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- Publisher Website: 10.26464/epp2017007
- Scopus: eid_2-s2.0-85029486173
- WOS: WOS:000448261800007
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Article: Observations of loading-unloading process at Saturn's distant magnetotail
Title | Observations of loading-unloading process at Saturn's distant magnetotail |
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Authors | |
Keywords | dipolarization loading-unloading process magnetic reconnection saturn magnetosphere |
Issue Date | 2017 |
Citation | Earth and Planetary Physics, 2017, v. 1, n. 1, p. 53-57 How to Cite? |
Abstract | Using in-situ measurements from the Cassini spacecraft in 2013, we report an Earth substorm-like loading-unloading process at Saturn's distant magnetotail. We found that the loading process is featured with two distinct processes: a rapid loading process that was likely driven by an internal source and a slow loading process that was likely driven by solar wind. Each of the two loading processes could also individually lead to an unloading process. The rapid internal loading process lasts for ~ 1–2 hours; the solar wind driven loading process lasts for ~ 3–18 hours and the following unloading process lasts for ~1–3 hours. In this letter, we suggest three possible loading-unloading circulations, which are fundamental in understanding the role of solar wind in driving giant planetary magnetospheric dynamics. |
Persistent Identifier | http://hdl.handle.net/10722/334499 |
ISSN | 2023 Impact Factor: 2.5 2023 SCImago Journal Rankings: 0.674 |
ISI Accession Number ID |
DC Field | Value | Language |
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dc.contributor.author | Yao, Zhong Hua | - |
dc.date.accessioned | 2023-10-20T06:48:35Z | - |
dc.date.available | 2023-10-20T06:48:35Z | - |
dc.date.issued | 2017 | - |
dc.identifier.citation | Earth and Planetary Physics, 2017, v. 1, n. 1, p. 53-57 | - |
dc.identifier.issn | 2096-3955 | - |
dc.identifier.uri | http://hdl.handle.net/10722/334499 | - |
dc.description.abstract | Using in-situ measurements from the Cassini spacecraft in 2013, we report an Earth substorm-like loading-unloading process at Saturn's distant magnetotail. We found that the loading process is featured with two distinct processes: a rapid loading process that was likely driven by an internal source and a slow loading process that was likely driven by solar wind. Each of the two loading processes could also individually lead to an unloading process. The rapid internal loading process lasts for ~ 1–2 hours; the solar wind driven loading process lasts for ~ 3–18 hours and the following unloading process lasts for ~1–3 hours. In this letter, we suggest three possible loading-unloading circulations, which are fundamental in understanding the role of solar wind in driving giant planetary magnetospheric dynamics. | - |
dc.language | eng | - |
dc.relation.ispartof | Earth and Planetary Physics | - |
dc.subject | dipolarization | - |
dc.subject | loading-unloading process | - |
dc.subject | magnetic reconnection | - |
dc.subject | saturn magnetosphere | - |
dc.title | Observations of loading-unloading process at Saturn's distant magnetotail | - |
dc.type | Article | - |
dc.description.nature | link_to_subscribed_fulltext | - |
dc.identifier.doi | 10.26464/epp2017007 | - |
dc.identifier.scopus | eid_2-s2.0-85029486173 | - |
dc.identifier.volume | 1 | - |
dc.identifier.issue | 1 | - |
dc.identifier.spage | 53 | - |
dc.identifier.epage | 57 | - |
dc.identifier.isi | WOS:000448261800007 | - |