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H. Peter

4 papers hereh-index 3267 citations11 works total

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

author position
  • middle author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
same name
  • H. Peter — 75 papers, h 32
  • H. Peter — 28 papers, h 17
  • H. Peter — 28 papers, h 12
  • H. Peter — 7 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
20232026
most citedSpatial distributions of EUV brightenings in the quiet-Sun

14 citations · 21 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2026

Small-scale impulsive EUV emission enhancements along network loops

A. Dolliou, H. Peter, S. Mandal +4

Network loops are a common feature in the quiet Sun. The physical processes sustaining their energy budget is still under discussion. We rely on a multi-instrumental (Solar Orbiter…

astro-ph.SR2024★ 14 cited

Spatial distributions of EUV brightenings in the quiet-Sun

C. J. Nelson, L. A. Hayes, D. Müller +16

The identification of large numbers of localised transient EUV brightenings, with small spatial scales, in the quiet-Sun corona has been one of the key early results from Solar Orb…

astro-ph.SR2024

Investigating coronal loop morphology and dynamics from two vantage points

Sudip Mandal, Hardi Peter, James A. Klimchuk +9

Coronal loops serve as the fundamental building blocks of the solar corona. Therefore, comprehending their properties is essential in unraveling the dynamics of the Sun's upper atm…

astro-ph.SR2023★ 7 cited

Slow solar wind sources. High-resolution observations with a quadrature view

Krzysztof Barczynski, Louise Harra, Conrad Schwanitz +16

The origin of the slow solar wind is still an open issue. One possibility that has been suggested is that upflows at the edge of an active region can contribute to the slow solar w…

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