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Observations of Electromagnetic Electron Holes and Evidence of Cherenkov Whistler Emission

We report observations of electromagnetic electron holes (EHs). We use multi-spacecraft analysis to quantify the magnetic field contributions of three mechanisms: the Lorentz transform, electron drift within the EH, and Cherenkov emission of whistler waves. The first two mechanisms account for the observed magnetic fields for slower EHs, while for EHs with speeds approaching half the electron Alfvén speed, whistler waves excited via the Cherenkov mechanism dominate the perpendicular magnetic field. The excited whistlers are kinetically damped and typically confined within the EHs.

preprint2020arXivOpen access
Konrad SteinvallYuri V. KhotyaintsevDaniel B. GrahamAndris VaivadsOlivier Le ContelChristopher T. Russell
physics.space-phphysics.plasm-ph
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Konrad SteinvallYuri V. KhotyaintsevDaniel B. GrahamAndris VaivadsOlivier Le ContelChristopher T. Russell

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