Statistical studies of duration of low-power solar flares

Author:

Боровик Александр1,Borovik Aleksandr2,Жданов Антон1,Zhdanov Anton2

Affiliation:

1. Институт солнечно-земной физики СО РАН

2. Institute of Solar Terrestrial Physics SB RAS

Abstract

This paper is a sequel to papers dealing with time parameters of solar flares in the Hα line. Using data from the international flare patrol for 1972–2010, we have determined the mean duration of flares of different importance and classes of area. We have established that 94.6 % of flares last more than 60 min. The duration of 90 % of flares with min is 2.1–3.3 hrs. In rare cases, flares can last about 12 hrs. The duration of powerful solar flares does not exceed 8.3 hrs. We have found that the duration of solar flares depends on features of their development. Flares with one brilliant point in the flare region have the shortest duration; two-ribbon flares and flares exhibiting several intensity maxima have the longest duration. We have confirmed that the duration of flares increases with increasing classes of area and brightness.

Publisher

Infra-M Academic Publishing House

Subject

Space and Planetary Science,Atmospheric Science,Geophysics

Reference28 articles.

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5. Borovik A.V., Zhdanov A.A. Statistical studies of low-power solar flares. Main phase duration. Solar-Terrestrial Physics. 2017a, vol. 3, no. 4, pp. 5–16. DOI: 10.12737/stp-34201701., Borovik A.V., Zhdanov A.A. Statistical studies of low-power solar flares. Main phase duration. Solar-Terrestrial Physics. 2017a, vol. 3, no. 4, pp. 5–16. DOI: 10.12737/stp-34201701.

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