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Article: A statistical analysis and comparison of the fine structures of the ion upflow associated with the double-peak subauroral ion drift

TitleA statistical analysis and comparison of the fine structures of the ion upflow associated with the double-peak subauroral ion drift
Authors
Keywordsdouble-peak subauroral ion drift
frictional heating
ion upflow
subauroral ion drift
subauroral polarization streams
Issue Date2023
Citation
Frontiers in Astronomy and Space Sciences, 2023, v. 10, article no. 1254243 How to Cite?
AbstractThe ion upflow associated with the subauroral ion drift (SAID) is a crucial component in the exchange of particles between the ionosphere and the ring currents. The ion upflow associated with the double-peak subauroral ion drift (DSAID), which is a subclass of the SAID, is more complex compared to SAID. In this study, we conducted a statistical analysis of the ion upflow associated with DSAID using Defense Meteorological Satellite Program (DMSP) F16–F18 data spanning 11 years (2010–2020) in the Northern Hemisphere. Our findings revealed that ion upflow associated with DSAID can exhibit either a double-peak or a one-peak upflow. The statistical characteristics of these two types of events displayed significant differences. In DSAID with a double-peak upflow event, the velocity of DSAID around the high-latitude peak was greater than that around the low-latitude peak. However, in DSAID with a one-peak upflow event, the DSAID velocities around the two peaks were very similar. Based on the formation mechanism of DSAID and the process of frictional heating in the ionosphere, we proposed that the formation of DSAID with a double-peak upflow and DSAID with a one-peak upflow are likely related to the formation process of DSAID.
Persistent Identifierhttp://hdl.handle.net/10722/347074

 

DC FieldValueLanguage
dc.contributor.authorZhang, Qiang-
dc.contributor.authorHan, De Sheng-
dc.contributor.authorTeng, Shang Chun-
dc.contributor.authorWang, Zhi Wei-
dc.contributor.authorZhang, Q. H.-
dc.contributor.authorXing, Zan Yang-
dc.contributor.authorWang, Yong-
dc.contributor.authorMa, Yu Zhang-
dc.date.accessioned2024-09-17T04:15:11Z-
dc.date.available2024-09-17T04:15:11Z-
dc.date.issued2023-
dc.identifier.citationFrontiers in Astronomy and Space Sciences, 2023, v. 10, article no. 1254243-
dc.identifier.urihttp://hdl.handle.net/10722/347074-
dc.description.abstractThe ion upflow associated with the subauroral ion drift (SAID) is a crucial component in the exchange of particles between the ionosphere and the ring currents. The ion upflow associated with the double-peak subauroral ion drift (DSAID), which is a subclass of the SAID, is more complex compared to SAID. In this study, we conducted a statistical analysis of the ion upflow associated with DSAID using Defense Meteorological Satellite Program (DMSP) F16–F18 data spanning 11 years (2010–2020) in the Northern Hemisphere. Our findings revealed that ion upflow associated with DSAID can exhibit either a double-peak or a one-peak upflow. The statistical characteristics of these two types of events displayed significant differences. In DSAID with a double-peak upflow event, the velocity of DSAID around the high-latitude peak was greater than that around the low-latitude peak. However, in DSAID with a one-peak upflow event, the DSAID velocities around the two peaks were very similar. Based on the formation mechanism of DSAID and the process of frictional heating in the ionosphere, we proposed that the formation of DSAID with a double-peak upflow and DSAID with a one-peak upflow are likely related to the formation process of DSAID.-
dc.languageeng-
dc.relation.ispartofFrontiers in Astronomy and Space Sciences-
dc.subjectdouble-peak subauroral ion drift-
dc.subjectfrictional heating-
dc.subjection upflow-
dc.subjectsubauroral ion drift-
dc.subjectsubauroral polarization streams-
dc.titleA statistical analysis and comparison of the fine structures of the ion upflow associated with the double-peak subauroral ion drift-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.3389/fspas.2023.1254243-
dc.identifier.scopuseid_2-s2.0-85174224693-
dc.identifier.volume10-
dc.identifier.spagearticle no. 1254243-
dc.identifier.epagearticle no. 1254243-
dc.identifier.eissn2296-987X-

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