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

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51#
發(fā)表于 2025-3-30 08:46:33 | 只看該作者
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.
52#
發(fā)表于 2025-3-30 14:28:45 | 只看該作者
53#
發(fā)表于 2025-3-30 19:48:57 | 只看該作者
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.
54#
發(fā)表于 2025-3-30 22:38:43 | 只看該作者
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
55#
發(fā)表于 2025-3-31 01:05:23 | 只看該作者
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
56#
發(fā)表于 2025-3-31 08:35:20 | 只看該作者
57#
發(fā)表于 2025-3-31 09:49:38 | 只看該作者
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
58#
發(fā)表于 2025-3-31 14:41:27 | 只看該作者
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
59#
發(fā)表于 2025-3-31 20:17:02 | 只看該作者
60#
發(fā)表于 2025-3-31 23:45:36 | 只看該作者
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