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Konfigurasi Medan Magnetik Daerah Aktif Di Matahari yang Menghasilkan Flare
Oleh:
Yatini, Clara Yono
Jenis:
Article from Bulletin/Magazine
Dalam koleksi:
Warta Lapan vol. 2 no. 3 (Jun. 2000)
,
page 108-114.
Ketersediaan
Perpustakaan Pusat (Semanggi)
Nomor Panggil:
WW20.2
Non-tandon:
1 (dapat dipinjam: 0)
Tandon:
tidak ada
Lihat Detail Induk
Isi artikel
Studied the magnetic field structure of six active regions in its relation to flare productivity. Three of these active regions (NOAA 5629, NOAA 6089, and NOAA 6919) produced many flares, both big flare and subflare, while the others (NOAA 5625, NOAA 6110, and NOAA 6926) did not. According to Somov’s Model of Potential Field, we conclude that the configuration of flaring active regions are more complex than the nonflaring ones.
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