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Article: In Situ Observational Evidence of the Polar Cap Arc at 1500 MLT (15MLT-PCA) Associated With the Lobe Reconnection

TitleIn Situ Observational Evidence of the Polar Cap Arc at 1500 MLT (15MLT-PCA) Associated With the Lobe Reconnection
Authors
Keywordscusp
dayside aurora
flux transfer events
lobe reconnection
polar cap aurora
Issue Date13-Nov-2024
PublisherWiley Open Access
Citation
Geophysical Research Letters, 2024, v. 51, n. 22 How to Cite?
AbstractThe polar cap arc at 1500 MLT (15MLT-PCA) has been considered as an auroral signature of the cusp's duskside boundary and been speculated to be caused by lobe reconnection. However, no observational evidence has been provided to support this speculation. Here we report a 15MLT-PCA event occurred on 29 November 2017 using multi-instrument observations. During the DMSP observed the 15MLT-PCA, Cluster, with its footprints at the root of the 15MLT-PCA, identified two FTEs in the southern hemisphere's lobe region, accompanied by an increase in electron and ion energy from hundreds of eVs to several keVs. AMPERE observed an increase in upward field-aligned currents associated with the 15MLT-PCA. SuperDARN observed a single cell convection with an enhancement of sunward plasma flow near the root of 15MLT-PCA. We suggest that these observations provide the in-situ observational evidence that the 15MLT-PCA is generated by a lobe reconnection at the cusp's duskside boundary.
Persistent Identifierhttp://hdl.handle.net/10722/353652
ISSN
2023 Impact Factor: 4.6
2023 SCImago Journal Rankings: 1.850
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorFeng, Huiting-
dc.contributor.authorHan, Desheng-
dc.contributor.authorTeng, Shangchun-
dc.contributor.authorQiu, Huixuan-
dc.contributor.authorZhou, Su-
dc.contributor.authorShi, Run-
dc.contributor.authorZhang, Yongliang-
dc.date.accessioned2025-01-22T00:35:29Z-
dc.date.available2025-01-22T00:35:29Z-
dc.date.issued2024-11-13-
dc.identifier.citationGeophysical Research Letters, 2024, v. 51, n. 22-
dc.identifier.issn0094-8276-
dc.identifier.urihttp://hdl.handle.net/10722/353652-
dc.description.abstractThe polar cap arc at 1500 MLT (15MLT-PCA) has been considered as an auroral signature of the cusp's duskside boundary and been speculated to be caused by lobe reconnection. However, no observational evidence has been provided to support this speculation. Here we report a 15MLT-PCA event occurred on 29 November 2017 using multi-instrument observations. During the DMSP observed the 15MLT-PCA, Cluster, with its footprints at the root of the 15MLT-PCA, identified two FTEs in the southern hemisphere's lobe region, accompanied by an increase in electron and ion energy from hundreds of eVs to several keVs. AMPERE observed an increase in upward field-aligned currents associated with the 15MLT-PCA. SuperDARN observed a single cell convection with an enhancement of sunward plasma flow near the root of 15MLT-PCA. We suggest that these observations provide the in-situ observational evidence that the 15MLT-PCA is generated by a lobe reconnection at the cusp's duskside boundary.-
dc.languageeng-
dc.publisherWiley Open Access-
dc.relation.ispartofGeophysical Research Letters-
dc.rightsThis work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.-
dc.subjectcusp-
dc.subjectdayside aurora-
dc.subjectflux transfer events-
dc.subjectlobe reconnection-
dc.subjectpolar cap aurora-
dc.titleIn Situ Observational Evidence of the Polar Cap Arc at 1500 MLT (15MLT-PCA) Associated With the Lobe Reconnection-
dc.typeArticle-
dc.description.naturepublished_or_final_version-
dc.identifier.doi10.1029/2024GL111793-
dc.identifier.scopuseid_2-s2.0-85208824769-
dc.identifier.volume51-
dc.identifier.issue22-
dc.identifier.eissn1944-8007-
dc.identifier.isiWOS:001369024700001-
dc.identifier.issnl0094-8276-

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