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

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Showing astro-ph.SRShow all

13 papers · 1 filter

astro-ph.SR2023★ 1 cited

Physics-based model of solar wind stream interaction regions: Interfacing between Multi-VP and 1D MHD for operational forecasting at L1

R. Kieokaew, R. F. Pinto, E. Samara +12

Our current capability of space weather prediction in the Earth's radiation belts is limited to only an hour in advance using the real-time solar wind monitoring at the Lagrangian…

astro-ph.SR2022★ 23 cited

The preferential orientation of magnetic switchbacks, implications for solar magnetic flux transport

Naïs Fargette, Benoit Lavraud, Alexis P. Rouillard +3

We investigate the orientation of the magnetic field deflections in switchbacks (SB) to determine if they are characterised by a possible preferential orientation. We compute the d…

astro-ph.SR2021★ 41 cited

Flux ropes and dynamics of the heliospheric current sheet

V. Réville, N. Fargette, A. P. Rouillard +19

Context. Solar Orbiter and PSP jointly observed the solar wind for the first time in June 2020, capturing data from very different solar wind streams, calm and Alfvénic wind as wel…

astro-ph.SR2021★ 19 cited

Magnetic reconnection as a mechanism to produce multiple protonpopulations and beams locally in the solar wind

B. Lavraud, R. Kieokaew, N. Fargette +37

Context. Spacecraft observations early revealed frequent multiple proton populations in the solar wind. Decades of research on their origin have focused on processes such as magnet…

astro-ph.SR2021★ 74 cited

Characteristic scales of magnetic switchback patches near the Sun and their possible association with solar supergranulation and granulation

Naïs Fargette, Benoit Lavraud, Alexis Rouillard +16

Parker Solar Probe (PSP) data recorded within a heliocentric radial distance of 0.3 AU have revealed a magnetic field dominated by Alfvénic structures that undergo large local vari…

astro-ph.SR2021★ 13 cited

Solar wind rotation rate and shear at coronal hole boundaries, possible consequences for magnetic field inversions

R. F. Pinto, N. Poirier, A. P. Rouillard +6

In-situ measurements by several spacecraft have revealed that the solar wind is frequently perturbed by transient structures (magnetic folds, jets, waves, flux-ropes) that propagat…