The piston model of coronal transients

Details The piston model of coronal transients The piston model of coronal transients

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.100..391h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 100, no. 1-2, March 1984, p. 391-406.

Astronomy and Astrophysics

Astrophysics

1

Dense Plasmas, Gas Dynamics, Plasma Dynamics, Solar Corona, Transient Response, Compressible Flow, Flow Distribution, Mass Transfer, Piston Theory, Solar Activity, Stellar Models

Scientific paper

Coronal transients represent a display of solar activities involving a large amount of energy. The present investigation is concerned with a piston model of the coronal transients. The characteristics of this model are discussed in detail, and the quantitative results of unsteady gasdynamics are applied to the coronal transient processes. The piston model provides explanations regarding the major features of the transient observations, taking into account the density profile, the geometric configuration, the kinetic process, and the classifications of the coronal transient. The ejection of dense plasma produced by the solar activities may be the source or the triggering factor of the coronal transient. The typical flow regions include the compression flow region, and the rarefaction flow region.

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