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 2015Show all

5 papers · 1 filter

astro-ph.SR2015★ 202 cited

Strong coronal channelling and interplanetary evolution of a solar storm up to Earth and Mars

Christian Möstl, Tanja Rollett, Rudy A. Frahm +15

The severe geomagnetic effects of solar storms or coronal mass ejections (CMEs) are to a large degree determined by their propagation direction with respect to Earth. There is a la…

astro-ph.SR2015★ 177 cited

From coronal observations to MHD simulations, the building blocks for 3D models of solar flares

Miho Janvier, Guillaume Aulanier, Pascal Demoulin

Solar flares are energetic events taking place in the Sun's atmosphere, and their effects can greatly impact the environment of the surrounding planets. In particular, eruptive fla…

astro-ph.SR2015★ 33 cited

Evidence of Twisted flux-tube Emergence in Active Regions

Mariano Poisson, Cristina H. Mandrini, Pascal Démoulin +1

Elongated magnetic polarities are observed during the emergence phase of bipolar active regions (ARs). These extended features, called magnetic tongues, are interpreted as a conseq…

astro-ph.SR2015

Comparing generic models for interplanetary shocks and magnetic clouds axis configurations at 1 AU

Miho Janvier, Sergio Dasso, Pascal Demoulin +2

Interplanetary Coronal Mass Ejections are the manifestation of solar transient eruptions, which can significantly modify the plasma and magnetic conditions in the heliosphere. They…

astro-ph.SR2015★ 59 cited

FIP Bias Evolution in a Decaying Active Region

D. Baker, D. H. Brooks, P. Démoulin +4

Solar coronal plasma composition is typically characterized by first ionization potential (FIP) bias. Using spectra obtained by Hinode's EUV Imaging Spectrometer (EIS) instrument,…