Electron Heating by Parallel Electric Fields in Magnetotail Reconnection

Fuente: arXiv
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Main Authors: Richard, Louis, Khotyaintsev, Yuri V., Norgren, Cecilia, Steinvall, Konrad, Graham, Daniel B., Egedal, Jan, Vaivads, Andris, Nakamura, Rumi
Format: Preprint
Published: 2024
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author Richard, Louis
Khotyaintsev, Yuri V.
Norgren, Cecilia
Steinvall, Konrad
Graham, Daniel B.
Egedal, Jan
Vaivads, Andris
Nakamura, Rumi
author_facet Richard, Louis
Khotyaintsev, Yuri V.
Norgren, Cecilia
Steinvall, Konrad
Graham, Daniel B.
Egedal, Jan
Vaivads, Andris
Nakamura, Rumi
contents We investigate electron heating by magnetic-field-aligned electric fields ($E_\parallel$) during anti-parallel magnetic reconnection in the Earth's magnetotail. Using a statistical sample of 140 reconnection outflows, we infer the acceleration potential associated with $E_\parallel$ from the shape of the electron velocity distribution functions. We show that heating by $E_\parallel$ in the reconnection outflow can reach up to ten times the inflow electron temperature. We demonstrate that the magnitude of the acceleration potential scales with the inflow Alfvén and electron thermal speeds to maintain quasi-neutrality in the reconnection region. Our results suggest that, as the inflow plasma parameter $β_{e\infty}$ increases, $E_\parallel$ becomes increasingly important to the ion-to-electron energy partition associated with magnetic reconnection.
format Preprint
id arxiv_https___arxiv_org_abs_2412_10188
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Electron Heating by Parallel Electric Fields in Magnetotail Reconnection
Richard, Louis
Khotyaintsev, Yuri V.
Norgren, Cecilia
Steinvall, Konrad
Graham, Daniel B.
Egedal, Jan
Vaivads, Andris
Nakamura, Rumi
Space Physics
Plasma Physics
We investigate electron heating by magnetic-field-aligned electric fields ($E_\parallel$) during anti-parallel magnetic reconnection in the Earth's magnetotail. Using a statistical sample of 140 reconnection outflows, we infer the acceleration potential associated with $E_\parallel$ from the shape of the electron velocity distribution functions. We show that heating by $E_\parallel$ in the reconnection outflow can reach up to ten times the inflow electron temperature. We demonstrate that the magnitude of the acceleration potential scales with the inflow Alfvén and electron thermal speeds to maintain quasi-neutrality in the reconnection region. Our results suggest that, as the inflow plasma parameter $β_{e\infty}$ increases, $E_\parallel$ becomes increasingly important to the ion-to-electron energy partition associated with magnetic reconnection.
title Electron Heating by Parallel Electric Fields in Magnetotail Reconnection
topic Space Physics
Plasma Physics
url https://arxiv.org/abs/2412.10188