activity
20112026
most citedElectrostatic solitary waves in the Earth's bow shock: nature, properties, lifetimes and origin

39 citations · 117 across the 7 of their papers we have counts for

collaborators

7 papers

physics.plasm-ph2026

The FLARE Facility

Hantao Ji, Jongsoo Yoo, Peiyun Shi +53

The Facility for Laboratory Reconnection Experiments (FLARE) has been constructed to study magnetic reconnection in multiple X-line regimes relevant to space, astrophysical, and fu…

physics.space-ph2023

Unveiling plasma energization and energy transport in the Earth Magnetospheric System: the need for future coordinated multiscale observations

A. Retino, L. Kepko, H. Kucharek +31

Energetic plasma is everywhere in the Universe. The terrestrial Magnetospheric System is a key case where direct measures of plasma energization and energy transport can be made in…

astro-ph.SR2021★ 30 cited

On the origin of switchbacks observed in the solar wind

Forrest S. Mozer, Stuart Bale, John Bonnell +3

The origin of switchbacks in the solar wind is discussed in two classes of theory that differ in the location of the source being either in the transition region near the Sun or in…

physics.space-ph2021★ 39 cited

Electrostatic solitary waves in the Earth's bow shock: nature, properties, lifetimes and origin

R. Wang, I. Y. Vasko, F. S. Mozer +4

We present a statistical analysis of more than two thousand bipolar electrostatic solitary waves (ESW) collected from ten quasi-perpendicular Earth's bow shock crossings by Magneto…

physics.space-ph2020★ 13 cited

Shock Drift Acceleration of Ions in an Interplanetary Shock Observed by MMS

E. L. M. Hanson, O. V. Agapitov, I. Y. Vasko +6

An interplanetary (IP) shock wave was recorded crossing the Magnetospheric Multiscale (MMS) constellation on 2018 January 8. Plasma measurements upstream of the shock indicate effi…

physics.space-ph2012★ 21 cited

Kinetic Scale Density Fluctuations in the Solar Wind

C. H. K. Chen, G. G. Howes, J. W. Bonnell +3

We motivate the importance of studying kinetic scale turbulence for understanding the macroscopic properties of the heliosphere, such as the heating of the solar wind. We then disc…