Research

Solar System Research

The cosmic neighborhood of the Earth is the central topic of the research at the Max Planck Institute for Solar System Research: the solar system with its planets, moons and diverse small bodies like comets and asteroids, and, of course, the Sun. Based on numerical simulations and novel measurement techniques the researchers probe the deep interior of our star and investigate its gaseous envelope, the solar magnet field and high-energy particles emitted by the Sun into space. Likewise they examine the surface and the interior of the planets as well as their magnetospheres, rings and moons. Further research areas comprise comets, asteroids and planetoids. The researchers develop physical models in order to specify the crucial processes, and evaluate them in numerical simulations. In addition the Max Planck Institute for Solar System Research is involved with scientific instruments in numerous missions of international space agencies.

Scientific Departments and Max Planck Research Groups at MPS

<p><span>All activity phenomena in the Sun and stars originate from their </span>magnetic fields, which arise due to a hydromagnetic dynamo that converts kinetic energy into magnetic form. Even the solar dynamo remains enigmatic due to the extreme complexity of phenomena related to it. Observations of other stars provide important constraints on the stellar dynamo mechanism(s). The work of the group aims at combining these observations with theory and models to gain better understanding of the solar dynamo.</p>

Max Planck Research Group: Solar and Stellar Magnetic Activity

All activity phenomena in the Sun and stars originate from their magnetic fields, which arise due to a hydromagnetic dynamo that converts kinetic energy into magnetic form. Even the solar dynamo remains enigmatic due to the extreme complexity of phenomena related to it. Observations of other stars provide important constraints on the stellar dynamo mechanism(s). The work of the group aims at combining these observations with theory and models to gain better understanding of the solar dynamo.

 
loading content