Speaker
Verena Heidrich-Meisner
Description
The solar wind is a continuous stream of charges particles emitted by the Sun. Its properties are determined by the conditions in the solar corona. The solar wind contains the transition from a collisionless to a thermalized plasma. Thereby the solar wind provides the opportunity to investigate fundamental plasma processes and give insights into to solar corona. SOHO celebrates his 30th anniversary this year and some of the particle instruments of CELIAS are still operational. Here, we give a short overview in solar wind science with SOHO/CELIAS.
Author
Co-authors
Lars Berger
(CAU Kiel)
Robert F. Wimmer-Schweingruber
(CAU Kiel)
