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)
Brooks, D. H.; Winebarger, A. R.; Savage, S.; Warren, H. P.; Pontieu, B. D.; Peter, H.; Cirtain, J. W.; Golub, L.; Kobayashi, K.; McIntosh, S. W.et al.; McKenzie, D.; Morton, R.; Rachmeler, L.; Testa, P.; Tiwari, S.; Walsh, R.: The Drivers of Active Region Outflows into the Slow Solar Wind. The Astrophysical Journal 894 (2), 144 (2020)
Chitta, L. P.; Peter, H.; Priest, E. R.; Solanki, S. K.: Impulsive coronal heating during the interaction of surface magnetic fields in the lower solar atmosphere. Astronomy and Astrophysics 644, A130 (2020)
Guo, L.-J.; de Pontieu, B.; Huang, Y.-M.; Peter, H.; Bhattacharjee, A.: Observations and modeling of the onset of fast reconnection in the solar transition region. The Astrophysical Journal 901 (2), 148 (2020)
Li, L.; Peter, H.; Chitta, L. P.; Song, H.: Relation of Coronal Rain Originating from Coronal Condensations to Interchange Magnetic Reconnection. The Astrophysical Journal 905 (1), 26 (2020)
Pontin, D. I.; Peter, H.; Chitta, L. P.: Non-thermal line broadening due to braiding-induced turbulence in solar coronal loops. Astronomy and Astrophysics 639, A21 (2020)
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.