Spectral and photometric characteristics of mid-latitude auroras during the magnetic storm of March 17, 2015

Автор: Mikhalev A.V., Beletsky A.B., Vasilyev R.V., Zherebtsov G.A., Podlesny S.V., Tashchilin M.A., Artamonov M.F.

Журнал: Солнечно-земная физика @solnechno-zemnaya-fizika

Статья в выпуске: 4 т.4, 2018 года.

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We study the spatiotemporal dynamics of mid-latitude aurora from observations in the south of Eastern Siberia during St. Patrick’s severe geomagnetic storm on March 17, 2015. We perform a morphological analysis of characteristics of the observed auroras. A preliminary conclusion is drawn that the analyzed event is the result of the manifestation of mid-latitude auroras of two types (type “d” and SAR arc) and ordinary aurora observed at the northern horizon. The maximum intensity of the dominant emission [OI] at 630.0 nm (~14 kR) allows this mid-latitude aurora to be attributed to the extreme auroras occurring in mid-latitudes, which is second only to the November 20, 2003 superstorm (~19 kR).

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Geomagnetic storm, mid-latitude aurora, spectrum of mid-latitude aurora, 557.7 and 630.0 nm emissions

Короткий адрес: https://sciup.org/142220309

IDR: 142220309   |   DOI: 10.12737/szf-44201806

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