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Title: Electron Energization by Inertial Alfvén Waves in Density Depleted Flux Tubes at Jupiter

Abstract

Juno satellite observations have illustrated substantial examples of broadband electron energization up to 105–106 eV levels. In order to explain these observations, we use a hybrid gyrofluid kinetic-electron model in an untilted dipolar topology to illustrate energization to high levels in weak current conditions by inertial Alfvén waves close to the Jupiter ionosphere for ambient plasma densities and magnetic field perturbations inferred from Juno satellite observations. The key to the high energization is the extremely low densities evident in the observations which necessitates the acceleration of electrons to very high velocities in order to carry the field-aligned current.

Authors:
ORCiD logo [1]; ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [3]; ORCiD logo [1]
  1. Univ. of Alaska, Fairbanks, AK (United States)
  2. Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States)
  3. Andrews Univ., Berrien Springs, MI (United States)
Publication Date:
Research Org.:
Princeton Plasma Physics Laboratory (PPPL), Princeton, NJ (United States)
Sponsoring Org.:
USDOE Office of Science (SC), Fusion Energy Sciences (FES); National Aeronautics and Space Administration (NASA)
OSTI Identifier:
1974426
Grant/Contract Number:  
AC02-09CH11466; 80NSSC19K0941; 80NSSC20K1279; 80NSSC19K0843; 80HQTR19T0076
Resource Type:
Accepted Manuscript
Journal Name:
Geophysical Research Letters
Additional Journal Information:
Journal Volume: 50; Journal Issue: 5; Journal ID: ISSN 0094-8276
Publisher:
American Geophysical Union (AGU)
Country of Publication:
United States
Language:
English
Subject:
58 GEOSCIENCES

Citation Formats

Damiano, P. A., Delamere, P. A., Kim, E. ‐H., Johnson, J. R., and Ng, C. S. Electron Energization by Inertial Alfvén Waves in Density Depleted Flux Tubes at Jupiter. United States: N. p., 2023. Web. doi:10.1029/2022gl102467.
Damiano, P. A., Delamere, P. A., Kim, E. ‐H., Johnson, J. R., & Ng, C. S. Electron Energization by Inertial Alfvén Waves in Density Depleted Flux Tubes at Jupiter. United States. https://doi.org/10.1029/2022gl102467
Damiano, P. A., Delamere, P. A., Kim, E. ‐H., Johnson, J. R., and Ng, C. S. Fri . "Electron Energization by Inertial Alfvén Waves in Density Depleted Flux Tubes at Jupiter". United States. https://doi.org/10.1029/2022gl102467. https://www.osti.gov/servlets/purl/1974426.
@article{osti_1974426,
title = {Electron Energization by Inertial Alfvén Waves in Density Depleted Flux Tubes at Jupiter},
author = {Damiano, P. A. and Delamere, P. A. and Kim, E. ‐H. and Johnson, J. R. and Ng, C. S.},
abstractNote = {Juno satellite observations have illustrated substantial examples of broadband electron energization up to 105–106 eV levels. In order to explain these observations, we use a hybrid gyrofluid kinetic-electron model in an untilted dipolar topology to illustrate energization to high levels in weak current conditions by inertial Alfvén waves close to the Jupiter ionosphere for ambient plasma densities and magnetic field perturbations inferred from Juno satellite observations. The key to the high energization is the extremely low densities evident in the observations which necessitates the acceleration of electrons to very high velocities in order to carry the field-aligned current.},
doi = {10.1029/2022gl102467},
journal = {Geophysical Research Letters},
number = 5,
volume = 50,
place = {United States},
year = {Fri Feb 24 00:00:00 EST 2023},
month = {Fri Feb 24 00:00:00 EST 2023}
}

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