Titlebook: Astrophysical and Laboratory Plasmas; A Festschrift for Pr A. J. Willis,T. W. Hartquist Book 1996 Springer Science+Business Media Dordrecht

EWE

ectropion

KEGEL

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Overview: 978-90-481-4729-8978-94-017-0803-6

行为

Foundation Actionscript 3.0 Animationof stellar transition regions show common behaviour as well as systematic trends. The basic methods used in making models of the transition region are set out. Observations relating to inhomogeneities in the solar transition region are summarized. The structure and energy balance of stellar transition regions and the trends emerging are discussed.

olfction

Inverse Kinematics: Dragging and Reachingf radiativelydriven stellar winds. The theory makes predictions which are shown to be in general accord with the data. We summarize recent results, primarily from the IUE satellite, which demonstrate the importance of time-dependent phenomena in hot-star outflows, and which, in particular, point to effects related to rotational modulation.

Favorable

Particle Attraction and Gravityof self-consistent hydrodynamic models for the production of the line-forming regions. We here review such modelling and stress the central role played by shock phenomena induced by winds and explosions on scales ranging from the circumstellar to the intergalactic.

Synovial-Fluid

https://doi.org/10.1007/978-94-017-0803-6Accretion; Chromosphere; Corona; Solar; Sun; astronomy; astrophysics

aneurysm

978-90-481-4729-8Springer Science+Business Media Dordrecht 1996