192 citations · 3.1k across the 75 of their papers we have counts for
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Solar Activity: Triennial Report of IAU Commission 10 (2006-2009)
J. A. Klimchuk, L. van Driel-Gesztelyi, C. J. Schrijver +9
Commission 10 deals with solar activity in all of its forms, ranging from the smallest nanoflares to the largest coronal mass ejections. This report reviews scientific progress ove…
Modeling the (upper) solar atmosphere including the magnetic field
H. Peter
The atmosphere of the Sun is highly structured and dynamic in nature. From the photosphere and chromosphere into the transition region and the corona plasma- changes from above…
Link between the chromospheric network and magnetic structures of the corona
Stefan Jendersie, Hardi Peter
Recent work suggested that the traditional picture of the corona above the quiet Sun being rooted in the magnetic concentrations of the chromospheric network alone is strongly ques…
First VUV full-Sun spectrum of the transition region with high spectral resolution compared to cool stars
Hardi Peter
This paper reports the first full-Sun vacuum ultraviolet (VUV) emission line profile originating from the transition region from the chromosphere to the corona. It is based on a ra…
Forward modeling of stellar coronae: from a 3D MHD model to synthetic EUV spectra
H. Peter, B. V. Gudiksen, A. Nordlund
A forward model is described in which we synthesize spectra from an ab-initio 3D MHD simulation of an outer stellar atmosphere, where the coronal heating is based on braiding of ma…
Coronal heating through braiding of magnetic field lines
H. Peter, B. V. Gudiksen, A. Nordlund
Cool stars like our Sun are surrounded by a million degree hot outer atmosphere, the corona. Since more than 60 years the physical nature of the processes heating the corona to tem…