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Solar and stellar flares and their impact on planets

Published online by Cambridge University Press:  09 September 2016

Kazunari Shibata
Kazunari Shibata*
Affiliation:
Kwasan and Hida Observatories, Kyoto University, Yamashina, Kyoto, Japan, 607-8471 email: shibata@kwasan.kyoto-u.ac.jp
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Abstract

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Recent observations of the Sun revealed that the solar atmosphere is full of flares and flare-like phenomena, which affect terrestrial environment and our civilization. It has been established that flares are caused by the release of magnetic energy through magnetic reconnection. Many stars show flares similar to solar flares, and such stellar flares especially in stars with fast rotation are much more energetic than solar flares. These are called superflares. The total energy of a solar flare is 1029 − 1032 erg, while that of a superflare is 1033 − 1038 erg. Recently, it was found that superflares (with 1034 − 1035 erg) occur on Sun-like stars with slow rotation with frequency once in 800 - 5000 years. This suggests the possibility of superflares on the Sun. We review recent development of solar and stellar flare research, and briefly discuss possible impacts of superflares on the Earth and exoplanets.

Keywords

stars:activitystars:flarestars:rotationstars:solar-typestars:starspots

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