Energy transport through Earth’s plasma sheet in 3-D

A statistical analysis of energy transport through Earth’s plasma sheet is performed using 6 years of Magnetospheric Multi-Scale (MMS) mission observations. The analysis entails a complete decomposition of the contributions to transport including the ion heat flux and enthalpy flux derived from the...

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Main Authors: K. C. Barik, C. C. Chaston
Format: Article
Language:English
Published: Frontiers Media S.A. 2025-01-01
Series:Frontiers in Astronomy and Space Sciences
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Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2024.1481448/full
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author K. C. Barik
C. C. Chaston
author_facet K. C. Barik
C. C. Chaston
author_sort K. C. Barik
collection DOAJ
description A statistical analysis of energy transport through Earth’s plasma sheet is performed using 6 years of Magnetospheric Multi-Scale (MMS) mission observations. The analysis entails a complete decomposition of the contributions to transport including the ion heat flux and enthalpy flux derived from the full ion pressure tensor to provide a three-dimensional (3-D) picture of plasma sheet energy transport. It is shown that the Poynting flux and enthalpy flux compete to dominate the total energy transport, while the heretofore ignored heat flux generally contributes a larger fraction of the total energy flux than the bulk kinetic energy flux. The spatial distribution of these fluxes are consistent with magnetic reconnection driven transport from an X-line statistically located at X∼−20RE. Kinetic fluxes stream Earthward from this point peaking mid-tail along the neutral sheet, while Poynting fluxes peak at higher latitudes and along the inner edge of the plasma sheet.
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spelling doaj-art-fd8cdc240125450da6263e2b1ead220c2025-01-06T06:59:25ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2025-01-011110.3389/fspas.2024.14814481481448Energy transport through Earth’s plasma sheet in 3-DK. C. BarikC. C. ChastonA statistical analysis of energy transport through Earth’s plasma sheet is performed using 6 years of Magnetospheric Multi-Scale (MMS) mission observations. The analysis entails a complete decomposition of the contributions to transport including the ion heat flux and enthalpy flux derived from the full ion pressure tensor to provide a three-dimensional (3-D) picture of plasma sheet energy transport. It is shown that the Poynting flux and enthalpy flux compete to dominate the total energy transport, while the heretofore ignored heat flux generally contributes a larger fraction of the total energy flux than the bulk kinetic energy flux. The spatial distribution of these fluxes are consistent with magnetic reconnection driven transport from an X-line statistically located at X∼−20RE. Kinetic fluxes stream Earthward from this point peaking mid-tail along the neutral sheet, while Poynting fluxes peak at higher latitudes and along the inner edge of the plasma sheet.https://www.frontiersin.org/articles/10.3389/fspas.2024.1481448/fullenergy transportplasma sheetmagnetotailmagnetic reconnectionion flow
spellingShingle K. C. Barik
C. C. Chaston
Energy transport through Earth’s plasma sheet in 3-D
Frontiers in Astronomy and Space Sciences
energy transport
plasma sheet
magnetotail
magnetic reconnection
ion flow
title Energy transport through Earth’s plasma sheet in 3-D
title_full Energy transport through Earth’s plasma sheet in 3-D
title_fullStr Energy transport through Earth’s plasma sheet in 3-D
title_full_unstemmed Energy transport through Earth’s plasma sheet in 3-D
title_short Energy transport through Earth’s plasma sheet in 3-D
title_sort energy transport through earth s plasma sheet in 3 d
topic energy transport
plasma sheet
magnetotail
magnetic reconnection
ion flow
url https://www.frontiersin.org/articles/10.3389/fspas.2024.1481448/full
work_keys_str_mv AT kcbarik energytransportthroughearthsplasmasheetin3d
AT ccchaston energytransportthroughearthsplasmasheetin3d