Do the Throat Auroras Create Polar Cap Patches?

Abstract Throat auroras and polar cap patches are common phenomena in the polar ionosphere resulting from magnetosphere‐ionosphere coupling. A campaign was organized, with all‐sky imagers at Yellow River Station, the European Incoherent Scatter Svalbard Radar, and coordinated low‐altitude spacecraft...

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Bibliographic Details
Published in:Geophysical Research Letters
Main Authors: Duan Zhang, Qing‐He Zhang, Kjellmar Oksavik, Tong Xu, Zan‐Yang Xing, L. R. Lyons, De‐Sheng Han, Hong‐Bo Zhang, Yu‐Zhang Ma, Ze‐Jun Hu, Jian‐Jun Liu, Yong Wang, Xiang‐Yu Wang
Format: Article in Journal/Newspaper
Language:English
Published: Wiley 2023
Subjects:
throat aurora
polar cap patch
polar ionosphere
magnetosphere‐ionosphere coupling
Geophysics. Cosmic physics
QC801-809
Svalbard
Online Access:https://doi.org/10.1029/2022GL102263
https://doaj.org/article/f2305ecca46043329fcffdf4c7cc30b8
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Summary:Abstract Throat auroras and polar cap patches are common phenomena in the polar ionosphere resulting from magnetosphere‐ionosphere coupling. A campaign was organized, with all‐sky imagers at Yellow River Station, the European Incoherent Scatter Svalbard Radar, and coordinated low‐altitude spacecraft observations. During periods of radial interplanetary magnetic field (IMF), observations showed that, as poleward moving throat auroras faded around the polar cap boundary, they linked to poleward moving ionization patches. The throat auroras were produced by soft‐electron precipitation associated with dayside magnetic reconnection. The red line emission intensity of throat auroras was correlated with dayside reconnection events. Dense plasma from lower latitudes was transported poleward via enhanced convection in the throat auroras to form patches. This is a potentially new formation mechanism for patches associated with throat auroras and magnetic reconnection for radial IMF. Moreover, the patches move anti‐sunward due to the E × B drift.

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