Is the Solar Wind Electron Strahl a Seed Population for the Earth’s Electron Radiation Belt?

1) Since the outer electron radiation belt is lost on occasion, the radiation belt needs seed electrons to rebuild. 2) The clear candidate for that seed population is energetic substorm-injected electrons in the dipolar magnetosphere. 3) The energetic substorm-injected electrons in the dipole come f...

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Main Authors: Joseph E. Borovsky, Andrei Runov
Format: Article
Language:English
Published: Frontiers Media S.A. 2022-06-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2022.930162/full
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author Joseph E. Borovsky
Andrei Runov
author_facet Joseph E. Borovsky
Andrei Runov
author_sort Joseph E. Borovsky
collection DOAJ
description 1) Since the outer electron radiation belt is lost on occasion, the radiation belt needs seed electrons to rebuild. 2) The clear candidate for that seed population is energetic substorm-injected electrons in the dipolar magnetosphere. 3) The energetic substorm-injected electrons in the dipole come from the suprathermal electron population in the magnetotail plasma sheet, delivered by substorms. Scenario (1)–3) begs the question: Where do these magnetotail suprathermal electrons come from? We are hypothesizing that one source (perhaps the dominant source) is the energetic field-aligned electron strahl in the solar wind, which are electrons fresh from the solar corona.
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spelling doaj.art-01d0d40956ae41c2b408baa5d9bc497f2022-12-22T03:35:36ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2022-06-01910.3389/fspas.2022.930162930162Is the Solar Wind Electron Strahl a Seed Population for the Earth’s Electron Radiation Belt?Joseph E. Borovsky0Andrei Runov1Space Science Institute, Boulder, CO, United StatesDepartment of Earth, Planetary, and Space Sciences, University of California, Los Angeles, Los Angeles, CA, United States1) Since the outer electron radiation belt is lost on occasion, the radiation belt needs seed electrons to rebuild. 2) The clear candidate for that seed population is energetic substorm-injected electrons in the dipolar magnetosphere. 3) The energetic substorm-injected electrons in the dipole come from the suprathermal electron population in the magnetotail plasma sheet, delivered by substorms. Scenario (1)–3) begs the question: Where do these magnetotail suprathermal electrons come from? We are hypothesizing that one source (perhaps the dominant source) is the energetic field-aligned electron strahl in the solar wind, which are electrons fresh from the solar corona.https://www.frontiersin.org/articles/10.3389/fspas.2022.930162/fullradiation beltstrahlplasma sheetpolar rainmagnetosphere
spellingShingle Joseph E. Borovsky
Andrei Runov
Is the Solar Wind Electron Strahl a Seed Population for the Earth’s Electron Radiation Belt?
Frontiers in Astronomy and Space Sciences
radiation belt
strahl
plasma sheet
polar rain
magnetosphere
title Is the Solar Wind Electron Strahl a Seed Population for the Earth’s Electron Radiation Belt?
title_full Is the Solar Wind Electron Strahl a Seed Population for the Earth’s Electron Radiation Belt?
title_fullStr Is the Solar Wind Electron Strahl a Seed Population for the Earth’s Electron Radiation Belt?
title_full_unstemmed Is the Solar Wind Electron Strahl a Seed Population for the Earth’s Electron Radiation Belt?
title_short Is the Solar Wind Electron Strahl a Seed Population for the Earth’s Electron Radiation Belt?
title_sort is the solar wind electron strahl a seed population for the earth s electron radiation belt
topic radiation belt
strahl
plasma sheet
polar rain
magnetosphere
url https://www.frontiersin.org/articles/10.3389/fspas.2022.930162/full
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AT andreirunov isthesolarwindelectronstrahlaseedpopulationfortheearthselectronradiationbelt