A model of hot loops associated with solar flares. I - Gasdynamics in the loops

Details A model of hot loops associated with solar flares. I - Gasdynamics in the loops A model of hot loops associated with solar flares. I - Gasdynamics in the loops

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...68..351n&link_type=abstract

Solar Physics, vol. 68, Dec. 1980, p. 351-379.

Physics

108

Coronal Loops, Dynamic Models, Gas Dynamics, Solar Atmosphere, Solar Flares, X Ray Sources, Density Distribution, Mach Number, Pressure Distribution, Shock Waves, Temperature Dependence, Temperature Distribution, Velocity Distribution

Scientific paper

A dynamical model suggested for the formation of soft X-ray emitting hot loops in solar flares is tested by numerical simulations of a solar model atmosphere in a magnetic loop. The atmosphere changes its state and forms a hot loop when the flare energy is released in the form of liberated heat at the top or around the transition region. The thermal components of radiations emitted from flare regions are interpreted in a unified manner by using physical quantities computed as functions of time and position in the flare loop model.

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