配偶 发表于 2025-3-30 08:46:33

Introduction: The Written Constitution,lack hole by electromagnetic torques is described and some recent formal developments are reviewed. It is suggested that AGN are only radio-loud when the nuclear stellar mass loss rate is low enough to allow this wind to collimate.

ERUPT 发表于 2025-3-30 14:28:45

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模范 发表于 2025-3-30 19:48:57

Gamma Ray Jets and Black Hole Magnetospheres in Active Galactic Nuclei,lack hole by electromagnetic torques is described and some recent formal developments are reviewed. It is suggested that AGN are only radio-loud when the nuclear stellar mass loss rate is low enough to allow this wind to collimate.

通情达理 发表于 2025-3-30 22:38:43

Solar Coronal Heating by Magnetic Flux Interaction,ing magnetic features that are usually observed to be present in the photosphere below bright points. The model has three phases: a preinteraction phase in which two opposite polarity photospheric magnetic fragments are unconnected magnetically; an interaction phase when the fragments reconnect in t

阻塞 发表于 2025-3-31 01:05:23

Magnetic Energy Dissipation and Coronal Heating by DC Currents, a high temperature of 10.K, and occasionally producing spectacular solar flares. The energy flux needed to balance the losses by radiation or by the solar wind of non-flaring coronal gas ranges between several 10. ergs cm. . . in quiet regions to 10. ergs cm. . . in active regions. Coronal holes do

Merited 发表于 2025-3-31 08:35:20

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货物 发表于 2025-3-31 09:49:38

MHD Winds and Jets,mptotically conical winds and cylindrical jets. A class of exact solutions of those MHD equations is studied, which is constructed via a judicious albeit simple choice of the dependence of the physical quantities on the appropriate streamline coordinates. This analytical example is reperesentative h

诽谤 发表于 2025-3-31 14:41:27

Magnetic White Dwarfs,ffect in spectral lines and of broad-band continuum polarization. Known magnetic white dwarfs are found in the effective temperature range between 5 and 30 kK; almost all appear to have H-rich atmospheres. Fields are also found in a number white dwarfs in close and interacting binary systems of the

核心 发表于 2025-3-31 20:17:02

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愤怒历史 发表于 2025-3-31 23:45:36

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查看完整版本: Titlebook: Cosmical Magnetism; D. Lynden-Bell Book 1994 Springer Science+Business Media Dordrecht 1994 Scale.astronomy.magnetosphere.quasar.relativis