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Electron heat flux instability
DOI: 10.1093/mnras/stw2900 Bibcode: 2017MNRAS.465.1672S

Lazar, M.; Yoon, P. H.; Saeed, Sundas +2 more

The heat flux instability is an electromagnetic mode excited by a relative drift between the protons and two-component core-halo electrons. The most prominent application may be in association with the solar wind where drifting electron velocity distributions are observed. The heat flux instability is somewhat analogous to the electrostatic Bunema…

2017 Monthly Notices of the Royal Astronomical Society
Ulysses 32