Boundary conditions for the phenomena of solar bursts established from the statistical behavior of hard X-ray bands

Details Boundary conditions for the phenomena of solar bursts established from the statistical behavior of hard X-ray bands Boundary conditions for the phenomena of solar bursts established from the statistical behavior of hard X-ray bands

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ipespreptr....c&link_type=abstract

M.S. Thesis Instituto de Pesquisas Espaciais, Sao Jose dos Campos (Brazil).

Physics

Boundary Conditions, Parameter Identification, Solar Flares, Statistical Analysis, Boundary Value Problems, Microwaves, Poisson Density Functions, Radiation Sources, Stochastic Processes, X Rays

Scientific paper

The statistical studies of solar burst parameters at X-rays and microwaves, as well as an analysis of the limits caused by instrumental sensitivity and their effect on the form of the distributions and on the establishment of boundary conditions for solar flare phenomena are presented. The statistical behavior of events observed with high sensitivity at hard X-rays with the HXRBS experiment (SMM) was performed. Maxima were formed in the parameters distribution, which is related to intrinsic characteristics of the source-regions. This result seems to confirm early studies which indicated the influence of the sensitivity limits. Assuming the maxima of the distributions as real, it was possible to establish boundary conditions for the mechanisms of primary energy release. The principal condition establishes that solar bursts are interpreted as a superposition of primary explosions. The statistical analysis permitted the estimate of a value for the amount of energy in a primary explosion, making use of adjustments of Poisson functions.

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