z-logo
open-access-imgOpen Access
Spectral and photometric characteristics of mid-latitude auroras during the magnetic storm of March 17, 2015
Author(s) -
A. V. Mikhalëv,
A. V. Mikhalëv,
Александр Белецкий,
Aleksandr Beletsky,
Роман Васильев,
Roman Vasilyev,
Г. А. Жеребцов,
G. A. Zherebtsov,
Степан Подлесный,
Stepan Podlesny,
Михаил Тащилин,
Михаил Тащилин,
Максим Артамонов,
Максим Артамонов
Publication year - 2018
Publication title -
solnechno-zemnaya fizika
Language(s) - English
Resource type - Journals
ISSN - 2412-4737
DOI - 10.12737/szf-44201806
Subject(s) - latitude , geomagnetic storm , storm , geomagnetic latitude , low latitude , earth's magnetic field , ionosphere , middle latitudes , geology , atmospheric sciences , climatology , physics , meteorology , geophysics , geodesy , magnetic field , quantum mechanics
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).

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom