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P. Démoulin

3 papers here

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

author position
  • middle author3

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph3
ORCID 0000-0001-8215-6532
same name
  • P. Démoulin — 1 paper, h 21

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

most citedNon-linear force-free field modeling of a solar active region around the time of a major flare and coronal mass ejection

305 citations · 492 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph2007★ 305 cited

Non-linear force-free field modeling of a solar active region around the time of a major flare and coronal mass ejection

C. J. Schrijver, M. L. DeRosa, T. Metcalf +14

Solar flares and coronal mass ejections are associated with rapid changes in field connectivity and powered by the partial dissipation of electrical currents in the solar atmospher…

astro-ph2007★ 152 cited

Progressive transformation of a flux rope to an ICME

S. Dasso, M. S. Nakwacki, P. Démoulin +1

The solar wind conditions at one astronomical unit (AU) can be strongly disturbed by the interplanetary coronal mass ejections (ICMEs). A subset, called magnetic clouds (MCs), is f…

astro-ph2007★ 35 cited

Are constant loop widths an artifact of the background and the spatial resolution?

M. C. Lopez Fuentes, P. Demoulin, J. A. Klimchuk

We study the effect of the coronal background in the determination of the diameter of EUV loops, and we analyze the suitability of the procedure followed in a previous paper (López…

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