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Appearance and Precipitation Characteristics of High-Latitude Pulsating Aurora

Authors :
Noora Partamies
Fasil Tesema
Emma Bland
Source :
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
Publication Year :
2022
Publisher :
Frontiers Media S.A., 2022.

Abstract

Characteristics of pulsating aurora (PsA) at the equatorward part of the auroral oval have been well described in the literature by previous studies. We extend our knowledge on high-latitude PsA observations by analysing 68 PsA events from the optical observatory on Svalbard, at 75° magnetic latitude. We found that the pulsating emission structures are particularly large and transient, they do not experience drift motion, or their drift motion cannot be traced. Our results show that the high-latitude PsA events relate to lower geomagnetic activity and weaker solar wind driving than the lower latitude PsA. The high-latitude PsA events also occur less frequently, which is in agreement with their association to lower-than-average geomagnetic activity. We further show that the ionospheric electron density values during high-latitude PsA events are low compared to the lower latitude PsA. This, together with the non-traceable nature of the pulsating emission structures, suggests that these events are strongly dominated by a sub-type called Amorphous Pulsating Aurora (APA). We therefore conclude that, unlike the lower latitude PsA events, the high-latitude PsA events are not likely to cause direct changes in the chemical composition of the mesosphere.

Details

Language :
English
ISSN :
2296987X
Volume :
9
Database :
Directory of Open Access Journals
Journal :
Frontiers in Astronomy and Space Sciences
Publication Type :
Academic Journal
Accession number :
edsdoj.0ac65a7ccace4e059a80dd44a56dd939
Document Type :
article
Full Text :
https://doi.org/10.3389/fspas.2022.923396