Chen, H.; Tian, H.; Li, L.; Peter, H.; Chitta, L. P.; Hou, Z.: Coronal condensation as the source of transition-region supersonic downflows above a sunspot. Astronomy and Astrophysics 659, p. A107 (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, p. A94 (2022)
Hu, H.; Liu, Y. D.; Chitta, L. P.; Peter, H.; Ding, M.: Spectroscopic and Imaging Observations of Spatially Extended Magnetic Reconnection in the Splitting of a Solar Filament Structure. The Astrophysical Journal 940, p. L12 (2022)
Li, L.; Peter, H.; Chitta, L. P.; Song, H.; Xu, Z.; Xiang, Y.: Reconfiguration and Eruption of a Solar Filament by Magnetic Reconnection with an Emerging Magnetic Field. The Astrophysical Journal 935, p. 85 (2022)
Mou, C.; Peter, H.; Xia, L.; Huang, Z.: Anisotropic nonthermal motions in the transition region of solar active regions. Astronomy and Astrophysics 660, p. A3 (2022)
Peter, H.; Chitta, L. P.; Chen, F.; Pontin, D. I.; Winebarger, A. R.; Golub, L.; Savage, S. L.; Rachmeler, L. A.; Kobayashi, K.; Brooks, D. H.et al.; Cirtain, J. W.; De Pontieu, B.; McKenzie, D. E.; Morton, R. J.; Testa, P.; Tiwari, S. K.; Walsh, R. W.; Warren, H. P.: Parallel Plasma Loops and the Energization of the Solar Corona. The Astrophysical Journal 933, p. 153 (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)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.