activity
20162020
most citedThe Solar Orbiter Science Activity Plan: translating solar and heliospheric physics questions into action

112 citations · 334 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2020112 cited

The Solar Orbiter Science Activity Plan: translating solar and heliospheric physics questions into action

I. Zouganelis, A. De Groof, A. P. Walsh +182

Solar Orbiter is the first space mission observing the solar plasma both in situ and remotely, from a close distance, in and out of the ecliptic. The ultimate goal is to understand…

astro-ph.SR2020

Meteospace, a New Instrument for Solar Survey at the Calern Observatory

J. -M. Malherbe, Th Corbard, K. Dalmasse +1

High cadence observations of solar activity (active regions, flares, filaments) in the H line were performed at Meudon and Haute Provence Observatories from 1956 to 2004. More t…

astro-ph.SR202064 cited

Relating streamer flows to density and magnetic structures at the Parker Solar Probe

Alexis P. Rouillard, Athanasios Kouloumvakos, Angelos Vourlidas +34

The physical mechanisms that produce the slow solar wind are still highly debated. Parker Solar Probe's (PSP's) second solar encounter provided a new opportunity to relate in situ…

astro-ph.SR201956 cited

Magnetic helicity budget of solar active regions prolific of eruptive and confined flares

J. K. Thalmann, K. Moraitis, L. Linan +3

We compare the coronal magnetic energy and helicity of two solar active regions (ARs), prolific in major eruptive (AR~11158) and confined (AR~12192) flaring, and analyze the potent…

astro-ph.SR201916 cited

Data-Optimized Coronal Field Model: I. Proof of Concept

K. Dalmasse, A. Savcheva, S. E. Gibson +5

Deriving the strength and direction of the three-dimensional (3D) magnetic field in the solar atmosphere is fundamental for understanding its dynamics. Volume information on the ma…

astro-ph.SR201712 cited

Studying the transfer of magnetic helicity in solar active regions with the connectivity-based helicity flux density method

K. Dalmasse, E. Pariat, G. Valori +2

In the solar corona, magnetic helicity slowly and continuously accumulates in response to plasma flows tangential to the photosphere and magnetic flux emergence through it. Analyzi…