modular architectures against representative missions including ISAM, ADR, spacecraft upgrading, and mission life extension.

📋 Candidate Profile & Academic Requirements

Academic Criteria:

Upper second-class (2:1) UK honours degree (or international equivalent) in Aerospace Engineering, Systems Engineering, or Mechatronic Engineering; OR

Any 2:1 honours degree plus a Master’s degree at Merit level (or international equivalent) in Aerospace Engineering, Systems Engineering, or Mechatronic Engineering.

Technical & Personal Attributes: Interest in space systems engineering, computational modeling, open to candidates returning from career breaks or seeking flexible/part-time study arrangements.

💰 Funding & Position Details

Duration: 3.5 years (Full-time or flexible part-time options at 50%, 60%, or 80%).

Expected Start Date: September 2027.

Financial Package: Full UK/International tuition fees, UKRI minimum annual stipend (£21,805 / year), plus up to £2,500 / year for research training support grants (RTSG). Candidates with industry co-funding or external funding are also eligible.

📅 Application Deadlines & Review Rounds

The position remains open until filled across two primary decision rounds:

First Application Review: Apply by November 1, 2026 (Decision expected by December 18, 2026).

Second Application Review: Apply by January 15, 2027 (Decision expected by March 30, 2027).

📩 How to Apply

Prior to applying, candidates are strongly recommended to contact the supervisors directly to discuss research alignment.

Formal applications must be submitted via the University of Manchester Online Application Portal selecting the PhD School of Engineering Scholarships option. Required documents:

Supporting Statement / Motivation Letter detailing interest and suitability for the project.

Curriculum Vitae (CV).

Academic Transcripts & Certificates.

Contact details for two academic/professional references.

Supervisors: Dr. Manu H. Nair & Dr. Nicholas Crisp

Department Portal: Department of Mechanical and Aerospace Engineering, University of Manchester.

For application and more details, see link below:  

https://www.findaphd.com/phds/project/school-of-engineering-phd-scholarships-more-spacecraft-framework-towards-modular-and-reusable-space-system-design/?p198964

The Department of Arctic Geophysics at The University Centre in Svalbard (UNIS) in Longyearbyen, Svalbard is hiring a 3-year PhD Fellow (Stipendiat, Code 1017). The position is part of a 5-year Research Council of Norway project investigating mesoscale ionospheric flows and space weather dynamics in collaboration with the University of Oslo (UiO) and the British Antarctic Survey (BAS).

The candidate will be enrolled in the doctoral program at the University of Oslo (UiO).

🔬 Core Responsibilities & Scientific Scope

Data Analysis & Modeling: Analyze historical and new datasets from SuperDARN and EISCAT radars to determine how ionospheric mesoscale flows (~10–100 km) vary across different Magnetic Local Times (MLT) under varying local conductivity, electric fields, and auroral precipitation drivers.

Methodology Development: Develop, deploy, and test new analysis methods on the Longyearbyen SuperDARN radar.

Radar Operations & Maintenance: Assist in operating and maintaining the Svalbard SuperDARN radar station located on Breinosa.

Collaborative Exchanges: Participate in international project collaborations, including research visits to BAS (Cambridge, UK) and UiO (Oslo, Norway), and present research at international conferences.

📋 Qualifications & Requirements

Required:

Education: Master’s degree (or equivalent) in a field relevant to space/ionospheric physics, completed or scheduled to be completed by January 31, 2027. Must meet admission requirements for the PhD program at UiO.

Physics & Math Background: Strong grounding in mathematics and physics relevant to ionospheric and space plasma physics.

Data Processing & Programming: Demonstrated experience in processing and analyzing large datasets using Python or MATLAB.

Language: Proficiency in written and spoken English.

Advantageous:

Hands-on experience with SuperDARN, EISCAT, or related analysis toolkits (PyDARN, FITACF, GUISDAP, RST).

Experience applying or developing AI/machine learning tools for scientific data analysis.

Peer-reviewed publication record (authorship or co-authorship).

Class B driver's license (valid in Svalbard) and experience living/working in Arctic/polar environments.

💼 Compensation & Position Details

Duration: 3 years (Full-time, no required teaching duties).

Start Date: March 2027 (flexible).

Location: UNIS, Longyearbyen, Svalbard (78°N).

Salary & Benefits: Base salary (PhD Code 1017) plus an additional Svalbard allowance of NOK 44,640 per year. Favorable tax regime in Svalbard (8% income tax + 7.6% national insurance). Includes membership in the Norwegian Public Service Pension Fund (SPK), relocation allowance (up to NOK 10,000), and access to staff housing.

📅 Application Deadline & Key Contacts

Application Deadline: October 23, 2026

Primary Contacts:

Professor Lisa Baddeley (lisab@unis.no)

Professor Dag Lorentzen (dagl@unis.no)

📩 How to Apply

Applications must be submitted electronically through Jobbnorge. Required attachments:

Motivational Letter (max 1 page) detailing scientific interest in the project and motivation to study at UNIS.

Full Academic CV.

Transcripts & Diplomas (Bachelor's and Master's degrees, or official confirmation of completion by Jan 31, 2027; retrieved via Vitnemålsportalen.no if studied in Norway).

References: Contact information for 2 references (including Master's thesis supervisor).

The newly established research group led by Dr. Ekaterina Ilin under the ERC Starting Grant project PLANETARE at the Max Planck Institute for Solar System Research (MPS) (Göttingen, Germany) is offering a PhD position in time-domain exoplanet science and stellar magnetism.

The project focuses on confirming and characterizing magnetic star-planet interaction (SPI) in close-in exoplanetary systems, evaluating how short-orbit exoplanets modulate host star magnetism through time-resolved X-ray, radio, and optical observations.

🔬 Research Scope & Core Objectives

X-ray Time-Domain Analysis: Analyze new and archival XMM-Newton X-ray observations of target systems to test whether suspected planet-induced emissions recur on the planetary orbital period.

Multi-Wavelength Extensions: Extend investigation to optical photometrics and radio diagnostics to evaluate different physical interaction mechanisms (e.g., planet-induced flaring).

Binary Interactions: Explore low-mass binary interactions at optical wavelengths.

Theoretical Modeling: Construct empirically motivated models of magnetic interactions and predict distinct observational signatures.

Observing Proposals: Formulate and submit observing proposals, selecting prime interaction candidates from project-identified targets.

📋 Candidate Profile & Preferred Skills

Education: Master’s degree (or equivalent) in Physics, Astrophysics, Astronomy, or a closely related discipline completed prior to the start date.

Programming Skills: Experience in scientific programming using Python.

Data Reduction: Prior experience in reducing and analyzing time-series datasets from X-ray, radio, or optical observatories.

Collaborative Mindset: Ability to work within a small, focused team (2 postdocs and 1 PhD student) and communicate research findings effectively at international stellar/exoplanet conferences.

💼 Position Details & Work Environment

Host Institution: Department of Solar & Stellar Interiors, Max Planck Institute for Solar System Research (MPS), Göttingen, Germany.

Start Date: Flexible in early 2027.

Team Structure: Part of the newly formed ERC PLANETARE group led by PI Ekaterina Ilin, collaborating closely with two postdoctoral researchers.

📅 Application Deadline & Process

Application Deadline: October 1, 2026 (Note: Related group postdoc positions close October 30, 2026). See comment section for links to more information and application details.

Inquiries: Dr. Ekaterina Ilin (ilin@mps.mpg.de).

For more information on how to apply:

https://www.mps.mpg.de/phd/star-planet-interactions

The Magnetospheres of the Outer Solar System (MOSS) group led by Prof. Sven Simon at the Georgia Institute of Technology (Atlanta, USA) is recruiting funded Ph.D. students starting in calendar year 2027.

The group conducts theoretical, computational, and observational studies of plasma interactions with moons in the outer Solar System, with a primary focus on the Galilean moons of Jupiter.

🔬 Core Research & Scope

Focus Area: Moon-magnetosphere plasma interactions in the outer solar system (e.g., Galilean satellites of Jupiter).

Methodologies: Theoretical plasma physics, kinetic and fluid numerical modeling, and spacecraft observational data analysis.

📋 Candidate Profile & Qualifications

Education: Undergraduate degree (B.S./B.Sc. or equivalent) in Physics, Astrophysics, Planetary Science, or a related discipline.

Core Competencies: Candidates should be comfortable tackling theoretical and/or numerical problems.

📅 Application Timeline & Home Departments

Georgia Tech allows prospective students to apply through either of two home departments depending on academic preference:

School of Earth and Atmospheric Sciences (EAS): Admissions recommendations are made directly by individual advisors.

School of Physics: Standard departmental admissions pathway.

Application Deadlines: December 2026 (for admission starting in 2027).

📩 How to Apply

Prior to submitting a formal university application, interested candidates are strongly encouraged to contact the PI directly to arrange an introductory meeting and discuss research alignment:

Primary Contact: Prof. Sven Simon

Email: ssimon32@gatech.edu (Attach your CV to the initial email)

For more information and how to apply, see link below:

https://svensimon.gatech.edu/

The International Max Planck Research School on Earth System Modelling (IMPRS-ESM), joint with the Max Planck Institute for Meteorology and Universität Hamburg, invites applications for its annual doctoral program starting March 1.

The school focuses on Earth system dynamics, climate variability, atmospheric/oceanic processes, and sustainability sciences using advanced numerical models and high-performance computing.

🔬 Research Scope & Tracks

Candidates work with complex Earth system models across four main research areas:

Atmospheric Processes and Climate Change

Earth System Coupled Dynamics and Climate Change

Ocean Climate Physics and Climate Variability

Economics and Sustainability Sciences

📋 Candidate Profile & Qualifications

Education: A first-class Master’s degree (including a written MSc thesis) in Physics, Geophysical Sciences (Meteorology/Oceanography), Mathematics, Computer Science, Engineering, Ecology, Economics, or Political Science (students completing their MSc are eligible).

Credit Requirement: Combined BSc + MSc coursework totaling at least 300 ECTS credits (or international equivalent).

Technical Skills: Experience with numerical modeling, scientific programming, large dataset processing, and statistical analysis.

📅 Annual Application Timeline & Key Dates

July 1 – September 15: Online application registration window.

September 20: Deadline for online reference letter submissions.

Early November: Interview invitations issued.

November 26–27: Candidate interviews.

March 1: PhD position start date (flexible upon agreement).

💰 Contract & Funding

Duration: 3-year doctoral contract with comprehensive social benefits.

Stipend/Salary: Monthly net payment of approx. €2,100 (sufficient to cover living expenses in Hamburg).

Supervision: Dedicated personal scientific Advisory Panel and structured graduate school support.

📩 How to Apply

Applications must be submitted electronically through the IMPRS-ESM online portal in two consolidated PDF files:

Application Package: Prepared according to official formatting instructions.

Two Reference Letters: Submitted directly by referees using the official IMPRS reference form before September 20. (Hardcopy or faxed submissions are not accepted).

The International Meridian Circle Program (IMCP), hosted by the National Space Science Center (NSSC) of the Chinese Academy of Sciences (CAS) in Beijing, China, is recruiting scientists across multiple career stages.

IMCP is establishing a global collaborative geospace super-observatory along the Asian-American and European-African Meridian sectors to investigate solar-terrestrial coupling, space weather dynamics, and atmosphere-lithosphere-ionosphere interaction.

🔬 Core Focus Areas

Disciplines: Space physics, space weather forecasting, solar physics, atmospheric physics, geophysics, data science, and numerical modeling.

Observation Framework: Ground-based distributed observation networks, instrument deployment, data standardization, and global observation coordination.

💼 Open Positions & Key Qualifications

Lead Expert

Scope: Internationally recognized leaders in ground-based observation, solar wind-geospace coupling (magnetosphere, ionosphere, thermosphere), and atmosphere-lithosphere processes.

Role: Lead international and China-based scientific programs, drive network deployment, and manage multi-institutional collaborations. Long-term position in Beijing.

Discipline Experts

Scope: Senior researchers (~20 years of research experience, professor-equivalent rank, with ≥3 years of international experience) in solar-terrestrial physics or ground-based space exploration instrumentation.

Role: Lead fundamental research programs or oversee global/domestic observational facility deployment and regional centers.

Early Career Scientists

Scope: Ph.D. with ≥7 years of experience (and ≥3 years at internationally recognized institutes/teams) focusing on geospace monitoring networks.

Role: Independent research, host visiting scholars, mentor postdocs, and contribute to network technical support and data standards.

Postdoctoral Positions

Scope: Ph.D. obtained within the past 3 years (under 35 years of age). Fresh Ph.D.s and international applicants are highly encouraged.

Role: Conduct innovative research on M-I coupling, space weather, and atmospheric dynamics using IMCP data and models. Renewable or convertible to permanent research staff.

📅 Salary, Support & Key Details

Benefits: Competitive salary package, research funding, office/lab infrastructure, transitional housing, and support for CAS/National talent programs.

Location: IMCP Headquarters, Beijing, China.

Application Window: Open until filled (rolling reviews start within one month of submission).

📩 How to Apply

Submit application materials electronically to hr@nssc.ac.cn. Required documents:

Curriculum Vitae (CV) with full publication list.

Research Statement & Plan (max 2 pages).

Two Recommendation Letters (mandatory for Postdoc applicants; optional for senior roles).

Contacts: Ms. Zheng, Dr. Ren

Phone: +86-10-62582610

Emails: hr@nssc.ac.cn / lwren@spaceweather.ac.cn

Dr. Kun Zhang is recruiting Ph.D. students for the Engineering Physics program at Embry-Riddle Aeronautical University (Daytona Beach Campus).

Key Details

Research Focus: Space physics, specializing in solar wind–magnetosphere interactions and inner magnetospheric physics.

Financial Support: Funding is available through Graduate Research Assistantships (RA) or Teaching Assistantships (TA), depending on qualifications.

Location: ERAU Daytona Beach Campus, Florida.

How to Apply

Review research projects on Dr. Zhang's Research Page and the application requirements on the ERAU Doctoral Admissions Page.

Early applications are strongly encouraged. Applicants should explicitly indicate their interest in working with Dr. Kun Zhang within their personal statement.

For more information, see link below:

https://erau.edu/admissions/graduate-admissions/doctoral-students 

For direct inquiries, contact Dr. Zhang at zhangk5@erau.edu. 

Dr. Piyush M. Mehta (Associate Professor and Director of the ASSIST Lab) is recruiting 2 Ph.D. students to join the Department of Mechanical, Materials, and Aerospace Engineering at West Virginia University.

The positions are backed by a new project funded by the National Science Foundation (NSF) Space Weather Program, in collaboration with co-investigators (Mrinal Kumar, Edward Oughton, Subhamoy Chatterjee, and Matthew Stevenson) alongside federal, industry, and international partners.

🔬 Research Scope & Core Focus

Primary Domain: Space Weather, Atmospheric/Thermospheric Modeling, Satellite Aerodynamics/Drag, and Space Situational Awareness (SSA).

Methodologies: Machine learning / AI integration for space weather forecasting, uncertainty quantification, probabilistic modeling, and upper-atmosphere dynamics.

📋 Candidate Profile & Qualifications

Target Audience: Highly motivated students interested in aerospace engineering, computational space physics, machine learning applications, and space environment sustainability.

Start Date: Spring 2027 start is possible and preferred.

📩 How to Apply

Interested candidates should reach out directly to Dr. Piyush M Mehta via email.

Contact Person: Dr. Piyush M Mehta

Email: piyush.mehta@mail.wvu.edu

Department: Department of Mechanical, Materials, and Aerospace Engineering, WVU 

The DAWN Group within the Institute of Earth Surface Dynamics and Expertise Center for Climate Extremes at the University of Lausanne (UNIL) is inviting applications for a fully funded PhD position lasting up to 5 years.

The position centers on pioneering research at the intersection of atmospheric physics and artificial intelligence.

🔬 Research Scope & Custom Project Proposal

Candidates are expected to propose a creative research idea spanning atmospheric physics (e.g., aerosol–cloud interactions, atmospheric convection, tropical meteorology, extremes) and scientific machine learning (e.g., causal ML, hybrid physics–AI modeling, generative modeling, operator learning).

📋 Candidate Profile & Qualifications

Education: Master's degree (completed or expected before start date) in Atmospheric Science, Climate Science, Physics, Applied Math, Statistics, Computer Science, or Data Science.

Technical Skills: Strong scientific programming and data-analysis skills (preferably Python) with experience handling large scientific datasets or numerical models.

Languages: Fluent in English (French or German are not required).

📅 Salary, Funding & Key Dates

Salary & Perks: Annual salary scaling from ~CHF 54k (Year 1) to ~CHF 63k (Year 5), plus 5 weeks paid holiday, computing hardware/GPU access, conference travel, and publication funding.

Target Start Date: March 1, 2027.

Application Deadline: September 15, 2026 (for full consideration).

📩 Required Application Documents

Submit via the UNIL online portal as separate PDFs:

CV & Transcripts/Certificates.

References PDF: Contact details for 2 academic referees.

Written Work Sample: One lead-authored report, thesis, or manuscript.

Short Statement (max 250 words): Favorite research experience, career goals, and teaching/mentoring interests.

Project Proposal (max 500 words): Creative PhD project idea linking atmospheric physics and AI.

Inquiries: dawn-jobs@unil.ch

For more information:

https://wp.unil.ch/dawn/phd-positions-details/ 

The Space Robotics and Generative Estimation Lab (SRGE) at Embry-Riddle Aeronautical University (ERAU) in Daytona Beach, Florida, is recruiting for multiple funded Ph.D. positions starting in January or August 2027.

🔬 Core Research & Hardware Operations

Focus Area: Planetary and terrestrial robotics, state estimation, autonomous navigation, and robotic control.

Hands-on Hardware: Daily work with real-world robotic platforms, including a fleet of 10+ quadrupeds, wheeled quadrupeds, rovers, bipeds, and hybrid platforms backed by dedicated high-performance computing power.

📋 Candidate Profile & Qualifications

Research Focus: Highly motivated candidates aiming for high-impact journal and conference publications.

Technical Skills: Comfortable with both software development and hardware integration.

Attributes: Resilient problem-solvers with a passion for hands-on field testing and physical robot deployment.

📅 Important Dates & Application Process

Start Dates: January 2027 or August 2027.

International Applicants (January 2027 Start): Must submit their official ERAU university application by September 15, 2026.

📩 How to Apply

Apply directly using the lab's dedicated recruitment form. For inquiries, email the lab directly (LinkedIn DMs are not monitored).

Application Form: Available via the post link (https://lnkd.in/eRdNWEJr)

Contact Email: spaceroboticserau@gmail.com 

The Department of Space Science at The University of Alabama in Huntsville (UAH) is offering one or two Graduate Research Assistant (GRA) positions for students pursuing a Ph.D. in Space Science, with a preferred start date of Spring 2027.

🔬 Core Research & Computational Methods

The positions focus on computational plasma physics and numerical modeling, specifically:

Computational Magnetic Reconnection: Studying the onset of plasma instabilities, particle acceleration, and particle transport mechanisms.

Numerical Techniques: Utilizing Particle-in-Cell (PIC), hybrid fluid-particle, or two-fluid simulation codes.

📋 Minimum Qualifications & Profile

Education: B.S. degree in Physics or a closely related field.

Desirable Background: Prior background or coursework in plasma physics and computational methods is preferred.

📩 How to Apply

Interested candidates should contact Dr. Haihong Che as soon as possible via email.

Contact Person: Dr. Haihong Che

Email: hc0043@uah.edu

Application Materials: Email your CV and college transcripts.

The Environmental Remote Sensing Lab in the Department of Geography at Texas A&M University (TAMU), led by Dr. Xiaojing Tang, is recruiting a motivated Ph.D. student starting in Fall 2027.

🔬 Core Research & Scope

Focus Area: Leveraging dense time series of Earth observation data to monitor environmental changes, specifically focusing on urban albedo changes and their impacts on urban climate using weather/climate modeling and simulations.

Applications: Land use/land cover change, urban albedo, climate modeling, and geospatial intelligence.

📋 Candidate Profile & Qualifications

Education: Strong quantitative foundation in environmental sciences, remote sensing science and technology, or related fields.

Technical Skills: Proficiency in scientific programming (Python, R, or MATLAB) and Google Earth Engine (GEE) is highly desirable.

Experience: Prior research experience in remote sensing, urban climate, or geospatial modeling is a plus.

📩 How to Apply

Interested applicants should email Dr. Xiaojing Tang directly at xjtang@tamu.edu with the following materials:

Cover letter

Curriculum Vitae (CV)

Academic transcripts

Writing sample

Contact details for references (names, emails, and affiliations)

The Faculty of Science at the University of Helsinki invites applications for a 3-year fixed-term Doctoral Researcher position within the Dynamic Meteorology Group at the Institute for Atmospheric and Earth System Research (INAR).

The candidate will work on the AI-Dream project under the supervision of Dr. Clément Bouvier, developing evaluation frameworks to test the physical validity and explainability of deep ML weather prediction models in HPC environments.

🔬 Core Responsibilities & Research Scope

Physics-Based AI Evaluation: Build test suites and criteria to assess the physical accuracy and conservation laws of deep ML weather forecasting models.

Explainable AI (XAI): Utilize state-of-the-art interpretability techniques, such as Deep Linear Probes and Latent Space Cartography, to inspect how ML models encode atmospheric dynamics.

HPC & Data Management: Handle large meteorological datasets in high-performance computing clusters.

International Collaboration: Work closely with international partner institutions, including a mandatory 3-month research visit to the University of Cambridge (working with Prof. Driscoll), as well as collaborations with Washington University, ECMWF, and LUT University.

📋 Candidate Profile & Eligibility

Education: Master’s degree (completed or near completion) in Meteorology, Physics, Computer Science, or a closely related quantitative field.

Domain Knowledge: Strong foundation in dynamic meteorology.

Technical Skills: Experience in Python programming and statistical data analysis. Prior experience in Machine Learning or Numerical Weather Prediction (NWP) is a strong advantage.

Requirements: Excellent written and spoken English skills, willingness to complete the 3-month research stay in Cambridge, and eligibility/enrolment in the University of Helsinki doctoral program (obtainable within the 6-month trial period).

📅 Contract, Salary & Key Dates

Duration: 3 years fixed-term, starting January 2027 at the latest (+ a 6-month probationary period).

Salary: Starting gross salary of approx. €2,700 – €2,900 per month, depending on qualifications, + occupational healthcare and sports benefits.

Location: Helsinki, Finland (INAR).

Application Deadline: 28/08/2026.

📩 How to Apply

Applications must be submitted as a single merged PDF via the official University of Helsinki recruitment system

The PDF must include:

Motivation Letter (1 page max).

Curriculum Vitae (2 pages max) emphasizing experience in Dynamic Meteorology, ML, or NWP.

Academic Transcripts & Grade Cards (B.Sc. and M.Sc. including thesis topic and grade).

Primary Contact: Dr. Clément Bouvier (clement.bouvier@helsinki.fi)

For more information,

https://jobs.helsinki.fi/job/Helsinki-Doctoral-Researcher%2C-Atmospheric-Sciences/1363904057/

The Planet Formation Group, led by Dr. Joanna Drążkowska at the Max Planck Institute for Solar System Research (MPS / University of Göttingen), is offering a PhD position focused on vertically resolved modeling of dust evolution in protoplanetary disks.

The project aims to build a comprehensive model connecting early micron-sized dust grains to planetesimals and planets, leveraging evidence from Solar System materials and disk observations.

🔬 Core Research & Code Development

The successful candidate will advance the group's publicly available 2D Monte Carlo code, mcdust, to investigate the interplay between disk midplane dynamics and vertically puffed-up disk surfaces. Potential research tracks tailored to candidate interest include:

Thermochemical Modeling: Coupling with codes like DALI (Dust and Lines) to study feedback between thermal structure, dust composition, and growth.

External Photoevaporation: Integrating PUFFIN (Python Utility For Fuv Irradiated disc deNsities) to model planetesimal and comet formation under stellar irradiation.

Dust Electrostatics: Incorporating aggregate electrostatic charging to analyze its influence on dust coagulation barriers.

📋 Candidate Profile

Education: Master's degree (or equivalent) in Astrophysics, Physics, Computational Physics, or a related field.

Core Competencies: Strong background in planet formation, computational astrophysics, or numerical fluid/particle modeling.

Technical Skills: Prior experience with Fortran and Python code development is strongly preferred.

📩 Contact & Application

Interested candidates should apply through the official MPS/institutional application portal.

Advisor: Dr. Joanna Drążkowska (Research Group Leader)

Phone: +49 551 384 979-523

Email: drazkowska@mps.mpg.de

For more information, see link below

https://www.mps.mpg.de/phd/planet-formation?c=3698433

The International Max Planck Research School for Astronomy & Cosmic Physics at the University of Heidelberg (IMPRS-HD) is inviting applications for its prestigious doctoral degree program (Dr. rer. nat.) in astrophysics starting in Fall 2027.

IMPRS-HD brings together Heidelberg University's Department of Physics & Astronomy with major Max Planck Institutes to offer an elite international graduate training framework.

🔬 Program Overview & Selection Process

Structure: Admissions take place once per year with the academic program commencing each September (earlier research start dates are possible depending on project funding).

Evaluation: Applications are reviewed by an inter-institutional selection committee. Project supervisors make final project offers based on academic records, research experience, and reference letters.

📋 Candidate Profile & Qualifications

Eligibility: Open to students worldwide holding (or nearing completion of) an M.Sc. or equivalent degree in Physics, Astronomy, or a closely related STEM field.

Key Selection Criteria: Proven academic excellence, strong research background/contributions, and high-quality letters of recommendation.

📅 Key Dates & Timeline

Application Deadline: November 3, 2026, at 14:00 CET (for the academic year starting Fall 2027).

Interviews: February 1–5, 2027 (conducted in-person in Heidelberg or via Zoom; invitations sent through May 2027).

First Offer Wave: Issued immediately following the February interview week.

📩 Application Instructions

Applications must be submitted online using the "Heyflow" system. Candidates must prepare all required text, CV, transcripts, and referee contact info prior to starting the online registration process.

For more information about application, see link below

https://www.imprs-hd.mpg.de/3192/Application 

The Department of Geodesy and Geodynamics (GEOGEO) at the Finnish Geospatial Research Institute (FGI) is recruiting a doctoral student for a 4-year fixed-term position (Sept 1, 2026 – Aug 31, 2030) within the Research Council of Finland–funded GraFePor project.

The project investigates gravity variations caused by Fennoscandian Postglacial Rebound (PGR) / Glacial Isostatic Adjustment (GIA), integrating terrestrial absolute gravity and satellite gravimetry to produce a state-of-the-art gravity change rate model for Fennoscandia and North America.

🔬 Core Responsibilities & Tasks

Field Operations: Plan and execute absolute gravity measurements across Finland and Fennoscandia (1–4 week field trips).

Data Processing & Modeling: Process absolute and satellite gravimetry time series, filter non-GIA environmental mass variations, and model GIA mechanisms.

Dissemination: Present findings at international conferences and publish in peer-reviewed journals alongside the GraFePor consortium.

📋 Candidate Profile & Skills

Education: Master’s degree in Geophysics, Geodesy, Geosciences, or a closely related discipline.

Technical Requirements: Excellent programming skills (e.g., Python, MATLAB), strong scientific writing, fluent English, and a valid driving license.

Desirable Assets: Experience with terrestrial/satellite gravimetry measurements and data analysis; understanding of GIA modeling and geodetic processing; Finnish or Swedish language skills.

📅 Contract, Salary & Benefits

Duration & Work Type: 4 years full-time (Sept 2026 – Aug 2030) with partial remote work options and flexible office hours (6-month trial period).

Salary: Base monthly scale of €2,821 to €3,510 (NLS requirement levels 8–10, based on experience), plus a personal performance component (up to +45%).

Location: Kirkkonummi / Helsinki region, Finland.

📩 How to Apply

Applications must be submitted electronically via the Finnish government portal - see comment section for directory (or by post to the registry office). Include a Motivation Letter, CV, and academic transcripts/publication list.

Primary Contact: Dr. Mirjam Bilker-Koivula

Email: mirjam.bilker-koivula@maanmittauslaitos.fi 

For more information:

https://valtiolle.fi/en/jobs/phd-student-in-gravity-research-23588/

The High Energy Physics Institute (IFAE) in Barcelona, Spain, is recruiting a doctoral researcher for its Gamma-ray Group.

The position offers a dual-track PhD combining hands-on R&D for next-generation space-based gamma-ray observatories (HERD, FOCUS) with scientific data analysis from state-of-the-art ground observatories (MAGIC, CTA-LST).

🔬 Core Responsibilities & Tasks

Instrumentation R&D: Design, test, and calibrate advanced detector hardware for future space-based gamma-ray missions.

Data Analysis: Process and interpret scientific observations from current ground-based arrays (MAGIC and Cherenkov Telescope Array LSTs) to investigate high-energy astrophysical sources and fundamental physics.

Simulation & Tooling: Build reconstruction and simulation software (in Python/C++) supporting space hardware studies and data pipelines.

📋 Candidate Profile & Qualifications

Education: Master’s degree in Physics (or equivalent) by the start date, eligible for enrollment in the Physics PhD program at the Autonomous University of Barcelona (UAB).

Technical Skills: Scientific programming proficiency (Python, C++, or data analysis toolkits).

Desirable Assets: Prior experience with detector instrumentation, space hardware, or gamma-ray astrophysics.

📅 Contract, Funding & Key Dates

Duration & Salary: 4-year (48-month) full-time predoctoral contract (Investigador/a predoctoral R1), funded by the Spanish Ministry of Science & Innovation (FEDER/FSE).

Perks: Includes doctoral tuition fees and fully funded support for a 2–3 month international research stay abroad.

Start Date: Must be available to start by November 30, 2026.

Application Deadline: September 15, 2026 for full consideration (Ref: IFAE2026/35_GAMMA-RAY_PhDStudent).

📩 How to Apply

Email your Motivation Letter, CV, official Transcripts/Grades, and arrange for two reference letters to be sent directly to:

Contacts: Dr. Javier Rico (jrico@ifae.es) and HR (rrhh@ifae.es)

For more information:

https://www.ifae.es/careers/jobs/2026/07/phd-position-for-the-gamma-ray-group/ 

The Chair of Earth Observation and Remote Sensing (Prof. Irena Hajnsek) at ETH Zurich is inviting applications for a 100% full-time PhD position starting in Autumn/Winter 2026.

The project leverages multi-modal Synthetic Aperture Radar (SAR) to monitor rapid environmental shifts and climate impacts across Arctic permafrost landscapes.

🔬 Core Focus & Technical Methods

SAR Signal Processing: Developing advanced algorithms for multi-modal radar, array signal processing, and satellite remote sensing.

Arctic Climate Science: Quantifying permafrost thawing and frozen landscape dynamics using high-resolution radar imagery.

Geospatial AI: Implementing computational data pipelines for large-scale environmental monitoring.

📋 Candidate Profile

Education: Master's degree in Geomatics, Geophysics, Electrical Engineering, Physics, Remote Sensing, or Environmental Engineering.

Technical Skills: Experience in digital signal processing, image processing, or remote sensing. Strong programming skills in Python, MATLAB, C, or C++ are required.

Essentials: Excellent English fluency and a valid European Category B driver's license for potential fieldwork.

📅 Benefits & Application Process

Environment: World-class computing infrastructure, high-impact journal publishing, conference travel, public transit discounts, and competitive Swiss doctoral salary/pension.

Application Materials: Cover letter, CV, academic transcripts, Master's thesis (PDF), and contacts for two references.

Applications must be submitted exclusively via the ETH online portal (email applications are rejected).

Inquiries: Prof. Irena Hajnsek (hajnsek@ifu.baug.ethz.ch) 

For more information and how to apply:

https://agristok.net/2026/07/07/doctoral-position-earth-observation-remote-sensing-eth-zurich-2026/ 

The High-Pressure Plasmas Group at the University of Madeira (Portugal), led by Dr. Pedro Almeida, is inviting expressions of interest for PhD positions.

The research focuses on fundamental and computational challenges in low-temperature and high-pressure plasma physics, combining physical theory, numerical simulations, and experimental validation.

🔬 Research Topics

Candidates can align their doctoral research with one of the following primary lines of investigation:

Self-Organization on Liquid Electrodes in Glow Discharges in Air:

Focus: Investigating the formation, stability dynamics, and phase transitions of self-organized patterns at plasma–liquid interfaces using physical modeling, numerical simulations, and experimental comparisons.

Numerical Simulation of Gas Discharges (Corona & Gliding Arcs):

Focus: Developing 2D and 3D fluid/computational models for low-temperature, high-pressure discharges—incorporating complex plasma chemistry, non-equilibrium energy transfer, Joule heating, and plasma-fluid flow coupling.

Stability of Self-Sustained DC Discharges in Air:

Focus: Examining stationary and pulsed regimes in both positive and negative corona discharges. The scope includes theoretical modeling, simulations, experimental validation, and optional extensions into surface dielectric breakdown.

📋 Candidate Profile & Skills

Education: Master’s degree (or equivalent) in Physics, Applied Physics, or a closely related STEM field.

Core Competencies: A strong foundation in plasma physics and a motivation for theoretical, computational, or experimental research.

Desirable Assets: Proficiency in scientific programming (e.g., Python, C++, Fortran), numerical methods for partial differential equations (PDEs), or hands-on experience with plasma diagnostics.

Languages: Good command of spoken and written English.

📩 How to Submit an Expression of Interest

Interested candidates should send a brief introductory email indicating their preferred research topic, accompanied by a CV or a concise summary of their academic background, directly to the group lead:

Contact: Dr. Pedro Almeida

Research Group: High-Pressure Plasmas Group, University of Madeira

Email: pedroja@staff.uma.pt  

For more information:

https://fisica.uma.pt/phd_positions.html#topics

For more information:

https://www.unitn.it/sites/default/files/2026-06/SST_Call_42_ENG.pdf 

Driven by the explosive growth of satellite mega-constellations, the global in-space servicing, assembly, and manufacturing (ISAM) market is accelerating rapidly—with the in-orbit refueling sector projected to reach a valuation of USD $1.1 billion by 2032.

Under the supervision of Dr. Priyanka Dhopade, this PhD project focuses on solving one of the most complex engineering hurdles in modern space logistics:

understanding and modeling liquid propellant behavior in zero gravity to enable the design of next-generation, sustainable fuel transfer systems.

🔬 Core Scientific Goals & Technical Scope

Because large-scale fluid transfer has not yet been routinely executed in microgravity environments, this project bridges fundamental fluid mechanics and aerospace engineering to create the foundation for orbital fuel stations:

Microgravity Fluid Mechanics: Investigating surface tension, capillary action, and sloshing dynamics in low-gravity environments, where traditional gravity-driven fluid management fails.

Computational Modeling: Leveraging computational fluid dynamics (CFD) and numerical simulations to predict how liquid propellants move, settle, and transfer between pressurized tanks in orbit.

System Optimization: Designing robust thermodynamic and physical transfer mechanisms to minimize boil-off, prevent bubble formation, and ensure safe, efficient refueling loops for deep-space and near-Earth assets.

📋 Candidate Profile

This interdisciplinary project operates at the cutting edge of space sustainability and fluid engineering. It is an ideal fit for a student holding a degree in:

Aerospace / Mechanical Engineering: With an interest in fluid systems, propulsion, thermodynamics, or orbital mechanics.

Physics / Applied Mathematics: Particularly those with a background in continuum mechanics, computational fluid dynamics (CFD), or microgravity physics.

Computational Data Science: Strong programming skills (such as Python, C++, or MATLAB) for handling complex physics engines or simulation pipelines.

📅 The Research Environment & Industry Impact

You will join a forward-looking research framework dedicated to long-term space environmentalism and hardware reliability. The project offers specialized training in:

Advanced CFD tools and multiphase flow modeling techniques.

Spacecraft subsystem engineering and thermodynamic control structures.

High-performance computing (HPC) for complex microgravity simulations.

📩 How to Apply & Inquiries

Interested candidates are highly encouraged to contact the supervisor directly to discuss project scope, application procedures, and institutional funding opportunities.

Primary Supervisor: Dr. Priyanka Dhopade  

For more information:

https://www.ssi.org.nz/current-opportunities 

An exciting PhD project is available to investigate the atmospheric impacts of space debris re-entry, focusing on how hundreds of tons of metallic vapor and vaporized satellite particles disperse in the upper atmosphere.

Under the supervisory team of Annika Seppälä (expert in atmospheric physics and solar-terrestrial coupling) and Priyanka Dhopade (expert in aerospace engineering and thermodynamics), this research aims to model atmospheric transport dynamics to evaluate potential threats to the recovery of the ozone layer.

🔬 Core Scientific Goals

The rapid expansion of satellite constellations means atmospheric re-entry of retired spacecraft is surging. This project addresses the long-term physical and chemical consequences of this metallic injection:

Transport Modeling: Developing and utilizing high-altitude atmospheric dynamics models to trace how vaporized satellite materials (such as aluminum oxides) are transported from the mesosphere down into the stratosphere.

Ozone Chemistry Impacts: Evaluating how these particulate distributions interact with stratospheric chemistry, potentially accelerating ozone depletion pathways.

Policy & Mitigation: Providing quantitative recommendations for international space traffic management, sustainable satellite design, and end-of-life deorbit mitigation strategies.

📋 Candidate Profile

This interdisciplinary project bridges aeronomy, fluid dynamics, and environmental science. It is highly suited for a student with a strong background in:

Physics / Geophysics / Meteorology: Particularly those interested in atmospheric modeling, fluid dynamics, or upper-atmospheric chemistry.

Aerospace Engineering: With an interest in orbital re-entry dynamics, aerothermodynamics, or planetary atmospheres.

Computational Science / Applied Mathematics: Strong programming skills (ideally Python, Fortran, or MATLAB) for handling complex climate, chemical transport, or fluid models.

📅 The Research Environment

You will be embedded in a highly collaborative research environment working at the intersection of atmospheric physics and aerospace engineering. The project provides comprehensive training in:

Global atmospheric circulation and chemical transport models.

The physics of the middle and upper atmosphere (stratosphere, mesosphere, thermosphere).

High-performance scientific computing and big data analysis.

📩 How to Apply & Inquiries

Interested candidates should reach out to the supervisory team for informal inquiries, project timelines, and funding availability prior to submitting a formal application.

Primary Contact: Associate Professor Annika Seppälä

Co-Supervisor: Dr. Priyanka Dhopade 

For more information:

https://www.ssi.org.nz/current-opportunities 

Prof. Sean Elvidge’s research group at the University of Birmingham is inviting applications for a PhD studentship at the intersection of space weather physics and global engineering infrastructure.

Global Navigation Satellite Systems (GNSS) like GPS and Galileo are central to modern infrastructure but must pass through the ionosphere; a highly dynamic, charged atmospheric layer.

Volatile space weather events drive variations in Total Electron Content (TEC), scintillation, and Traveling Ionospheric Disturbances (TIDs) that delay and disrupt these critical signals.

This project will develop advanced models to predict, nowcast, and mitigate these errors to protect high-precision Positioning, Navigation, and Timing (PNT) services.

🔬 Technical Scope & Methods

The research will address how high-precision protocols like Precise Point Positioning (PPP) degrade during severe geomagnetic storms. Potential avenues include:

Precision Corrections: Designing advanced regional or global ionospheric corrections that maintain high fidelity during intense solar storms.

Uncertainty Quantification: Building statistical models that dynamically quantify uncertainty to warn safety-critical users (e.g., aviation, autonomous transport) of system degradation.

Data-Driven Frameworks: Ingesting large-scale satellite datasets using data assimilation, statistical learning, and signal processing.

📋 Candidate Profile

This position is highly suited for a quantitative student holding a degree in Physics, Geophysics, Mathematics, Data Science, or Engineering.

You will receive rigorous training in scientific computing, ionospheric physics, and big data analytics. Prior GNSS experience is useful but not essential; curiosity and mathematical ability are prioritized.

📩 How to Apply

Candidates must submit an informal inquiry to the Principal Investigator before initiating a formal university application.

Contact: Prof. Sean Elvidge

Email: s.elvidge@bham.ac.uk 

For more information, visit:

https://www.findaphd.com/phds/project/ionospheric-auroral-and-ocean-clutter-models-for-monostatic-and-bistatic-hf-sensing-systems/?p197504

An exceptional PhD studentship is available within a multidisciplinary research group led by Prof. Sean Elvidge at the University of Birmingham. The project operates at the vibrant interface of space weather science, radio engineering, and operational systems to pioneer the future of High-Frequency (HF) over-the-horizon sensing.

🔬 The Research Challenge & Technical Scope

This PhD project focuses on modeling, predicting, and mitigating environmental clutter for both co-located (monostatic) and separated/networked (bistatic) HF configurations.

Key research avenues include:

Ionospheric & Auroral Clutter Modeling,

Ocean Clutter Modeling, and

Experimental Validation.

Depending on your core technical strengths, the workflow can easily flex to prioritize ray tracing, signal processing, numerical scattering simulation, statistical characterization, machine learning for clutter classification, or real-time data assimilation using ionospheric data pipelines.

📋 Candidate Profile

This project is highly suited for an analytically minded student holding (or completing) a degree in:

Physics / Geophysics (particularly space plasma physics, aeronomy, or ionospheric dynamics). Engineering / Signal Processing (radio frequency engineering or computational wave propagation).

Applied Mathematics / Computational Modeling.

Key Skills You Will Gain: Comprehensive training in scientific programming, advanced HF sensing, space environment forecasting architectures, and the structural analysis of massive, multi-dimensional experimental datasets.

📅 Collaboration & Impact

Environment: You will join a highly collaborative, international network bridging fundamental physical principles with high-impact defense and space domain awareness applications.

Outcomes: Your research tools will directly guide next-generation networked sensing layouts, helping predict how geomagnetic storms affect target detectability on any given day.

📩 How to Apply

Prior to submitting a formal application through the university admissions portal, candidates are required to submit an informal expression of interest directly to the Principal Investigator.

For more details on this role, see link:

https://www.findaphd.com/phds/project/ionospheric-auroral-and-ocean-clutter-models-for-monostatic-and-bistatic-hf-sensing-systems/?p197504 

Contact: Prof. Sean Elvidge

Email: s.elvidge@bham.ac.uk 

The Department of Technology Systems at the University of Oslo (UiO) is inviting applications for a 3-year PhD Research Fellowship in Space Science, based at the Space Systems group in Kjeller, Lillestrøm.

🔬 Research Avenues

• The specific research direction is flexible and can be tailored to the candidate's background:

• The Martian Water Cycle

• Space Weather Atmospheric Impacts

• Martian Aurora

📋 Candidate Profile & Skills

Required Qualifications:

A Master’s degree (or equivalent 4-year foreign degree) in Physics, Planetary Science, Meteorology, Geophysics, or a similar field, defended before the autumn start date.

Proven programming experience in Python, specifically tailored for scientific data processing and analysis.

Fluency in oral and written English.

Academic Excellence: Equivalent to a minimum average grade of C for the Bachelor's degree, and a minimum average grade of B (including a grade of B or better for the thesis) for the Master's degree in the Norwegian system.

Desired Assets:

Knowledge of atmospheric or space physics.

Prior experience with spectroscopic data analysis, remote sensing, or planetary science datasets.

📅 Contract, Salary & Timeline

Duration: 3 years full-time. A 4th year may be considered, which includes 25% career-promoting work (teaching or research assistance).

Salary: Position code 1017, ranging from NOK 550,800 to 595,000 per annum (subject to a 2% statutory contribution deduction to the State Pension Fund).

Perks: Membership in the Statens Pens Pensjonskasse (excellent pension, mortgage, and insurance benefits), 1.5 hours of paid exercise time per week, and family-friendly surroundings.

Starting Date: Preferred Autumn 2026.

Security: Candidates must successfully clear national export control, sanctions, and security checks.

📩 How to Apply

• Applications must be submitted via the electronic Jobbnorge portal. Your package must include:

• A Cover Letter detailing your motivation and research interests.

• A full CV (listing education, positions, and any scientific publications).

• Certified transcripts and diplomas for both Bachelor's and Master's degrees (with an official explanation of your university's grading scale for foreign applicants).

• Letters of recommendation along with contact data for 2–3 professional references.

• Documentation of English proficiency (if applicable).

For more details, see link:

https://www.jobbnorge.no/en/available-jobs/job/303704/phd-research-fellow-in-mars-atmospheric-science

The Graduate Program in Electrical and Computer Engineering (Pós-graduação em Engenharia Elétrica e Computação) at Universidade Presbiteriana Mackenzie in São Paulo, Brazil, is inviting international applications for a fully funded PhD scholarship.

This opportunity is perfect for researchers looking to work at the intersection of solar physics, upper atmospheric science, and instrumentation.

🔬 Core Research Themes

• Candidates will have the opportunity to align their doctoral thesis with several active, high-impact research areas:

• Solar & Stellar Activity: Investigating solar flares, stellar atmospheric dynamics, and flaring mechanisms.

• Ionosphere / VLF (Very Low Frequency): Analyzing upper atmospheric physics, D-region ionospheric disturbances, and wave propagation.

• Space Geodesy: Utilizing space-based geodetic techniques to study Earth's shape, orientation, and gravity field variations.

• Radio Telescope Design & Operations:

• Developing, calibrating, and managing cutting-edge instrumentation for radio astronomy and solar observations.

📋 Candidate Profile & Eligibility

• Target Audience: International applicants holding (or close to completing) a Master’s degree in Physics, Astronomy, Space Geophysics, Electrical Engineering, or a related field.

• Core Competencies: A strong motivation for space science data analysis, numerical modeling, or radio hardware engineering.

📅 Application Mechanics

• The selection process is organized in partnership with the GCUB (Grupo de Cooperação Internacional de Universidades Brasileiras) mobility framework.

• Official Program Guidelines: Comprehensive application rules, language parameters, and document requirements can be reviewed directly via the GCUB Call for Applications Portal.

• Review Status: The call was published on June 14, 2026, and is actively accepting international portfolios.

📩 How to Apply & Inquiries

• For scientific inquiries regarding research infrastructure, prospective advisors, or laboratory capabilities, you can contact Dr. Paulo Simões directly:

Email: paulo.simoes@mackenzie.br 

The Division of Geodesy and Geoinformatics at KTH Royal Institute of Technology in Stockholm, Sweden, invites applications for a 100% full-time PhD position in Artificial Intelligence for Earth Observation. This doctoral research will focus on advancing AI-driven Earth Observation (EO) methods for environmental intelligence.

🔬 Research Themes & Tasks

The selected candidate will explore cutting-edge AI and machine learning approaches to analyze multi-modal, multi-temporal, and multi-resolution satellite imagery alongside geospatial data.

📋 Candidate Profile

Admission Requirements:

Education: A Master's degree in Geomatics, Computer Science, Electrical Engineering, or related natural sciences/engineering disciplines. Must meet standard basic eligibility for Swedish postgraduate education.

Core Skills: Strong proficiency in image analysis, computer vision, pattern recognition, and machine learning/deep learning, backed by a solid data science background.

Programming & Languages: Proficient coding skills in Python, C++, and Matlab. Candidates must demonstrate fluent spoken English and excellent scientific reading/writing skills, fulfilling the mandatory English B/6 requirement.

Assets: Prior experience working with generative AI or geospatial foundation models is highly valued.

📅 Contract, Benefits & Timeline

Location: KTH Campus, Stockholm, Sweden.

Duration: The position is for a maximum 4-year full-time equivalent doctoral contract, structured to target a Licentiate degree within an initial two-year employment period. Contracts are renewed sequentially. Up to 20% of the role may include training or departmental administration.

Compensation: Monthly salary paid in accordance with KTH’s official Doctoral student salary agreement, featuring extensive employee benefits.

Application Deadline: July 9, 2026 (Midnight CEST).

📩 How to Apply

• Applications must be submitted electronically through the KTH recruitment system under reference number PA-2026-1857. Your complete application portfolio must include:

• Certified copies of diplomas, transcripts, and official language certificates (with English or Swedish translations if necessary).

• A comprehensive CV detailing professional and academic experience.

• An application letter (maximum 2 pages) describing your academic interests, motivation, and how they relate to your future goals.

• Representative publications or technical reports (with abstracts and links for longer documents).

For scientific or administrative questions, contact Prof. Yifang Ban directly at yifang@kth.se.

For more information:

https://www.kth.se/lediga-jobb/938749?l=en

The Space Research Centre of the Polish Academy of Sciences (CBK PAN) in Warsaw is inviting applications for a 4-year PhD position. Funded by the National Science Centre, Poland (NCN) under the SONATA BIS-15 call, the project is titled "The Subparsec Structure of the Local Interstellar Medium" and is led by Dr. Paweł Swaczyna.

This unique project challenges the prevailing paradigm of our local space environment by using interstellar neutral atom data from NASA missions to map the boundary interactions right outside our solar system.

🔬 The Research Challenge & Tasks

Astrophysical data shows that our solar system is currently sitting inside an interaction zone between two warm interstellar clouds moving at different velocities. As a PhD student, you will look for structural signatures of this cloud-cloud interaction by doing the Mission Data Analysis, Computational Modeling, Dissemination

📋 Candidate Profile

• Education: Master’s degree in Physics, Astronomy, Mathematics, or a related field with coursework in statistics or data analysis. Candidates nearing graduation may apply with an advisor's letter stating an expected graduation date before the doctoral program begins.

• Technical Skills: Solid knowledge of at least one programming language: Python, C/C++, or Mathematica.

• Language & Spirit: Good command of English for scientific writing and international team collaboration. Full motivation to engage with the project tasks and a readiness to enroll in the GeoPlanet Doctoral School.

📅 Details, Funding & Location

Location: In person at the CBK PAN headquarters in Warsaw, Poland.

Scholarship Funding: 5,000 PLN per month for up to 48 months.

💰 Financial Note: This NCN research project scholarship is separate from and additional to the standard doctoral stipend provided by the GeoPlanet Doctoral School.

Important Dates:

Application Deadline: 15 June 2026.

Results Announced: By 27 July 2026.

Start Date: 1 October 2026.

📩 How to Apply

Applications must be submitted via the GeoPlanet Doctoral School recruitment portal. During submission, candidates must explicitly select the project topic: "Searching for the subparsec structure of the local interstellar medium surrounding the Sun in observations from the IBEX and IMAP missions".

Note for international applicants: It is highly recommended to include a general recognition statement from the NAWA Qualification Tool to verify your diploma eligibility.

For specific questions regarding the project science, contact Dr. Paweł Swaczyna at pswaczyna@cbk.waw.pl.

The Space Research Laboratory (SRL) within the Department of Physics and Astronomy at the University of Turku, Finland, is inviting applications for a three-year, fixed-term research position. The role can be appointed at the level of Doctoral Researcher, Project Researcher, or Research Assistant, depending on the candidate's current academic qualifications.

The successful applicant will join the AIPAD project (Artificial Intelligence for Solar Energetic Particle Pitch-Angle Distributions), a multidisciplinary initiative funded by the Research Council of Finland. Led by Dr. Nina Dresing, the project is run in close collaboration with the Algorithmics and Computational Intelligence research group at the university's Department of Computing.

🔬 The Research Framework: AIPAD

Solar energetic particle (SEP) events triggered by explosive solar eruptions pose severe radiation hazards to technological infrastructure, GPS systems, and astronauts.

A major puzzle in space weather physics is distinguishing the relative contributions of solar flares versus coronal shocks in accelerating these particles.

The AIPAD project tackles this challenge by merging space physics with computer science: Data Analysis, Machine Learning Integration.

📋 Role Tiering & Candidate Requirements

The position is highly flexible and accommodates candidates at different stages of their early research career:

1. Research Assistant

2. Project Researcher

3. Doctoral Researcher

Fluency in English (matching the mandatory English proficiency criteria required by the University of Turku Graduate School).

📅 Location, Timeline & Terms

Location: Turku, Finland (On-site working in Finland is required).

Duration: 3 years, fixed-term.

Application Window: Applications open 26 May 2026 and close 10 July 2026 at 16:00 (Europe/Helsinki time).

📩 How to Apply

Candidates must submit their applications through the University of Turku's electronic recruitment portal before the July deadline.

Prior to applying, international candidates are strongly encouraged to review the student information, language requirements, and application criteria detailed on the EXACTUS Doctoral Programme portal.

For more information and how to apply:

https://ats.talentadore.com/apply/doctoral-researcher-project-researcher-research-assistant-fixed-term-position-in-space-physics/ZvnwA3?UTUID=21513

Are you passionate about space autonomy? The GNC Lab of the University of Naples Federico II is recruiting!

Focus: Guidance, Navigation, and Control for proximity ops.

Applications: Servicing, Debris Removal, and Deep Space Exploration.

Partnership: Work alongside CIRA and spend 6 months at a top international research center.

⏳ Deadline: April 8, 2026 (13:00 Italian Time).

for more information,see link

https://www.dii.unina.it/source/dottorato/ciclo-41/IngInd_Borsa29.pdf 

Are you passionate about space autonomy? The GNC Lab of the University of Naples Federico II is recruiting!

Focus: Guidance, Navigation, and Control for proximity ops.

Applications: Servicing, Debris Removal, and Deep Space Exploration.

Partnership: Work alongside CIRA and spend 6 months at a top international research center.

⏳ Deadline: April 8, 2026 (13:00 Italian Time).

for more information,see link

https://www.dii.unina.it/source/dottorato/ciclo-41/IngInd_Borsa29.pdf 

Are you ready to push the boundaries of our understanding of the Sun, stars, and space weather? The School of Aerospace at HIT Shenzhen is looking for highly motivated PhD students to join a world-class research team working at the frontier of solar and space science.

About the Research

You’ll work across five cutting-edge areas: physics of solar and stellar coronae, flares, and CMEs; space weather impacts on Earth’s magnetosphere and exoplanet habitability; socioeconomic consequences of space weather; high-resolution numerical simulations of solar and stellar atmospheres; and AI and machine learning applied to large observational and simulation datasets. Whether your strength is in theory, computation, observation, or AI — there’s a place for you here.

Who We’re Looking For

A Master’s degree in physics, astrophysics, plasma physics, applied mathematics, computational physics, or a related field. Programming experience in Python, Fortran, or C++ is highly desirable, and prior ML or data science experience is a strong plus. Strong English communication skills and a genuine passion for research are essential.

What We Offer

A fully funded position with a competitive stipend and full tuition waiver, state-of-the-art computational facilities, and international collaboration opportunities spanning space weather to lunar and Mars missions — all based in vibrant, sunny Shenzhen, China’s Silicon Valley.

📅 Application Deadline: May 20, 2026

🎓 Expected Start: September 2026

📩 Send your CV, cover letter, transcripts, two referee contacts, and an optional research proposal to yuanding@hit.edu.cn — subject: “HITSZ PhD Application – Aerospace Science.” 

The High-Resolution Weather and Climate Modeling Group at the ETH Zurich (Institute for Atmospheric and Climate Sciences, IAC) is recruiting a PhD student for a Swiss National Science Foundation (SNSF)–funded Ambizione project.

📅 Start date: Between May 1 and September 1, 2026

🗓 Application deadline: March 14, 2026 (applications before March 15 receive full consideration)

Supervision by Monika Feldmann and Andreas Prein.

🌩 Project Overview

Severe thunderstorms are a major source of weather-related damage, particularly near mountain ranges, where climate change signals appear amplified.

This PhD focuses on idealized high-resolution numerical modeling to isolate and understand the physical drivers of enhanced climate trends over mountains.

Project partners include:

• MeteoSwiss

• Pennsylvania State University

• European Severe Storms Laboratory

The position includes funding for international research visits and participation in a planned field campaign.

🧪 Research Tasks

The PhD candidate will:

• Analyze observational datasets to identify typical thunderstorm events

• Analyze climate model outputs to assess systematic environmental changes

• Derive representative, idealized initial conditions

• Design and run simulations with ICON

• Study impacts of topography and climate change on storm dynamics

• Collaborate internationally in data exchange and modeling

• Present findings at conferences and to broader audiences

• Publish peer-reviewed articles

🎓 Profile

Required

• Master’s degree in meteorology, climate science, physics, or related field

• Programming experience in data analysis and visualization

Desired

• Experience in severe thunderstorm dynamics or numerical modeling

• Familiarity with Linux and HPC clusters

• Python programming experience

• Strong interest in extreme weather phenomena

🌍 What ETH Zurich Offers

• Fully funded SNSF Ambizione PhD position

• Access to state-of-the-art HPC systems for high-resolution ICON simulations

• Close supervision in an interactive research environment

• Strong national and international collaborations

• Funding for research stays abroad & field campaign participation

• Support for publications and conference presentations

• Competitive salary per ETH Zurich regulations

• Inclusive, diverse, and sustainability-focused working culture

📄 Application Details

Submit your online application by March 14, 2026, including:

• Motivation letter

• CV

• MSc transcripts

• Contact details of three references

📧 Scientific inquiries: monika.feldmann@unibe.ch (no applications via email) 

Are you interested in astrochemistry, dust formation, and computational modelling? Here’s an exciting PhD opportunity at University College Dublin within an ERC Starting Grant project.

The School of Physics at UCD invites applications for a PhD position in computational astrochemistry, supervised by Dr Marie Van de Sande, as part of the ERC Starting Grant ASHES, which focuses on dust formation in the outflows of asymptotic giant branch (AGB) stars.

🌌 Why this matters

Most stars pass through the AGB phase near the end of their lives, ejecting material that enriches the interstellar medium—the raw material for future stars and planets. These stellar outflows are driven by dust formation, yet the detailed chemistry behind this process remains poorly understood. This PhD aims to help solve that puzzle.

🔬 What you’ll work on

• Extending large chemical reaction networks to include dust nucleation

• Using results from quantum chemical calculations

• Developing the first 1D bottom-up dust growth models

• Advancing to 3D chemical models by post-processing hydrodynamical simulations

• Bridging the gap between theory and observations

💻 Ideal background

• Degree in chemistry, physics, or astronomy

• Interest in chemical kinetics modelling

• Motivation to build skills in Python, Fortran, data analysis, and visualisation

✈️ What’s included

As part of the ERC ASHES project, you’ll have strong support for conferences, workshops, and international research visits, working in a vibrant and collaborative research environment.

📄 How to apply

Send the following to mvdsande@strw.leidenuniv.nl by 15 March 2026:

• CV (education, skills, expertise)

• One-page motivation letter

• Names and contact details of two referees

📩 Enquiries

Dr Marie Van de Sande

✉️ mvdsande@strw.leidenuniv.nl

If you’re passionate about astrochemistry, stellar evolution, and computational science, this is a fantastic opportunity to join a cutting-edge ERC-funded project.

The Space Research Laboratory (SRL) within the Department of Physics and Astronomy at the University of Turku, Finland, is inviting applications for a three-year, fixed-term research position. The role can be appointed at the level of Doctoral Researcher, Project Researcher, or Research Assistant, depending on the candidate's current academic qualifications.

The successful applicant will join the AIPAD project (Artificial Intelligence for Solar Energetic Particle Pitch-Angle Distributions), a multidisciplinary initiative funded by the Research Council of Finland. Led by Dr. Nina Dresing, the project is run in close collaboration with the Algorithmics and Computational Intelligence research group at the university's Department of Computing.

🔬 The Research Framework: AIPAD

Solar energetic particle (SEP) events triggered by explosive solar eruptions pose severe radiation hazards to technological infrastructure, GPS systems, and astronauts.

A major puzzle in space weather physics is distinguishing the relative contributions of solar flares versus coronal shocks in accelerating these particles.

The AIPAD project tackles this challenge by merging space physics with computer science: Data Analysis, Machine Learning Integration.

📋 Role Tiering & Candidate Requirements

The position is highly flexible and accommodates candidates at different stages of their early research career:

1. Research Assistant

2. Project Researcher

3. Doctoral Researcher

Fluency in English (matching the mandatory English proficiency criteria required by the University of Turku Graduate School).

📅 Location, Timeline & Terms

Location: Turku, Finland (On-site working in Finland is required).

Duration: 3 years, fixed-term.

Application Window: Applications open 26 May 2026 and close 10 July 2026 at 16:00 (Europe/Helsinki time).

📩 How to Apply

Candidates must submit their applications through the University of Turku's electronic recruitment portal before the July deadline.

Prior to applying, international candidates are strongly encouraged to review the student information, language requirements, and application criteria detailed on the EXACTUS Doctoral Programme portal.

For more information and how to apply, see link below

https://ats.talentadore.com/apply/doctoral-researcher-project-researcher-research-assistant-fixed-term-position-in-space-physics/ZvnwA3?UTUID=21513

Are you passionate about uncovering the mysteries of our closest star?

Dr. Susanna Parenti (Paris-Saclay) and Prof. Andrew Hillier (Exeter) are seeking a motivated PhD candidate for a unique joint position between the University of Exeter and Université Paris-Saclay.

🔬 The Project

This research focuses on the modelling and observations of the chromospheric response to solar flares. This is a fantastic opportunity to work at the intersection of theoretical modeling and high-level solar observation within two world-class institutions.

📅 Key Details

Topic: Solar Physics / Chromospheric Flares

Location: Dual placement in the UK and France

Deadline: 22nd March 2026

For Full Details & Application: See link below

http://uksolphys.org/studentships/joint-phd-in-solar-physics-at-exeter-paris-saclay/

Start: As soon as possible

Duration: Initially 3 years

Salary: EG 13 TV-L (≈ €43,500/year)

Location: Kühlungsborn, Germany (with campaigns at ALOMAR, Norway)

We invite applications for a research position focused on optical remote sensing of the middle atmosphere (mesosphere & lower thermosphere). The role is part of AMILIS (Anthropogenic Material Influx Lidar Study), funded by the German Aerospace Center (DLR), investigating metal atoms and aerosols linked to space-debris re-entry.

🔬 Your Research

• Optical/quantum remote sensing of atoms in the MLT

• Set up and operate a multi-metal lidar

• Hands-on optics & laser work (spectroscopy, dye lasers, laser physics)

• Software development for lidar control

• Data analysis to separate natural variability from anthropogenic effects

• Night/weekend lidar soundings (per regulations)

🎓 Your Profile

• Master’s degree in physics, engineering, environmental sciences, or related

• Initial experience with experimental methods (e.g., spectroscopy, lasers)

• Programming skills (Python, Julia, C/C++)

• Strong communication and teamwork skills

• Independent, hands-on researcher mindset

🌍 What We Offer

• Attractive workplace near the Baltic Sea

• World-leading lidar systems & modern facilities

• International research environment

• VBL pension, flexible hours, mobile work options

• Family-friendly policies & equality of opportunity

• Part of the Leibniz Association, closely linked with the University of Rostock

📝 How to Apply

Submit one PDF including:

• Motivation letter

• CV

• Diploma (final grade)

• Certificates/references (if available)

📌 Open until filled (travel costs not covered)

Contact and application: 

Prof. Dr. Gerd Baumgarten

Email: baumgarten@iap-kbom.de

♿ Equal Opportunities

Women are explicitly encouraged to apply. Applicants with disabilities receive preference with equal qualifications. 

Offered through BEST — Between Earth and Sky in Toulouse (co-funded by the EU's Marie Skłodowska-Curie Actions COFUND scheme), this fully funded PhD position focuses on developing an intermediate-fidelity stochastic model of Earth's orbital environment. Supervised by Prof. Joan-Pau Sánchez Cuartielles, the project will establish quantitative orbital footprint indicators to guide early mission architectures, constellation geometries, collision avoidance strategies, and post-mission disposal options.

🔬 Research Objectives & Scope

Stochastic Environment Modeling: Construct a stochastic model capable of evaluating long-term orbital degradation as a finite shared resource.

Architectural & Operational Trade-offs: Quantify the long-term impact of spacecraft reliability, fragmentation risk, active debris removal, and maneuvering capabilities on orbital sustainability.

Life Cycle & Sustainability Metrics: Extend traditional Earth-centered Life Cycle Assessment (LCA) methods to incorporate long-term orbital footprint metrics.

📋 Candidate Eligibility & Rules

Academic Requirements: Must hold a Master’s degree (or equivalent diploma) by the call deadline and must not already hold a doctoral degree.

MSCA Mobility Rule: Applicants must not have resided or carried out their main activity (work, studies, etc.) in France for more than 12 months in the 36 months immediately preceding the call deadline (November 23, 2026).

Interdisciplinary & Mobility Requirements: Includes mandatory international mobility and co-supervision with an international partner institution.

💼 What the BEST Program Offers

Funding: Fully funded 3-year PhD contract under standard EU MSCA COFUND conditions.

Mobility & Development: Dedicated funding for mandatory international mobility, specialized training, and career development activities within an international doctoral community.

📅 Key Application Dates & Contacts

Application Deadline: November 23, 2026 at 12:00 PM CET

Application Portal: edd-projets.utoulouse.fr

Project Reference ID: Proposal #76117 (https://lnkd.in/gZSz7TBQ)

Inquiries:

Research & Academic Inquiries: Prof. Joan-Pau Sánchez (joan-pau.sanchez@isae-supaero.fr)

Eligibility & Administrative Inquiries: BEST Helpdesk (best-helpdesk@utoulouse.fr)

The Cooperative Institute for Satellite Earth System Studies (CISESS) within the Earth System Science Interdisciplinary Center (ESSIC) at the University of Maryland, College Park is hiring a scientist in satellite remote sensing of precipitation and clouds.

Depending on qualifications and degree level, the position title will be appointed as Faculty Specialist (M.S. required), Postdoctoral Associate, or Assistant Research Scientist (Ph.D. required).

🔬 Core Responsibilities & Active Research Directions

Algorithm Development: Develop, train, and evaluate machine learning models (e.g., PyTorch, TensorFlow) for geophysical retrievals across passive microwave, infrared, and visible tropospheric satellite observations.

Dataset Engineering: Construct and maintain collocated datasets spanning multi-sensor spaceborne platforms and ground-based references.

Validation & Uncertainty: Validate precipitation and cloud property retrievals against weather radar/ground sensors and quantify retrieval uncertainties or unobserved direct quantities.

Interagency Collaboration: Work closely in an interdisciplinary team partnering with NOAA and NASA.

📋 Candidate Qualifications

Required:

Education: Ph.D. in Atmospheric Science, Hydrology, Environmental Science, or a related field; OR M.S./Ph.D. in Computer Science with demonstrated experience applying ML to scientific problems.

Programming & ML: Strong Python skills and practical experience training machine learning models using frameworks such as PyTorch or TensorFlow.

Domain Knowledge: Working understanding of tropospheric satellite observations across passive microwave, IR, and visible spectra.

Eligibility: U.S. Citizenship, Green Card holder, or applicant from a non-designated country (due to facility access requirements).

Desirable:

Experience with satellite/ground precipitation estimation, weather radar validation, multi-sensor collocation, uncertainty quantification, or GPU-based large-scale model training.

💼 Position Details & Timeline

Duty Station: ESSIC, College Park, MD (On-site/Hybrid workspace).

Appointment: 1-year initial appointment with potential for renewal based on performance and funding.

Salary: Commensurate with qualifications and experience.

Review Date: Application review begins September 30, 2026 (open until filled).

📩 How to Apply

Applications must be submitted via the UMD Online Survey Application Form:

[https://lnkd.in/g8UDiXfA)

Required Attachments:

Curriculum Vitae (CV)

Cover Letter: Brief statement (half a page) detailing how your background fits the requirements.

Inquiries Contact: Dr. Veljko Petkovic (veljko.petkovic@umd.edu) 

The Independent Safety Office at the European Space Research and Technology Centre (ESTEC) in Noordwijk, Netherlands is recruiting an Internal Research Fellow (PostDoc) to evaluate policy options, risk metrics, and regulatory frameworks supporting ESA's Zero Debris initiative.

The Fellow will conduct multidisciplinary, theoretical research to stress-test debris mitigation requirements and model incentive structures (e.g., tradable quotas, insurance premiums) under evolving technological landscapes.

🔬 Research Scope & Core Tasks

Compliance Analysis: Review outcomes of ESA project reviews since the Zero Debris initiative was introduced, identifying feasibility and verification challenges.

Technological Roadmaps & Scenarios: Analyze lessons learned from ESA R&D activities, consult domain experts, and formulate future scenarios incorporating technology roadmaps (e.g., ESA Vision 2040).

Policy & Regulatory Frameworks: Perform comparative analyses of regulation in analogous sectors (e.g., fisheries, EU AI Act, Zero Deforestation targets) to evaluate transferability of tools like cap-and-trade schemes and orbital zoning.

Incentive Structures: Model the uptake and impact of mitigation incentives (e.g., tradable debris quotas) across different space actors and jurisdictions.

📋 Candidate Profile & Qualifications

Education:

Completed within the past 5 years, or close to completing, a Ph.D. in Aerospace Engineering, Mathematics, Physics, Computer Science, or a related field.

A Ph.D. in Space Policy or Space Law is also considered if research included quantitative/numerical approaches.

Technical Skills & Requirements:

Knowledge of space debris mitigation approaches, guidelines, and regulations.

Familiarity with computational tools (e.g., Python).

Strong research/publication record and capability for autonomous research.

Proficiency in English or French (knowledge of another ESA Member State language is an asset).

Nationality Eligibility:

Candidates must be nationals of an ESA Member State, Associate Member State, or Cooperating State (including Canada).

📅 Key Application Details & Required Documents

Job Requisition ID: 20888

Posting Date: September 10, 2026

Closing Date: October 1, 2026 at 23:59 CEST

Grade Band: F2 - F2 (Internal Research Fellow)

Location: ESTEC, Noordwijk, Netherlands

📩 How to Apply

Applications must be submitted online via the ESA Careers Portal. Required submission materials:

Curriculum Vitae (CV)

Motivation Letter

Research Proposal (max 5 pages, uploaded under "Additional Documents" in the application information section)

For more information and how to apply:

https://jobs.esa.int/job/Noordwijk-Internal-Research-Fellow-%28PostDoc%29-inSpace-Debris-Mitigation/1435899133/  

The Rosseland Centre for Solar Physics (RoCS) at the Institute of Theoretical Astrophysics (ITA), University of Oslo (Blindern, Oslo, Norway), is hiring a Researcher for a 2-year position under the Research Council of Norway FRIPRO project “MultiSCORE: Multi-scale structure of the coronal environment”, led by Petra Kohutova.

The project investigates large- and small-scale structures in the solar corona by combining multi-vantage-point spaceborne observations (Solar Orbiter and SDO) with numerical models and magnetic field extrapolations.

🔬 Core Responsibilities & Scientific Scope

Observational Analysis: Analyze fine-scale coronal structures using Solar Orbiter/EUI imaging and SPICE spectroscopic data.

3D Reconstruction: Reconstruct three-dimensional active region structures by combining multi-vantage-point data from Solar Orbiter and SDO/AIA with magnetic field extrapolation constraints.

Model Validation: Compare observational results and 3D reconstructions against synthetic observables derived from numerical simulations.

Dissemination & Outreach: Publish in peer-reviewed scientific journals, present at astrophysics/solar physics conferences, and participate in departmental outreach activities.

📋 Key Qualifications & Required Skills

Required:

Education: PhD degree (approved thesis and defense completed) in Solar Physics, Astrophysics, or a closely related discipline.

Data Analysis: Demonstrated experience analyzing Solar Orbiter dataset tools and instruments.

Programming: Proficiency in Python, IDL, or Julia.

Language: Fluent oral and written communication skills in English.

Security: Must be security-eligible under the Norwegian Security Act (background checks may apply).

Desired:

Experience with scaling and intermittency analysis techniques applied to solar/space plasma observations or simulations.

Hands-on experience with coronal magnetic field extrapolation methods.

💼 Compensation & Position Details

Duration: 2 years (Full-time, located at Blindern, Oslo).

Start Date: Flexible between January 1, 2027, and October 1, 2027.

Salary Range: NOK 595,000 – 690,000 / year (Position code 1109), minus 2% statutory contribution to the State Pension Fund.

Benefits: Public pension scheme via Statens Pensjonskasse (beneficial mortgages/insurance), welfare schemes, and 1.5 hours/week of exercise during working hours.

📩 How to Apply

Applications must be submitted electronically via the Jobbnorge recruitment portal. Required attachments (in English or a Scandinavian language) include:

Cover Letter (motivation, research interests, summary of scientific work).

Research Statement (1–2 pages on project fit and proposed ideas/directions).

Curriculum Vitae (CV) (education, employment history, pedagogical/administrative experience).

Copies of Educational Certificates & Transcripts (retrieved via Vitnemålsportalen.no where applicable).

Publication List & Up to 5 Selected Academic Works.

Contact Details for 2–3 References.  

For more information:

https://www.jobbnorge.no/en/available-jobs/job/307635/researcher-in-solar-physics  

The Department of Computer Science at Aalto University (Otaniemi campus, Espoo, Finland) is recruiting a Doctoral Researcher in the High-Performance Computing Lab led by Assoc. Prof. Maarit Korpi-Lagg.

The position is part of the PEAS (Population of Exoplanets around Active Suns) consortium—working alongside the University of Helsinki and the Leibniz Institute for Astrophysics Potsdam (AIP)—to build GPU-accelerated models of stellar dynamos and evaluate their impact on exoplanet habitability and space weather environments.

🔬 Core Responsibilities & Technical Scope

Magnetohydrodynamic (MHD) Simulations: Develop and run fully compressible, large-scale global and local MHD solar/stellar dynamo models using LUMI-class supercomputing resources.

Physics-Informed Machine Learning: Interface global MHD outputs with data-driven differential rotation constraints, active region progenitor tracking, and model pruning/selection.

Coronal & Wind Coupling: Couple global/local radiative MHD solvers with Space Weather Modeling Framework (SWMF) modules (AWSoM/IA) to simulate stellar coronae and stellar winds driven by dynamo-generated surface magnetic maps.

Teaching & Open Science: Participate in standard departmental teaching (~1,612 hours total annual workload) and open-science releases of code/data.

📋 Candidate Profile & Qualifications

Education: Master’s degree completed before contract start (e.g., Astrophysics, Applied Physics, Computational Science, or related).

Required Technical Skills: Strong programming capabilities in C/C++/Fortran and Python; coursework or experience in scientific computing, MHD/fluid dynamics, PDEs, parallel/GPU programming, and version control.

Preferred Experience: Experience with MHD/fluid dynamics solvers, physics-informed ML, GPU computing, or SWMF-like coronal models.

📅 Contract, Salary & Supercomputing Infrastructure

Appointment Type: 2-year fixed term with an option for a 2-year extension.

Starting Salary: €3,168.20 / month, including Finnish occupational healthcare and social security benefits.

HPC Resources: Access to Aalto Triton cluster, national CSC supercomputers (Roihu), and EuroHPC Tier-0 systems (LUMI).

Application Deadline: October 15, 2026.

📩 How to Apply

Submit a single consolidated PDF via Aalto University’s Workday recruitment portal including:

Curriculum Vitae (CV)

Cover Letter (1–2 pages detailing fit and research motivation)

Degree Transcripts

Contact info for 1–2 referees

Links to code repositories, theses, or preprints (if available)

Research Contact: Assoc. Prof. Maarit Korpi-Lagg (maarit.korpi-lagg@aalto.fi)

HR Contact: hr-cs@aalto.fi  

The British Antarctic Survey (BAS) is recruiting an open-ended (permanent) Radiation Belt Scientist to join its world-leading magnetospheric physics group in Cambridge, UK.

The position will contribute to the ongoing development and expansion of the BAS Radiation Belt Model (BAS-RBM), which provides hourly forecasts to the European Space Agency (ESA) and is licensed to the UK Met Office.

Depending on qualifications and leadership experience, the position will be appointed at either Band E or Band F.

🔬 Core Responsibilities & Duties

Band E Scope:

Lead research on Earth's radiation belts, wave-particle interactions, storm-time dynamics, atmospheric particle precipitation, and data assimilation.

Lead applications for competitive research grants, publish peer-reviewed papers, present at international conferences, and supervise Ph.D. students.

Band F Scope (in addition to Band E):

Line-manage junior scientists and research teams.

Lead negotiations and contract definitions with commercial, governmental, and external bodies (e.g., ESA, Met Office).

Develop new operational and commercial applications using existing radiation belt frameworks.

📋 Candidate Profile & Qualifications

Education: Ph.D. or equivalent experience in Physics, Applied Mathematics, Space Physics, or a closely related field.

Domain Expertise: Strong background in magnetospheric physics (radiation belt physics is highly desirable) with demonstrated mathematical and computational modeling capabilities.

Technical & Programming Skills: Proven programming ability; good working knowledge of Python, FORTRAN, and Git is desirable.

Band F Requirements: Proven track record of securing competitive grant/fellowship funding and experience leading small research teams.

📅 Salary, Contract & Key Dates

Contract Type: Open-ended (Permanent appointment).

Salary:

Band E (S2): £52,907 – £58,198 per annum

Band F (S2): £64,463 – £70,909 per annum

Location: Cambridge, United Kingdom.

Application Deadline: August 30, 2026, at 06:55 PM / 23:59 GMT (Job Ref: BAS 26/65 / 2542).

Interview Date: September 25, 2026.

📩 How to Apply

Applications must be submitted electronically via the official UKRI/BAS jobs portal using Job Identification 2542. 

For more information See link below.

https://fa-evzn-saasfaukgovprod1.fa.ocs.oraclecloud.com/hcmUI/CandidateExperience/en/sites/UKRI-Careers/job/2542

Security vetting/clearance will form part of the onboarding process.  

The South African National Space Agency (SANSA) is recruiting a permanent Researcher (Space Physics Focus) within its Space Science Programme located in Hermanus, Western Cape.

This permanent role centers on conducting independent research in space physics, delivering operational applications for space weather, writing grant proposals, and supervising postgraduate students.

🔬 Core Responsibilities & Focus Areas

Independent Research: Lead cutting-edge research in space physics, with a primary focus on solar physics, heliophysics, and operational space weather applications.

Human Capital Development: Lecture, deliver seminars, and actively supervise postgraduate students (MSc/PhD) to grow South Africa's space science capacity.

Grant Writing & Collaboration: Author competitive research proposals, establish national/international partnerships, and build research networks (especially across other African nations).

📋 Candidate Profile & Qualifications

Education: Ph.D. in Space Science, Space Physics, Applied Mathematics, or Engineering.

Experience: 3–5 years in a dedicated research role with a strong track record of peer-reviewed publications (preferably first-authored).

Technical & Academic Skills: Advanced programming (preferably Python), experience writing research proposals, and public science outreach.

Key Advantages: Research that aligns with SANSA's operational space weather goals, established research contacts across Africa, and an NRF (National Research Foundation) rating.

📅 Contract, Salary & Key Dates

Positions Available: 1

Contract Type: Permanent

Location: Hermanus, Western Cape, South Africa

Compensation: Market-related

Closing Date: 03 August 2026 (Job Ref: RES004)

📩 How to Apply

Submit your application and detailed CV through the official SANSA career portal.

Application Portal and For more information:

https://sansajobs.mcidirecthire.com/Vacancy/ViewDetails?parameters=q4%2f37VDQTFWXnK7wNIeCPW0C7QllPbP7Mzq1htukcaEQNGungduQaTKsWxYlbyqh844ybuT5BI%2b2G2aDWlNIWD8787UKpzGWmIyyKO2mpLKi2bJlQMWCYkxtFcrdNaZydSD7HXVGD9Uy6HUC%2f1CYgQ%3d%3d 

The Department of Physics and Astronomy at the University of Iowa invites applications for an open-rank, tenure-track faculty position in Experimental Space Physics. While targeted primarily at the rank of tenure-track Assistant Professor, exceptional applications at the Associate or Full Professor level will be fully considered.

The University of Iowa holds a legendary status in space physics—stretching from James Van Allen’s discovery of Earth’s radiation belts in 1958 to leading current NASA missions like TRACERS. To carry this legacy forward, the university has established the Iowa Spaceflight Laboratory, a unified, state-of-the-art facility backed by an extensive engineering and technical staff equipped to design, fabricate, and test spaceflight hardware.

🔬 Core Responsibilities

Research Leadership, Educational Excellence, Institutional Service.

📋 Candidate Profile & Qualifications

Minimum Requirements:

Education: A Ph.D. in Physics or a closely related discipline awarded by the position's start date.

Scholarship: A demonstrated record of high-quality scholarship in experimental space physics.

Academic Potential: Strong potential to develop an internationally recognized, externally funded research portfolio alongside a firm commitment to effective teaching and excellent communication.

Desirable Merits:

Direct experience engineering or managing suborbital (sounding rocket/balloon) and/or orbital space missions.

A proven track record of securing external research funding.

Concrete, strategic plans to leverage the newly commissioned Iowa Spaceflight Laboratory facilities and engineering staff.

Clear potential for synergy and research collaboration with existing space physics or plasma faculty. 

📅 Timeline, Location & Institutional Disclosures

Location: Iowa City, Iowa (A midsize, highly rated Midwest college town designated as a UNESCO City of Literature).

Review Window: Formal review of applications begins on October 1, 2026, continuing on a rolling basis until the position is filled.

Work Authorization: The department notes that it will not cover the $100,000 fee associated with certain H-1B sponsorships subject to the September 19, 2025, Presidential Proclamation, but explicitly encourages international candidates to explore alternative work authorization pathways with their immigration team.

Vetting: Successful candidates will undergo a standard background/credential check and a mandatory self-disclosure of prior misconduct history.

📩 How to Apply

Applications must be submitted electronically via the official portal at Jobs@UIowa under Requisition #75971. Your digital application package must include:

Letter of Interest (Cover Letter).

Curriculum Vitae (CV).

Research Statement (detailing past scholarship and future plans to leverage Iowa's hardware infrastructure).

Teaching Statement (outlining pedagogical philosophy and mentoring approaches).

Three Professional References: Contact emails must be provided; the online system will automatically prompt your references to upload their letters of recommendation directly. 

For informal inquiries or to discuss research alignment, you can contact the search committee chair, Professor Jasper Halekas, with the subject line “Experimental Space Physics Faculty Search” at jasper-halekas@uiowa.edu.

For more information:

https://jobs.uiowa.edu/faculty/view/75971 

𝑨𝒇𝒓𝒊𝒄𝒂𝒏 𝑹𝒆𝒔𝒆𝒂𝒓𝒄𝒉 𝑻𝒂𝒍𝒆𝒏𝒕𝒔 𝑬𝒙𝒑𝒆𝒓𝒊𝒆𝒏𝒄𝒊𝒏𝒈 𝑴𝒆𝒏𝒕𝒐𝒓𝒊𝒏𝒈 𝑰𝒏 𝑺𝒄𝒊𝒆𝒏𝒄𝒆 (𝑨𝑹𝑻𝑬𝑴𝑰𝑺) is a one-year partnership designed to foster career goals through expert exchange, networking, and interpersonal relationships.

🌍 𝑾𝒉𝒂𝒕 𝒊𝒔 𝑨𝑹𝑻𝑬𝑴𝑰𝑺?

This programme pairs graduates and doctoral candidates from African universities with Junior Scientists, PhDs, and Postdocs at Max Planck Institutes (MPIs). It is a mutual learning experience aimed at developing intercultural competence and broadening professional perspectives.

𝑾𝒉𝒂𝒕 𝒊𝒔 𝑨𝑹𝑻𝑬𝑴𝑰𝑺?

𝑶𝒏𝒆-𝒀𝒆𝒂𝒓 𝑴𝒆𝒏𝒕𝒐𝒓𝒔𝒉𝒊𝒑: Sustained collaboration with at least one exchange per month via email or video call.

4-𝑾𝒆𝒆𝒌 𝑹𝒆𝒔𝒆𝒂𝒓𝒄𝒉 𝑺𝒕𝒂𝒚: Mentees will visit their mentor’s Max Planck Institute in Germany to deepen scientific knowledge and expand their network.

𝑺𝒌𝒊𝒍𝒍 𝑩𝒖𝒊𝒍𝒅𝒊𝒏𝒈: Training in communication, leadership, and project proposal preparation.

𝑺𝒄𝒊𝒆𝒏𝒕𝒊𝒇𝒊𝒄 𝑾𝒐𝒓𝒌𝒔𝒉𝒐𝒑: All participants will gather at the end of the research stay to share project results.

𝑭𝒖𝒍𝒍 𝑭𝒖𝒏𝒅𝒊𝒏𝒈: Support includes a 4-week research stay and reimbursement of visa and health insurance costs.

📝 𝑾𝒉𝒐 𝑪𝒂𝒏 𝑨𝒑𝒑𝒍𝒚?

Mentees: Graduates or doctoral candidates currently enrolled in a recognized African university. Must have a good command of English.

Mentors: PhDs and Postdocs at Max Planck Institutes interested in scientific exchange with African researchers.

📅 Deadline to Apply: April 13, 2026 📧 How to Apply: Send your CV, motivation letter, and the completed questionnaire to artemis@gv.mpg.de.

Don't miss the chance to gain international experience and shape your scientific career! 

Are you a graduate with a passion for orbital mechanics and estimation theory? The Space Observation and Astrodynamics Research (SOAR) Lab at Embry-Riddle Aeronautical University is expanding!

They are looking for motivated PhD candidates to conduct research in the vital field of Space Domain Awareness (SDA).

The Ideal Candidate:

🎓 Background in Aerospace Engineering, Astrodynamics, or Applied Math.

🛠️ Experience with Estimation, Optimization, and Programming (Python/MATLAB/C++).

💡 Highly motivated and research-driven.

This is your chance to join a premier aerospace institution and contribute to critical research in space sustainability and security.

📅 Application: Reviewing now for upcoming cycles.

📧 Contact: Email CV and transcripts to bhadaurs@erau.edu. 

📍 Boulder, Colorado | 🗓 July 13–24, 2026

Theme: Beyond Boundaries: Training Earth System Scientists and Engineers in Convergence Research for Compound Hazard Resilience

The ASP (Advanced Study Program) at NSF NCAR is now inviting applications for the 2026 EdEC ASP Summer Colloquium—a prestigious two-week, fully funded program designed to train the next generation of researchers to tackle compound hazards through convergence research.

🌪️🔥⚡ Why this matters

People and communities increasingly face compound hazards—co-occurring, cascading, or consecutive events such as tornadoes + floods, wildfires + flash flooding, or hurricanes followed by heatwaves. Building resilience requires integrating physical sciences, engineering, social sciences, and data/AI methods—and that’s exactly what this colloquium is about.

🔬 What you’ll gain

• Hands-on training in convergence research using a systems approach

• Scenario-based, experiential, and team-based learning

• Exposure to real-world challenges in weather, space weather, S2S hazards, and disaster resilience

• Collaboration with peers and experts across disciplines

• A clearer pathway from research to practical, actionable solutions

👩🏽‍🔬👨🏼‍💻 Who should apply

Graduate students who are:

• Interested in compound hazards and resilience

• Excited to work in interdisciplinary teams

• From Earth system sciences, solar & space physics, engineering, AI/ML, data science, social & behavioral sciences, or related fields

💰 Funding & logistics

• ASP covers travel and living expenses for 25 selected students

• A $200 registration fee applies (often covered by universities; financial assistance available if needed)

📝 Application details

• Applications open: December 12, 2025

• Applications close: February 22, 2026

• Includes long-form responses + 3-page CV

• AI use guidelines apply

If you’re a graduate student interested in breaking disciplinary boundaries and building skills that matter for real-world hazard resilience, this is an opportunity you don’t want to miss.

🔗 Questions? Contact the ASP colloquium coordinator via the program page: https://lnkd.in/dxR6BP7M 

We’re excited to invite undergraduate students to apply for the 2026 Summer Internship at Yerkes Observatory. This immersive program offers hands-on astronomy, research, and public engagement at one of the world’s most historic observatories.

🔭 What You’ll Do

• Work with on-site telescopes, including the 40″ Great Refractor, 0.6-m, and 1-m reflectors

• Gain practical experience in astronomy research and instrumentation

• Support public outreach programs and events at Yerkes

• Receive science communication mentorship

• Present your work at the end-of-program showcase

📅 Key Dates

• Application deadline: Monday, February 9, 2026 (5:00 PM CT)

• Decisions announced: Early March 2026

📧 Questions? Contact science-info@yerkesobservatory.org

To apply: see link below

https://yerkesobservatory.org/2026-summer-internship/