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researcher

P. Démoulin

47 papers hereh-index 5711.4k citations378 works total

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

author position
  • first author2
  • middle author36
  • last author5

Across the 43 of 47 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR40
  • astro-ph5
  • physics.space-ph2
same name
  • P. Démoulin — 22 papers, h 11
  • P. Démoulin — 19 papers, h 21
  • P. Démoulin — 5 papers, h 4
  • P. Démoulin — 4 papers, h 1
  • P. Démoulin — 4 papers, h 5
  • P. Démoulin — 3 papers, h 4

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
19992024
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 · 2.5k across the 47 of their papers we have counts for

collaborators
Showing 2022Show all

3 papers · 1 filter

physics.space-ph2022★ 4 cited

A robust estimation of the twist distribution in magnetic clouds

V. Lanabere, P. Démoulin, S. Dasso

Magnetic clouds (MCs) are observed insitu by spacecraft. The rotation of their magnetic field is typically interpreted as the crossing of a twisted magnetic flux tube, or flux rope…

astro-ph.SR2022★ 45 cited

Statistical Analysis of the Radial Evolution of the Solar Winds between 0.1 and 1 au, and their Semi-empirical Iso-poly Fluid Modeling

Dakeyo, Maksimovic, Démoulin +2

Statistical classification of the Helios solar wind observations into several populations sorted by bulk speed has revealed an outward acceleration of the wind. The faster the wind…

astro-ph.SR2022★ 10 cited

Eruption of EUV Hot-Channel near Solar Limb and Associated Moving Type-IV Radio Burst

P. Vemareddy, P. Démoulin, K. Sasikumar Raja +3

Using the observations from Solar Dynamics Observatory, we study an eruption of a hot-channel flux rope (FR) near the solar-limb on February 9, 2015. The pre-eruptive structure is…

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