Distribution of low-power solar flares by brightness rise time

Using data from the international flare patrol for 1972–2010, we have formed an electronic database for more than 123 thousand solar flares. We determined the mean brightness rise time (flash phase) for flare area classes and importance. We show that the mean flash phase increased with increasing ar...

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Bibliographic Details
Main Authors: Borovik A.V., Zhdanov A.A.
Format: Article
Language:English
Published: INFRA-M 2018-09-01
Series:Solar-Terrestrial Physics
Subjects:
Online Access:https://naukaru.ru/en/nauka/article/23002/view