The piston model for coronal transient with forerunner

Details The piston model for coronal transient with forerunner The piston model for coronal transient with forerunner

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986sssmp..29..755t&link_type=abstract

Scientia Sinica, Series A - Mathematical, Physical, Astronomical and Technical Sciences (ISSN 0253-5831), vol. 29, July 1986, p.

Physics

Astronomical Models, Solar Corona, Solar Flares, Pistons, Shock Fronts, Solar Physics, Transient Response, Velocity Distribution

Scientific paper

A piston model of coronal transients with forerunners is developed and evaluated. In this model, a forerunner is formed as a spherical piston (consisting of a small amount of plasma ejected from the solar surface into a closed magnetic region) moves slowly outward prior to the main ejection. The model is described mathematically; numerical simulations are performed; and the model is shown to predict the observed configuration, kinetics, and dynamics of these large-scale transients with reasonable accuracy.

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