Journal article
Properties of Ion-Inertial Scale Plasmoids Observed by the Juno Spacecraft in the Jovian Magnetotail
Journal of geophysical research. Space physics, Vol.127(3), pp.e2021JA030181-n/a
03/01/2022
DOI: 10.1029/2021JA030181
PMCID: PMC9286786
PMID: 35865743
Abstract
We expand on previous observations of magnetic reconnection in Jupiter's magnetosphere by constructing a survey of ion-inertial scale plasmoids in the Jovian magnetotail. We developed an automated detection algorithm to identify reversals in the B theta ${B}_{\theta }$ component and performed the minimum variance analysis for each identified plasmoid to characterize its helical structure. The magnetic field observations were complemented by data collected using the Juno Waves instrument, which is used to estimate the total electron density, and the JEDI energetic particle detectors. We identified 87 plasmoids with "peak-to-peak" durations between 10 and 300 s. Thirty-one plasmoids possessed a core field and were classified as flux-ropes. The other 56 plasmoids had minimum field strength at their centers and were termed O-lines. Out of the 87 plasmoids, 58 had in situ signatures shorter than 60 s, despite the algorithm's upper limit being 300 s, suggesting that smaller plasmoids with shorter durations were more likely to be detected by Juno. We estimate the diameter of these plasmoids assuming a circular cross section and a travel speed equal to the Alfven speed in the surrounding lobes. Using the electron density inferred by Waves, we contend that these plasmoid diameters were within an order of the local ion-inertial length. Our results demonstrate that magnetic reconnection in the Jovian magnetotail occurs at ion scales like in other space environments. We show that ion-scale plasmoids would need to be released every 0.1 s or less to match the canonical 1 ton/s rate of plasma production due to Io.
Details
- Title: Subtitle
- Properties of Ion-Inertial Scale Plasmoids Observed by the Juno Spacecraft in the Jovian Magnetotail
- Creators
- Yash Sarkango - University of MichiganJames A. Slavin - University of MichiganXianzhe Jia - University of MichiganGina A. DiBraccio - Goddard Space Flight CenterGeorge B. Clark - Johns Hopkins University Applied Physics LaboratoryWeijie Sun - University of MichiganBarry H. Mauk - Johns Hopkins University Applied Physics LaboratoryWilliam S. Kurth - University of IowaGeorge B. Hospodarsky - University of Iowa
- Resource Type
- Journal article
- Publication Details
- Journal of geophysical research. Space physics, Vol.127(3), pp.e2021JA030181-n/a
- DOI
- 10.1029/2021JA030181
- PMID
- 35865743
- PMCID
- PMC9286786
- NLM abbreviation
- J Geophys Res Space Phys
- ISSN
- 2169-9380
- eISSN
- 2169-9402
- Publisher
- Amer Geophysical Union
- Number of pages
- 24
- Grant note
- 80NSSC17K0604; 80NSSC20K1286; 699041X / NASA; National Aeronautics & Space Administration (NASA) Southwest Research Institute
- Language
- English
- Date published
- 03/01/2022
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984455553202771
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