activity
20142023
most citedElectron-Scale Dynamics of the Diffusion Region during Symmetric Magnetic Reconnection in Space

323 citations · 1.9k across the 32 of their papers we have counts for

collaborators
Showing 2020Show all

5 papers · 1 filter

astro-ph.SR2020★ 112 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★ 67 cited

Tearing instability and periodic density perturbations in the slow solar wind

Victor Réville, Marco Velli, Alexis Rouillard +4

In contrast with the fast solar wind, that originates in coronal holes, the source of the slow solar wind is still debated. Often intermittent and enriched with low FIP elements --…

physics.plasm-ph2020★ 24 cited

Simulation of plasmaspheric plume impact on dayside magnetic reconnection

Jérémy Dargent, Nicolas Aunai, Benoît Lavraud +2

During periods of strong magnetic activity, cold dense plasma from the plasmasphere typically forms a plume extending towards the dayside magnetopause, eventually reaching it. In t…

astro-ph.SR2020★ 111 cited

Parker Solar Probe In-Situ Observations of Magnetic Reconnection Exhausts During Encounter 1

T. D. Phan, S. D. Bale, J. P. Eastwood +23

Magnetic reconnection in current sheets converts magnetic energy into particle energy. The process may play an important role in the acceleration and heating of the solar wind clos…

astro-ph.SR2020★ 64 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…