activity
20172022
most citedElectron scale structures and magnetic reconnection signatures in the turbulent magnetosheath

113 citations · 612 across the 14 of their papers we have counts for

collaborators

27 papers

physics.space-ph20229 cited

Mirror mode storms observed by Solar Orbiter

A. P. Dimmock, E. Yordanova, D. B. Graham +8

Mirror modes are ubiquitous in space plasma and grow from pressure anisotropy. Together with other instabilities, they play a fundamental role in constraining the free energy conta…

physics.space-ph2022

2D reconstruction of magnetotail electron diffusion region measured by MMS

J. M. Schroeder, J. Egedal, G. Cozzani +4

Models for collisionless magnetic reconnection in near-Earth space are distinctly characterized as 2D or 3D. In 2D kinetic models, the frozen-in law for the electron fluid is usual…

astro-ph.SR202238 cited

Kinetic-scale current sheets in near-Sun solar wind: properties, scale-dependent features and reconnection onset

A. Lotekar, I. Y. Vasko, T. Phan +6

We present statistical analysis of 11,200 proton kinetic-scale current sheets (CS) observed by Parker Solar Probe during 10 days around the first perihelion. The CS thickness i…

astro-ph.SR2021

Signatures of coronal hole substructure in the solar wind: combined Solar Orbiter remote sensing and in situ measurements

T. S. Horbury, R. Laker, L. Rodriguez +21

Context. The Sun's complex corona is the source of the solar wind and interplanetary magnetic field. While the large scale morphology is well understood, the impact of variations i…

physics.space-ph2021

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.plasm-ph2021

Non-Maxwellianity of electron distributions near Earth's magnetopause

D. B. Graham, Yu. V. Khotyaintsev, M. André +6

Plasmas in Earth's outer magnetosphere, magnetosheath, and solar wind are essentially collisionless. This means particle distributions are not typically in thermodynamic equilibriu…