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Periodical patterns in major flare occurrence and their relation to magnetically complex active regions (CROSBI ID 116800)

Prilog u časopisu | izvorni znanstveni rad | međunarodna recenzija

Temmer, Manuela ; Veronig, Astrid ; Rybak, Jan ; Brajša, Roman ; Hanslmeier, Arnold Periodical patterns in major flare occurrence and their relation to magnetically complex active regions // Advances in space research, 38 (2006), 5; 886-890-x

Podaci o odgovornosti

Temmer, Manuela ; Veronig, Astrid ; Rybak, Jan ; Brajša, Roman ; Hanslmeier, Arnold

engleski

Periodical patterns in major flare occurrence and their relation to magnetically complex active regions

A periodical occurrence rate of major solar flares (observed in hard X-rays) of ~24 days (synodic) was first reported by Bai (1987) for the years 1980-1985. Here we report a significant relation between the appearance of 24-day period in major H-alpha flares and magnetically complex sunspot groups (i.e., including a gamma and/or delta configuration). From synoptic maps of magnetograms (NSO/KP) patterns in the magnetic flux evolution are traced which might be the cause of the 24-day period observed in flare activity.

solar flares; solar activity; magnetic fields

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Podaci o izdanju

38 (5)

2006.

886-890-x

objavljeno

0273-1177

Povezanost rada

Fizika

Indeksiranost