Breu, C.; Peter, H.; Cameron, R. H.; Solanki, S. K.; Przybylski, D.; Rempel, M.; Chitta, L. P.: A solar coronal loop in a box: Energy generation and heating. Astronomy and Astrophysics 658, A45 (2022)
Chen, Y.; Peter, H.; Przybylski, D.; Tian, H.; Zhang, J.: Doppler shifts of spectral lines formed in the solar transition region and corona. Astronomy and Astrophysics 661, A94 (2022)
Chen, Y.; Przybylski, D.; Peter, H.; Tian, H.; Auchère, F.; Berghmans, D.: Transient small-scale brightenings in the quiet solar corona: A model for campfires observed with Solar Orbiter. Astronomy and Astrophysics 656, L7 (2021)
Chitta, L. P.; Peter, H.; Young, P.R.: Extreme-ultraviolet bursts and nanoflares in the quiet-Sun transition region and corona. Astronomy and Astrophysics 647, A159 (2021)
Li, L.; Peter, H.; Chitta, L. P.; Song, H.: On-disk Solar Coronal Condensations Facilitated by Magnetic Reconnection between Open and Closed Magnetic Structures. The Astrophysical Journal 910 (2), 82 (2021)
Li, L.; Peter, H.; Chitta, L. P.; Song, H.: Formation of a Solar Filament by Magnetic Reconnection and Coronal Condensation. The Astrophysical Journal Letters 919 (2), L21 (2021)
Li, L.-P.; Peter, H.; Chitta, L. P.; Song, H.-Q.: Revisiting the formation mechanism for coronal rain from previous studies. Research in Astronomy and Astrophysics 21 (10), 255 (2021)
Li, L.; Peter, H.; Chitta, L. P.; Song, H.; Ji, K.; Xiang, Y.: Magnetic Reconnection between Loops Accelerated By a Nearby Filament Eruption. The Astrophysical Journal 908 (2), 213 (2021)
Ni, L.; Chen, Y.; Peter, H.; Tian, H.; Lin, J.: A magnetic reconnection model for hot explosions in the cool atmosphere of the Sun. Astronomy and Astrophysics 646, A88 (2021)
Peter, H.; Ballester, E. A.; Andretta, V.; Auchere, F.; Belluzzi, L.; Bemporad, A.; Berghmans, D.; Buchlin, E.; Calcines, A.; Chitta, L. P.et al.; Dalmasse, K.; Aleman, T. d. P.; Feller, A.; Froment, C.; Harrison, R.; Janvier, M.; Matthews, S.; Parenti, S.; Przybylski, D.; Solanki, S. K.; Štěpán, J.; Teriaca, L.; Bueno, J. T.: Magnetic imaging of the outer solar atmosphere (MImOSA): Unlocking the driver of the dynamics in the upper solar atmosphere. Experimental Astronomy (2021)
Bewerbungsfrist 1 November 2022. Promotionsprojekte in Planetenwissenschaft, Sonnenphysik, Astrophysik, Magnetfelder der Sonne, Helioseismologie, Asteroseismologie ...
First Light für die wissenschaftlichen Instrumente von Sunrise III: Das ballongetragene Sonnenobservatorium bereitet sich auf den nächsten Forschungsflug vor.
Das dienstälteste Sonnenobservatorium im Weltraum wird 25 Jahre alt – und trägt gerade wegen seines hohen Alters noch immer maßgeblich zur Sonnenforschung bei.