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DOI | 10.1029/2020GL089818 |
Polar Flattening of Jupiter's Magnetosphere | |
Ranquist D.A.; Bagenal F.; Wilson R.J. | |
发表日期 | 2020 |
ISSN | 0094-8276 |
卷号 | 47期号:16 |
英文摘要 | Jupiter's magnetosphere is filled with plasma that expands from Io into an equatorial plasma disk, which preferentially inflates the magnetosphere against the solar wind equatorially. This results in a polar flattened magnetosphere and changes the dynamics between the solar wind and the magnetopause boundary. The degree of polar flattening at Jupiter, however, is not well known because no spacecraft has traversed the magnetopause at high latitudes. Instead, estimates must be made from much lower latitudes. In this study, we present a new method of estimating the large-scale shape of magnetospheres by using magnetic field draping within the magnetosheath. Utilizing data of Jupiter's dawn magnetosheath from the Juno spacecraft, we estimate the ratio of the semimajor to semiminor axes of the Jupiter-Sun-North Y-Z elliptical cross section of Jupiter's magnetopause is 1.29 ± 0.29. ©2020. American Geophysical Union. All Rights Reserved. |
英文关键词 | Solar wind; Elliptical cross section; Equatorial plasma disk; High Latitudes; Jupiter's magnetosphere; Jupiters; Magnetosheaths; Magnetopause; Jupiter; magnetic field; magnetopause; magnetosphere; plasma; polar region; solar wind; spacecraft |
语种 | 英语 |
来源期刊 | Geophysical Research Letters
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文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/169935 |
作者单位 | Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, CO, United States |
推荐引用方式 GB/T 7714 | Ranquist D.A.,Bagenal F.,Wilson R.J.. Polar Flattening of Jupiter's Magnetosphere[J],2020,47(16). |
APA | Ranquist D.A.,Bagenal F.,&Wilson R.J..(2020).Polar Flattening of Jupiter's Magnetosphere.Geophysical Research Letters,47(16). |
MLA | Ranquist D.A.,et al."Polar Flattening of Jupiter's Magnetosphere".Geophysical Research Letters 47.16(2020). |
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