Numerical solution of the inverse problem of determining the spectrum of solar cosmic rays in the source

Details Numerical solution of the inverse problem of determining the spectrum of solar cosmic rays in the source Numerical solution of the inverse problem of determining the spectrum of solar cosmic rays in the source

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25..534m&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, July-Aug. 1985, p. 534-540. In Russian.

Mathematics

Logic

3

Astronomical Spectroscopy, Solar Cosmic Rays, Spectrum Analysis, Error Analysis, Green'S Functions, Integral Equations, Radiation Sources, Solar Flares, Solar Protons

Scientific paper

A method for determining the spectrum of solar cosmic rays (SCR) in the source is proposed which is based on the numerical solution of the appropriate integral equation using data on the SCR time profile near earth orbit. Methodological questions are examined, and the applicability of the method is illustrated by results for the solar proton events of May 28, 1972, August 7, 1972, and September 7, 1973.

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