中文版 | English
Title

Dynamic Jovian Magnetosphere Responses to Enhanced Solar Wind Ram Pressure: Implications for Auroral Activities

Author
Corresponding AuthorZhang, Binzheng
Publication Years
2022-10-16
DOI
Source Title
ISSN
0094-8276
EISSN
1944-8007
Volume49Issue:19
Abstract
The main emission (ME) of the Jovian aurora is thought to be related to the current system associated with the breakdown of plasma corotation in the middle magnetosphere. According to the mainstream corotation breakdown model, the intensity of the Jovian ME is expected to decrease when the solar wind (SW) ram pressure increases, which is not fully consistent with auroral observations. In addition to the field-aligned current (FAC), Alfvenic power (AP) play an important role in regulating planetary auroral emissions. We use three-dimensional global simulations to investigate how these proxies of auroral emission respond to enhanced SW ram pressure. We found that during SW compression, both FAC and AP experience up-down-up trends, which is not revealed by any previous simulations, while could potentially explain many observations. The results suggest that different Jovian auroral activities including brightening or dimming can be observed during SW compression period.
Keywords
URL[Source Record]
Indexed By
Language
English
Important Publications
NI Journal Papers
SUSTech Authorship
Others
Funding Project
National Natural Science Foundation of China[41922060] ; RGC General Research Fund["17300719","17308520"] ; Key Research Program of the Institute of Geology and Geophysics, CAS[IGGCAS-201904] ; NASA["80NSSC19K0822","80NSSC20K1279"] ; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB 41000000]
WOS Research Area
Geology
WOS Subject
Geosciences, Multidisciplinary
WOS Accession No
WOS:000865787800001
Publisher
ESI Research Field
GEOSCIENCES
Data Source
Web of Science
Citation statistics
Cited Times [WOS]:0
Document TypeJournal Article
Identifierhttp://kc.sustech.edu.cn/handle/2SGJ60CL/405946
DepartmentDepartment of Earth and Space Sciences
Affiliation
1.Univ Hong Kong, Dept Phys, Hong Kong, Peoples R China
2.Univ Hong Kong, Dept Earth Sci, Hong Kong, Peoples R China
3.Chinese Acad Sci, Inst Geol & Geophys, Beijing, Peoples R China
4.Univ Alaska Fairbanks, Dept Phys, Fairbanks, AK USA
5.OJ Brambles Consulting, Preston, Lancs, England
6.Southern Univ Sci & Technol, Dept Earth & Space Sci, Shenzhen, Peoples R China
7.Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA
Recommended Citation
GB/T 7714
Feng, Enhao,Zhang, Binzheng,Yao, Zhonghua,et al. Dynamic Jovian Magnetosphere Responses to Enhanced Solar Wind Ram Pressure: Implications for Auroral Activities[J]. GEOPHYSICAL RESEARCH LETTERS,2022,49(19).
APA
Feng, Enhao.,Zhang, Binzheng.,Yao, Zhonghua.,Delamere, Peter A..,Zheng, Zhiqi.,...&Sorathia, Kareem A..(2022).Dynamic Jovian Magnetosphere Responses to Enhanced Solar Wind Ram Pressure: Implications for Auroral Activities.GEOPHYSICAL RESEARCH LETTERS,49(19).
MLA
Feng, Enhao,et al."Dynamic Jovian Magnetosphere Responses to Enhanced Solar Wind Ram Pressure: Implications for Auroral Activities".GEOPHYSICAL RESEARCH LETTERS 49.19(2022).
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