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Titlebook: Unstable Current Systems and Plasma Instabilities in Astrophysics; Proceedings of the 1 Mukul R. Kundu,Gordon D. Holman Conference proceedi

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發(fā)表于 2025-3-23 13:04:03 | 只看該作者
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發(fā)表于 2025-3-23 16:37:39 | 只看該作者
On the Role of Double Layers in Astrophysical Plasmasodels. Some problems of this sort are described, and some central issues in structure and dynamics of double layers are identified, which must be addressed in astrophysical contexts. These include the determination of kinetic boundary conditions, and the relations of time and length scales of local
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發(fā)表于 2025-3-23 18:47:54 | 只看該作者
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發(fā)表于 2025-3-23 22:50:33 | 只看該作者
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發(fā)表于 2025-3-24 02:22:33 | 只看該作者
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發(fā)表于 2025-3-24 08:14:28 | 只看該作者
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發(fā)表于 2025-3-24 12:17:09 | 只看該作者
Computer Simulation of Reconnection in Planetary Magnetospheres models to make a comparison of the computer models with analytic theory meaningful. In addition more detailed, even three-dimensional, models can be used for a comparison with extended data from in situ observations. The computer studies have basically confirmed the reconnection picture that was ba
18#
發(fā)表于 2025-3-24 16:13:10 | 只看該作者
Observational Evidence for Magnetic Reconnection in Microwave Solar Bursts in the coronal magentic field configurations that took place before the onset of an impulsive burst observed on 14 May 1980. We also discuss a second set of 6 cm VLA observations (spatial resolution 18″; arc) where several interacting loops were involved in triggering the onset of an impulsive burs
19#
發(fā)表于 2025-3-24 21:50:59 | 只看該作者
Acceleration of Runaway Electrons and Joule Heating in Solar Flarese production of D.C. electric fields. On the other hand, microwave and hard X-ray observations of flares provide specific requirements for the number and energy of energetic electrons produced during a flare, and the timescales involved in accelerating them. The microwave emission from flares is und
20#
發(fā)表于 2025-3-25 02:04:39 | 只看該作者
Links between Jet Instabilities, Radiation and Propagation in Astrophysics a cloud can lead to tunneling through large clouds, or propelling of smaller clouds out of the jet path. In this fashion jets may clear their way through an inhomogeneous medium, avoiding lateral disturbances and preheating their path.
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