Why does the radio activity accompanying the flares in the two large active regions of June 1982 differ so much?

Title:

Why does the radio activity accompanying the flares in the two large active regions of June 1982 differ so much?

Creator:

Bumba, V. and Klvaňa, M.

Identifier:

https://cdk.lib.cas.cz/client/handle/uuid:d5f34422-1e17-4c99-ac23-5c81fe1738f5
uuid:d5f34422-1e17-4c99-ac23-5c81fe1738f5

Subject:

heliophysics, radio-emission activity, and flares

Type:

model:article and TEXT

Format:

bez média and svazek

Description:

An attempt is presented to explain the large difference in the intensity, frequency range and number of radio activity events following the large flares in the two complex active regions of June 1982 (NOAA Nos. 3763 and 3776). The topology of their local magnetic fields in relation to the global field is discussed as one of the main factors causing this effect.

Language:

Czech

Rights:

http://creativecommons.org/publicdomain/mark/1.0/
policy:public

Coverage:

21-24

Source:

Publications of the Astronomical Institute of the Academy of Sciences of the Czech Republic | 1998 Volume:87-88 | Number:88

Harvested from:

CDK

Metadata only:

false