activity
19992019
most citedThe Origin of Non-Maxwellian Solar Wind Electron Velocity Distribution Function: Connection to Nanoflares in the Solar Corona

48 citations · 149 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2019★ 9 cited

A Brief Review on Particle Acceleration in Multi-island Magnetic Reconnection

H. Che, G. P. Zank

The basic physics and recent progresses in theoretical and particle-in-cell (PIC) simulation studies of particle acceleration in multi-island magnetic reconnection are briefly revi…

physics.space-ph2018

On the Rates of Steady, Quasi-steady and Impulsive Magnetic Reconnection

H. Che

Magnetic reconnection (MR) is considered as a major source of particle energization in astrophysical plasma. In the past, analysis of MR often assumes the magnetostatic condition,…

physics.space-ph2017★ 38 cited

How Electron Two-Stream Instability Drives Cyclic Langmuir Collapse and Continuous Coherent Emission

H. Che, M. L. Goldstein, P. H. Diamond +1

Continuous plasma coherent emission is maintained by repetitive Langmuir collapse driven by the nonlinear evolution of a strong electron two-stream instability. The Langmuir waves…

astro-ph.SR2016★ 24 cited

Electron Two-stream Instability and Its Application in Solar and Heliophysics

Haihong Che

It is well known that electron beams accelerated in solar flares can drive two-stream instability and produce radio bursts in the solar corona as well as in the interplanetary medi…

astro-ph.SR2016★ 2 cited

Common Origin of Kinetic Scale Turbulence and the Electron Halo in the Solar Wind -- Connection to Nanoflares

Haihong Che

We summarize our recent studies on the origin of solar wind kinetic scale turbulence and electron halo in the electron velocity distribution function. Increasing observations of na…

astro-ph.SR2014★ 48 cited

The Origin of Non-Maxwellian Solar Wind Electron Velocity Distribution Function: Connection to Nanoflares in the Solar Corona

H. Che, M. Goldstein

The formation of the observed core-halo feature in the solar wind electron velocity distribution function is a long-time puzzle. In this letter based on the current knowledge of na…