Chen, F.; Peter, H.; Bingert, S.; Cheung, M. C. M.: A model for the formation of the active region corona driven by magnetic flux emergence. Astronomy and Astrophysics 564, A12 (2014)
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)
Peter, H.; Bingert, S.; Klimchuk, J. A.; de Forest, C.; Cirtain, J. W.; Golub, L.; Winebarger, A. R.; Kobayashi, K.; Korreck, K. E.: Structure of solar coronal loops: from miniature to large-scale. Astronomy and Astrophysics 556, A104 (2013)
van Wettum, T.; Bingert, S.; Peter, H.: Parameterisation of coronal heating: spatial distribution and observable consequences. Astronomy and Astrophysics 554, A39 (2013)
Zacharias, P.; Peter, H.; Bingert, S.: Investigation of mass flows in the transition region and corona in a three-dimensional numerical model approach. Astronomy and Astrophysics 531, A97 (2011)
Bingert, S.; Peter, H.: Nanoflare Heating in the Solar Corona. In: High Performance Computing in Science and Engineering 14, S. 113 - 120 (Hg. Nagel, W. E.; Kröner, D. H.; Resch, M. M.). Springer International Publishing, Switzerland (2015)
Chen, F.; Peter, H.; Bingert, S.: Magnetic Field Lines and Coronal Loops A Difficult Relation. Living With a Star / Iris / Hinode Meeting, Portland, USA (2014)
Chen, F.; Peter, H.; Bingert, S.; Cheung, M. C. M.: Magnetic field lines and coronal loops. 14th European Solar Physics Meeting, Dublin, Ireland (2014)
Bewerbungsfrist 1 Oktober 2023. Promotionsprojekte in Planetenwissenschaften, Sonnenphysik, Astrophysik, Magnetfelder der Sonne, Helioseismologie, Asteroseismologie ...
In der mittleren Korona der Sonne entdeckt ein Forscherteam netzartige, dynamische Plasmastrukturen – und einen wichtigen Hinweis auf den Antrieb des Sonnenwindes.