Email this article 
Simulation of current sheet in the Jupiter’s near magnetotail
- Authors: Setsko P.V.1
-
Affiliations:
- Polar Geophysical Institute
- Issue: Vol 87, No 2 (2023)
- Pages: 248-253
- Section: Articles
- URL: https://rjeid.com/0367-6765/article/view/654485
- DOI: https://doi.org/10.31857/S0367676522700442
- EDN: https://elibrary.ru/AIIYWI
- ID: 654485
Cite item
Open Access
Access granted
Subscription or Fee Access
Abstract
We considered numerical modeling of the current sheet in the Jupiter’s near magnetotail to estimate the possible range of parameters of this layer depending on the presence of hot sulfur and oxygen ions. The characteristics of the obtained stationary configurations of the current sheet formed by counterflows of either protons alone, or oxygen ions alone, or sulfur ions alone, are in good agreement with the Juno’s data.
About the authors
P. V. Setsko
Polar Geophysical Institute
Author for correspondence.
Email: setsko@pgia.ru
Russia, 184209, Apatity
References
- Artemyev A.V., Vasko I.Y., Kasahara S. // Planet. Space Sci. 2014. V. 96. P. 133.
- Zhang X.-J., Ma Q., Artemyev A.V. et al. // J. Geophys. Res. Space Phys. 2020. V. 125. No. 8. Art. No. e2020JA027957.
- Kistler L.M., Mouikis C.G., Cao X. et al. // J. Geophys. Res. 2006. V. 111. No. A11. Art. No. A11222.
- Kronberg E.A., Ashour-Abdalla M., Dandouras I. et al. // Space Sci. Rev. 2014. V. 184. P. 173.
- Artemyev A. V., Angelopoulos V., Runov A., Zhang X.-J. // J. Geophys. Res. Space Phys. 2020. V. 125. No. 7. Art. No. e2019JA027612.
- Мингалев О.В., Малова Х.В., Мингалев И.В. и др. // Физика плазмы. 2018. Т. 44. № 10. С. 769.
- Мингалев О.В., Сецко П.В., Мельник М.Н. и др. // Физика плазмы. 2022. Т. 48. № 3. С. 237.
- Зеленый Л.М., Малова Х.В., Артемьев А.В. и др. // Физика плазмы. 2011. Т. 37. № 2. С. 137.
- Зеленый Л.М., Малова Х.В., Григоренко Е.Е., Попов В.Ю. // УФН. 2016. Т. 186. № 11. С. 1153.
- Мингалев О.В., Сецко П.В., Мельник М.Н. и др. // Солн.-земн. физ. 2021. Т. 7. № 2. С. 12.
Supplementary files
