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Summer school on Machine Learning for Space 2026

Course Overview

8th to 12th June 2026 – KTH, Stockholm, Sweden

This one-week summer school introduces modern machine learning (ML) methods applied to heliophysics and magnetospheric science, aimed at graduate students and early-career researchers. The program combines foundational lectures with hands-on coding sessions, enabling participants to build both conceptual understanding and practical skills.


Participants will explore core ML techniques—including supervised and unsupervised learning methods—and learn how to access, preprocess, and analyze real datasets from major space missions. Guided by experienced mentors, attendees will work directly with mission data, develop reproducible workflows, and implement ML models relevant to current research challenges in space physics.


The summer school emphasizes interactive learning, collaborative problem-solving, and discussion of best practices in scientific machine learning. At the end of the week, participants will have the opportunity to present their work or research interests in short lightning talks presentations, providing a platform for feedback, discussion, and networking.


Please note that the Summer School does not offer fellowships or financial support. Participants are responsible for their own travel and accommodation costs. The summer school does not include lunch or dinner. Participants are expected to arrange and pay for their own meals.


🎯Learning Objectives

By participating in the Summer School, attendees will be able to:

  1. Explain core concepts in space physics and identify key machine-learning applications in the field.
  2. Locate, access, and preprocess datasets from major missions such as Magnetospheric Multiscale Mission, Cluster, THEMIS, Solar and Heliospheric Observatory, Solar Dynamics Observatory, Solar Orbiter, and OMNI, applying workflows for cleaning, normalization, feature extraction, and time alignment.
  3. Apply and interpret dimensionality-reduction and unsupervised techniques (e.g., PCA, clustering, covariance analysis) to uncover structure and regimes in space-physics data.
  4. Design, implement, and validate machine-learning models for classification, prediction, and event detection in space-physics applications.
  5. Critically assess model performance, limitations, uncertainty, and physical interpretability, and discuss the role of ML in current and future space missions.
  6. Demonstrate proficiency with Python-based scientific and ML tools, such as scikit-learn, Pandas, and PyTorch.

  

Prerequisites

Basic Python programming and introductory linear algebra are recommended. No prior machine-learning expertise is required.


Who should apply:
This summer school is designed for graduate students and early-career researchers who are studying or conducting research in space physics, space weather, or related areas. As well as those with a machine learning background who are beginning to apply their skills in these fields. 


Participation in the summer school is free of charge, but registration is mandatory and subject to approval by the organizer. 


Sign-up using the form: https://forms.gle/6n79Vdw2Nxxm3BPF9

The sign-up will close on the  12th of April, 2026. 

 Credit: ESA/ATG medialab 

Schedule

Schedule is preliminary and subject to change.

13:00–13:30 Welcome and logistics 

13:30–14:15 Overview of heliophysics & space physics 

14:15–15:00 Introduction to ML Fundamentals

15:15–16:15 Participant introduction, Meet & Greet


 09:00–10:00 Understanding Your Data

10:00–10:30 Data preprocessing: cleaning, normalization, PCA 

10:30-11:00 Common ML Pitfalls in Space Physics

11:15–12:30 Structure Discovery in High-Dimensional Space

13:30–17:00 Hands‑on: Load datasets, apply PCA/clustering, explore time series features


 09:00–10:00 Magnetosphere basics: regions & dynamics 

10:00–11:00 MMS, Cluster, THEMIS datasets & data access

11:15–12:30 ML for magnetospheric applications: event detection, boundary finding 

13:30–17:00 Handson: Fetch data, identify events, classify/regime detection, boundary detection‑on: Fetch data, identify events, classify/regime detection, boundary detection


 09:00–10:00 Solar & heliospheric physics: activity cycles, solar wind, CMEs 

10:00–11:00 SOHO, SDO, Solar Orbiter, OMNI datasets  

11:15–12:30 ML methods: solar image classification, CME forecasting, solar wind prediction 

13:30–17:00 Hands‑on: Solar image segmentation, predictive modeling, project time


09:00–10:00 Inspiring talks: The state of ML in space research.
10:00–11:00 Discussion: Onboard autonomy, future missions.

11:15–12:00 Lightning talks

12:00-12:30 Closing remarks


Instructors and Organizers

Jonah Ekelund (Co-Organizing Chair, Instructor)

 KTH Royal Institute of Technology

jonahek (at) kth.se

Stefano Makidis (Co-Organizing Chair, Instructor)

 KTH Royal Institute of Technology 

George Miloshevich (Instructor)

KU Leuven

Ekaterina Dineva (Instructor)

KU Leuven

Panagiotis Gonidakis (Instructor)

KU Leuven

Venue and Practical Information

What to bring: a laptop with Python and Jupyter Notebook installed; alternatively, you can use Google Colab.


Fee: Participation in the summer school is free of charge, but registration is mandatory and subject to approval by the organizer. 


Sign-up: 

Sign-up using the form: https://forms.gle/6n79Vdw2Nxxm3BPF9

The sign-up will close on the 12th of April, 2026.  

KTH Royal Institute of Technology

KTH Entré, Drottning Kristinas väg, Stockholm, Sweden

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