The Space Plasma Physics group carries out research into plasma processes throughout the heliosphere, including the magnetospheres of Earth and other planets and the solar wind. Fundamental plasma processes in the solar system are investigated through the theoretical modeling and by the analysis of satellite data.
The Earth's magnetosphere originates from the interaction between the solar wind and the Earth's magnetic field. The solar wind distorts the terrestrial dipole field, expands the magnetosphere on the night side and forms the magnetic tail like a windsock in the breeze. In the night side of the magnetosphere oppositely directed magnetic fields are brought together and a current is induced in the center. Through various plasma processes in the magnetosphere, a substantial part of the electromagnetic energy can cause particles to be energized, which can then penetrate into the Earth's ionosphere and generates the Northern lights. Such interactions are also present in the magnetospheres of other planets.
The solar wind is a turbulent flow from the Sun's outer atmosphere into interplanetary space and forms a bubble around the solar system called the heliosphere. Explosive solar flares can release large amounts of energy and mass in the form of a plasma cloud from electrically charged particles. The solar wind influences the movement of dust in the heliosphere and interacts with local magnetic fields affecting the atmospheres and magnetospheres of the planets, moons and small celestial bodies.
The research group's data analysis focuses on space missions for which IWF has built scientific instruments such as Cluster, THEMIS, Rosetta, MMS, BepiColombo, and Solar Orbiter. Cross-cutting research topics are:
In addition to the analysis of satellite data from currently flying missions, the research group also deals with the planning and preparation of future space missions.