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 2020Show all

5 papers · 1 filter

astro-ph.SR2020★ 36 cited

Alfvenic Perturbations in a Sunspot Chromosphere Linked to Fractionated Plasma in the Corona

D. Baker, M. Stangalini, G. Valori +7

In this study, we investigate the spatial distribution of highly varying plasma composition around one of the largest sunspots of solar cycle 24. Observations of the photosphere, c…

astro-ph.SR2020★ 11 cited

The Magnetic Environment of a Stealth Coronal Mass Ejection

Jennifer O'Kane, Cecilia Mac Cormack, Cristina H. Mandrini +4

Interest in stealth coronal mass ejections (CMEs) is increasing due to their relatively high occurrence rate and space weather impact. However, typical CME signatures such as extre…

astro-ph.SR2020★ 38 cited

20 Years of ACE Data: How Superposed Epoch Analyses Reveal Generic Features in Interplanetary CME Profiles

F. Regnault, M. Janvier, P. Démoulin +4

Interplanetary coronal mass ejections (ICMEs) are magnetic structures propagating from the Sun's corona to the interplanetary medium. With over 20 years of observations at the L1 l…

astro-ph.SR2020★ 10 cited

Active-Region Tilt Angles from White-Light Images and Magnetograms: The Role of Magnetic Tongues

M. Poisson, P. Démoulin, C. H. Mandrini +1

The presence of elongations in active region (AR) polarities, called magnetic tongues, are mostly visible during their emergence phase. AR tilts have been measured thoroughly using…

astro-ph.SR2020★ 23 cited

Can Sub-photospheric Magnetic Reconnection Change the Elemental Composition in the Solar Corona?

Deborah Baker, Lidia van Driel-Gesztelyi, David H. Brooks +6

Within the coronae of stars, abundances of those elements with low first ionization potential (FIP) often differ from their photospheric values. The coronae of the Sun and solar-ty…