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Астрофизический семинар ИНАСАН № 2 (8 Февраля 2001 г., 11:00)

Опубликовано: 08/02/2001

Докладчик: Г.С. Бисноватый-Коган

Название доклада: “Магниторотационные модели взрыва: сверхновые и образование джетов”

Краткое содержание доклада:
Magnetorotational explosion is based on using of the rotational energy, which is transformed into the energy of the outburst with the help of a magnetic field. 2-D MHD calculations are performed wich gave an efficiency of transformation of the order of 10 percent. The geometry of the explosion depends on the topology of a magnetic field. Equatorial and jet-like outbursts have been obtained. Asymmetric one-side ejections could also be formed in such explosions. The talk is based on works made together with N.V.Ardelyan (MGU) and S.G.Moiseenko (IKI).

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