Analisis Empirik Kejadian Flare Terkait Dengan Perubahan Fisik Sunspot  

Oleh:

Dani, Tiar ; J, Suprijatno ; Gunawan A.

Jenis: Article from Journal - ilmiah nasional
Dalam koleksi: Majalah Sains dan Teknologi Dirgantara (Fulltext) vol. 2 no. 3 (Sep. 2007), page 122-131.
Topik: Perubahan Fisik Sunspot
Fulltext: MM32_02_03_Tiar Dani.pdf (218.37KB)

Ketersediaan

Perpustakaan Pusat (Semanggi) Nomor Panggil: MM32 Non-tandon: 1 (dapat dipinjam: 0) Tandon: tidak ada

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Isi artikel

Sunspot class and magnetic field complexity of the sunspot group, determine the productivity of the flare production. Sunspot group class that most productive for flare appearance is FKC, and for magnetic complexity class is BGD. At the moment of maximum sunspot group area, magnetic complexity B are the most appearance. Magnetic complexity B, BG, and BGD are productive for flare occurrence.

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