Dynamic spectral characteristics of thermal models for solar hard X-ray bursts

Details Dynamic spectral characteristics of thermal models for solar hard X-ray bursts Dynamic spectral characteristics of thermal models for solar hard X-ray bursts

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...67..143b&link_type=abstract

Solar Physics, vol. 67, Aug. 1980, p. 143-162. Research supported by the Science Research Council of England;

Physics

31

Astronomical Models, Solar Magnetic Field, Solar X-Rays, Thermal Radiation, X Ray Spectra, Bremsstrahlung, Bursts, Dynamic Characteristics, Integral Equations, Life (Durability), Maxwell-Boltzmann Density Function, Solar Spectra

Scientific paper

It is proposed that the source for solar hard X-ray bursts may consist of a distribution of many small impulsively-heated kernels, each cooled by anomalous conduction, with lifetimes shorter than current burst data temporal resolution. The dynamic spectra of bursts are governed by the dynamic evolution of the kernel production process, such as magnetic-field dissipation in the tearing mode. An integral equation is formulated, the solution of which yields information on this kernel production process from dynamic burst spectra, for any kernel model.

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