Investigating the Occurrence of Magnetic Reconnection at Jupiter's Dawn Magnetopause During the Juno Era

Abstract In this study, observations from the Jovian auroral distributions experiment, Jupiter energetic particle detector instrument, and Magnetic field investigation instruments on Juno are used to identify signatures of magnetic reconnection at Jupiter's dawn magnetopause and relate these si...

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Main Authors: J. Montgomery, R. W. Ebert, G. Clark, S. A. Fuselier, F. Allegrini, F. Bagenal, S. J. Bolton, G. A. DiBraccio, R. J. Wilson
Format: Article
Language:English
Published: Wiley 2022-07-01
Series:Geophysical Research Letters
Subjects:
Online Access:https://doi.org/10.1029/2022GL099141
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author J. Montgomery
R. W. Ebert
G. Clark
S. A. Fuselier
F. Allegrini
F. Bagenal
S. J. Bolton
G. A. DiBraccio
R. J. Wilson
author_facet J. Montgomery
R. W. Ebert
G. Clark
S. A. Fuselier
F. Allegrini
F. Bagenal
S. J. Bolton
G. A. DiBraccio
R. J. Wilson
author_sort J. Montgomery
collection DOAJ
description Abstract In this study, observations from the Jovian auroral distributions experiment, Jupiter energetic particle detector instrument, and Magnetic field investigation instruments on Juno are used to identify signatures of magnetic reconnection at Jupiter's dawn magnetopause and relate these signatures to the local plasma environment. Magnetopause crossings occurred between 73–114 Jovian radii and 4.3–6.2 magnetic local time at low latitudes. Reconnection signatures include plasma energization and ion velocity enhancements resembling reconnection jets. We test for diamagnetic suppression which considers the magnetic shear and plasma beta (β) before and after a magnetopause crossing. Findings show that a large majority of these dawn magnetopause crossings at Jupiter have a low likelihood for local magnetic reconnection (are diamagnetically suppressed) because of high delta β values and/or low magnetic shear angles across the magnetopause boundary. These crossings exhibit no evidence of local reconnection while crossings that are not diamagnetically suppressed show multiple signatures of reconnection, adhering to the Swisdak relation.
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series Geophysical Research Letters
spelling doaj-art-8c1de08197174bccabbf0e35ecde3b592025-08-20T03:14:16ZengWileyGeophysical Research Letters0094-82761944-80072022-07-014914n/an/a10.1029/2022GL099141Investigating the Occurrence of Magnetic Reconnection at Jupiter's Dawn Magnetopause During the Juno EraJ. Montgomery0R. W. Ebert1G. Clark2S. A. Fuselier3F. Allegrini4F. Bagenal5S. J. Bolton6G. A. DiBraccio7R. J. Wilson8Department of Physics and Astronomy University of Texas at San Antonio San Antonio TX USADepartment of Physics and Astronomy University of Texas at San Antonio San Antonio TX USAJohns Hopkins University Applied Physics Lab Laurel MD USADepartment of Physics and Astronomy University of Texas at San Antonio San Antonio TX USADepartment of Physics and Astronomy University of Texas at San Antonio San Antonio TX USALaboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder CO USASouthwest Research Institute San Antonio TX USANASA Goddard Space Flight Center Greenbelt MD USALaboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder CO USAAbstract In this study, observations from the Jovian auroral distributions experiment, Jupiter energetic particle detector instrument, and Magnetic field investigation instruments on Juno are used to identify signatures of magnetic reconnection at Jupiter's dawn magnetopause and relate these signatures to the local plasma environment. Magnetopause crossings occurred between 73–114 Jovian radii and 4.3–6.2 magnetic local time at low latitudes. Reconnection signatures include plasma energization and ion velocity enhancements resembling reconnection jets. We test for diamagnetic suppression which considers the magnetic shear and plasma beta (β) before and after a magnetopause crossing. Findings show that a large majority of these dawn magnetopause crossings at Jupiter have a low likelihood for local magnetic reconnection (are diamagnetically suppressed) because of high delta β values and/or low magnetic shear angles across the magnetopause boundary. These crossings exhibit no evidence of local reconnection while crossings that are not diamagnetically suppressed show multiple signatures of reconnection, adhering to the Swisdak relation.https://doi.org/10.1029/2022GL099141solar windmagnetosphereJupiterJunomagnetic reconnectionplasma
spellingShingle J. Montgomery
R. W. Ebert
G. Clark
S. A. Fuselier
F. Allegrini
F. Bagenal
S. J. Bolton
G. A. DiBraccio
R. J. Wilson
Investigating the Occurrence of Magnetic Reconnection at Jupiter's Dawn Magnetopause During the Juno Era
Geophysical Research Letters
solar wind
magnetosphere
Jupiter
Juno
magnetic reconnection
plasma
title Investigating the Occurrence of Magnetic Reconnection at Jupiter's Dawn Magnetopause During the Juno Era
title_full Investigating the Occurrence of Magnetic Reconnection at Jupiter's Dawn Magnetopause During the Juno Era
title_fullStr Investigating the Occurrence of Magnetic Reconnection at Jupiter's Dawn Magnetopause During the Juno Era
title_full_unstemmed Investigating the Occurrence of Magnetic Reconnection at Jupiter's Dawn Magnetopause During the Juno Era
title_short Investigating the Occurrence of Magnetic Reconnection at Jupiter's Dawn Magnetopause During the Juno Era
title_sort investigating the occurrence of magnetic reconnection at jupiter s dawn magnetopause during the juno era
topic solar wind
magnetosphere
Jupiter
Juno
magnetic reconnection
plasma
url https://doi.org/10.1029/2022GL099141
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