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

33 papers

physics.plasm-ph2023★ 1 cited

HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence

Kristopher G. Klein, Harlan Spence, Olga Alexandrova +47

HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division designed to explore the dynamic three-dimensional mechanisms controlling the physics of plasma…

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…

physics.space-ph2023★ 18 cited

Parker Solar Probe Observations of High Plasma Beta Solar Wind from Streamer Belt

Jia Huang, J. C. Kasper, Davin E. Larson +23

In general, slow solar wind from the streamer belt forms a high plasma beta equatorial plasma sheet around the heliospheric current sheet (HCS) crossing, namely the heliospheric pl…

physics.space-ph2022★ 6 cited

Hybrid simulations of the cusp and dayside magnetosheath dynamics under \ quasi-radial interplanetary magnetic fields

J. Ng, L. J. Chen, Y. Omelchenko +2

Under quasi-radial interplanetary magnetic fields (IMF), foreshock turbulence can have an impact on the magnetosheath and cusps depending on the location of the quasi-parallel shoc…

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…

physics.space-ph2021★ 30 cited

Multi-spacecraft observations of the structure of the sheath of an interplanetary coronal mass ejection and related energetic ion enhancement

E. K. J. Kilpua, S. W. Good, N. Dresing +18

Sheaths ahead of coronal mass ejections (CMEs) are large heliospheric structures that form with CME expansion and propagation. Turbulent and compressed sheaths contribute to the ac…