Radiation hazard from solar flares in terrestrial space. II - Method for determining the dose and the risk of exceeding the dose

Details Radiation hazard from solar flares in terrestrial space. II - Method for determining the dose and the risk of exceeding the dose Radiation hazard from solar flares in terrestrial space. II - Method for determining the dose and the risk of exceeding the dose

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979kosis..17..122p&link_type=abstract

Kosmicheskie Issledovaniia, vol. 17, Jan.-Feb. 1979, p. 122-126. In Russian.

Biology

Earth Environment, Flight Hazards, Radiation Dosage, Radiobiology, Solar Flares, Spacecraft Environments, Monte Carlo Method, Risk, Solar Protons, Statistical Analysis

Scientific paper

Kolomenskii et al. (1978) have derived a model describing the radiation environment produced by solar cosmic rays from an analysis of statistical data. In the present paper, this statistical model is used as a basis to develop a Monte Carlo technique for calculating the absorbed dose of cosmic-ray protons and evaluating the radiation hazard probability (risk) in orbital flights. Risk-versus-dose curves are obtained for several specific space missions.

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