A two-component thermal model of X-ray burst sources

Details A two-component thermal model of X-ray burst sources A two-component thermal model of X-ray burst sources

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...39..175h&link_type=abstract

Solar Physics, vol. 39, Nov. 1974, p. 175-192.

Physics

2

Astronomical Models, Plasma Jets, Solar Flares, Solar X-Rays, Electron Flux Density, Flow Velocity, Mach Number, Oso-5, Plasma Temperature, Satellite Observation, Shock Fronts, Temperature Effects

Scientific paper

A semi-empirical model of the soft X-ray source associated with solar flares is presented, based on the results of the two temperature analysis of OSO-5 data obtained by Herring and Craig (1973). The model makes use of a jet of plasma rising from the solar surface as the basic origin of the soft X-ray emitting region, and gives rise to a cool region caused by randomisation of the jet, and a hot region caused by a shock front. Two different geometries are examined, and the model allows flow velocities and electron densities to be calculated.

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