Solar-Terrestrial Physics (Dec 2018)

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

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

DOI
https://doi.org/10.12737/stp-44201806
Journal volume & issue
Vol. 4, no. 4
pp. 42 – 47

Abstract

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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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