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researcher

H. Peter

28 papers hereh-index 12660 citations18 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author2
  • first author3
  • middle author12
  • last author4

Across the 21 of 28 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR28
same name
  • H. Peter — 75 papers, h 32
  • H. Peter — 28 papers, h 17
  • H. Peter — 7 papers, h 3
  • H. Peter — 4 papers, h 3
  • H. Peter — 2 papers, h 4
  • H. Peter — 2 papers, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20102025
most citedHot Explosions in the Cool Atmosphere of the Sun

338 citations · 2.1k across the 28 of their papers we have counts for

collaborators
Showing 2013Show all

4 papers · 1 filter

astro-ph.SR2013★ 137 cited

Structure of solar coronal loops: from miniature to large-scale

H. Peter, S. Bingert, J. A. Klimchuk +6

We will use new data from the High-resolution Coronal Imager (Hi-C) with unprecedented spatial resolution of the solar corona to investigate the structure of coronal loops down to…

astro-ph.SR2013★ 61 cited

Observationally driven 3D MHD model of the solar corona above an active region

Ph. -A. Bourdin, S. Bingert, H. Peter

Aims. The goal is to employ a 3D magnetohydrodynamics (MHD) model including spectral synthesis to model the corona in an observed solar active region. This will allow us to judge t…

astro-ph.SR2013★ 10 cited

Magnetic field diagnostics and spatio-temporal variability of the solar transition region

H. Peter

Magnetic field diagnostics of the transition region from the chromosphere to the corona faces us with the problem that one has to apply extreme UV spectro-polarimetry. While for co…

astro-ph.SR2013★ 7 cited

Parametrization of coronal heating: spatial distribution and observable consequences

T. van Wettum, S. Bingert, H. Peter

We investigate the difference in the spatial distribution of the energy input for parametrizations of different mechanisms to heat the corona of the Sun and possible impacts on the…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.