Bourdin, P. A.; Bingert, S.; Peter, H.: Scaling laws of coronal loops compared to a 3D MHD model of an active region. Astronomy and Astrophysics 589, A86 (2016)
Bourdin, P. A.; Bingert, S.; Peter, H.: Coronal energy input and dissipation in a solar active region 3D MHD model. Astronomy and Astrophysics 580, A72 (2015)
Bourdin, P.-A.; Bingert, S.; Peter, H.: Observationally driven 3D magnetohydrodynamics model of the solar corona above an active region. Astronomy and Astrophysics 555, A123 (2013)
Bourdin, P.-A.: Observationally driven 3D MHD model of the solar corona above a magnetically active region. Dissertation, Georg‐August‐Univ., Göttingen (2013)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.