The main focus of this Priority Programme is to quantify terrestrial transport mechanisms and solar-terrestrial interactions through data analysis and modeling. The research programme builds on data from satellites on low-Earth orbits, such as CHAMP, GRACE, and GOCE. Special focus is given to the Swarm satellite mission.

Swarm DISC is a consortium of expert partners supporting the exploitation of the Swarm mission.

TIRO develops high-quality topside TEC (Total Electron Content) and inter-satellite KBR (K-Band Ranging) electron density products derived from multi-LEO satellite observations covering nearly two solar cycles from 2000 until now.

SWAMI aims to enhance the understanding of space weather processes and their impact on atmospheric density by: developing improved atmosphere and thermosphere models; new geomagnetic activity indices; and improving the forecast capabilities of the existing and new geomagnetic activity indices.

The Daedalus mission has been proposed to the European Space Agency (ESA) in response to the call for ideas for the Earth Observation programme's 10th Earth Explorer. It was selected in 2018 as one of three candidates for a Phase-0 feasibility study.

PRISM develops products from Swarm mission measurements that characterize plasmapause related boundaries in the topside Ionosphere.

This project is a part of the European Space Agency's (ESA's) Space Situational Awareness (SSA) programme, which includes the Space Weather (SWE) Segment. The objectives of this project are to coestimation of the definition and development activities within the Geomagnetic Conditions Expert Service Centre.

This project is a part of the European Space Agency's (ESA's) Space Situational Awareness (SSA) programme, which includes the Space Weather (SWE) Segment. The objectives of this project are to coestimation of the definition and development activities within the Ionospheric Weather Expert Service Centre.

The project focuses on connecting and understanding long-term changes of the Earth’s magnetic field, paleomagnetosphere, solar variability and their implications on paleoclimate studies in an interdisciplinary manner, in particular considering geomagnetic excursions during the past 100 ka.

We study the configuration of the paleomagnetosphere and the solar variability over the past 100 ka, in particular during geomagnetic excursions, and their effects on the shielding against galactic cosmic rays and in situ cosmogenic nuclide production rates.

This project aims at developing a new, data-based model of the last geomagnetic field reversal, the Matuyama-Brunhes reversal about 780 000 years ago.

This collaborative project with the University of Potsdam aims at a better understanding of uncertainties in global geomagnetic field reconstructions on centennial to millennial timescales.

Quantifying the electrodynamic characteristics of equatorial plasma depletions and its effects on navigatinal systems, such as GPS. (Project within SPP1788 - Dynamic Earth)

Novel methods for the 3D reconstruction of the dynamic evolution of the Van Allen belts using multiple satellite measurements (project B06 of Collaborative Research Centre 1294 “Data Assimilation: The seamless integration of data and models”)

Characterization of induced tidal signals. Investigation of the influence of space weather in coastal areas, which has been intensified by the ocean effect.

Characterization of the cooling of the Bardarbunga Dykes in Iceland.

High resolution modeling of the crustal magnetic field of the Mars. (Project within SPP1788 - Dynamic Earth)

On this site you will find some archived projects of the Section 2.3.