Dynamic Jovian Magnetosphere Responses to Enhanced Solar Wind Ram Pressure: Implications for Auroral Activities
Dynamic Jovian Magnetosphere Responses to Enhanced Solar Wind Ram Pressure: Implications for Auroral Activities
复制标题
动态木星磁层对增强太阳风冲压压力的响应:对极光活动的影响
DOI:
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复制
发表时间:
2022
影响因子:
5.2
通讯作者:
K. Sorathia
中科院分区:
文献类型:
--
作者:
Enhao Feng;Binzheng Zhang;Z. Yao;P. Delamere;Zhiqi Zheng;O. Brambles;S. Ye;K. Sorathia
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), Alfvénic 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.
DOI:
10.1029/2021ja029886
发表时间:
2021-08
期刊:
Journal of Geophysical Research: Space Physics
影响因子:
--
作者:
R. Lysak;Yan Song;S. Elliott;W. Kurth;A. Sulaiman;D. Gershman
通讯作者:
R. Lysak;Yan Song;S. Elliott;W. Kurth;A. Sulaiman;D. Gershman
DOI:
10.1016/j.jastp.2021.105616
发表时间:
2021
影响因子:
1.9
作者:
Keiling, Andreas
通讯作者:
Keiling, Andreas
影响因子:
5.2
作者:
Damiano, P. A.;Delamere, P. A.;Johnson, J. R.
通讯作者:
Johnson, J. R.