50 citations · 58 across the 5 of their papers we have counts for
5 papers
Coronal bright point statistics II. Magnetic polarities and mini loops
I. Kraus, Ph. -A. Bourdin, J. Zender +2
Context. The solar corona maintains temperatures of a million Kelvin or more. The plasma heating mechanisms responsible for these extreme temperatures are still unclear. Large regi…
Solar wind entry into Mercury's magnetosphere: Simulation results for the second swingby of BepiColombo
Daniel Teubenbacher, Willi Exner, Moritz Feyerabend +7
Context. We use a global 3D hybrid plasma model to investigate the interaction between Mercury's magnetosphere and the solar wind for the second BepiColombo swingby, evaluate magne…
Data-driven simulations of magnetic field evolution in Active Region 11429: Magneto-friction method using PENCIL code
P. Vemareddy, Jörn Warnecke, Ph. A. Bourdin
Coronal magnetic fields evolve quasi statically over long time scales and dynamically over short time scales. As of now there exists no regular measurements of coronal magnetic fie…
Coronal bright point statistics I. Lifetime, shape, and coronal co-rotation
I. Kraus, Ph. -A. Bourdin, J. Zender +2
Context. The corona of the Sun is the part of the solar atmosphere with temperatures of over one million Kelvin, which needs to be heated internally in order to exist. This heating…
Ensemble Prediction of a Halo Coronal Mass Ejection Using Heliospheric Imagers
T. Amerstorfer, C. Möstl, P. Hess +5
The Solar TErrestrial RElations Observatory (STEREO) and its heliospheric imagers (HI) have provided us the possibility to enhance our understanding of the interplanetary propagati…