Radiation measurements on the Mir Orbital Station

Radiation measurements made onboard the MIR Orbital Station have spanned nearly a decade and covered two solar cycles, including one of the largest solar particle events, one of the largest magnetic storms, and a mean solar radio flux level reaching 250×10 4 Jansky that has been observed in the last...

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Veröffentlicht in:Radiation measurements 2002-10, Vol.35 (5), p.393-422
Hauptverfasser: Badhwar, G.D, Atwell, W, Reitz, G, Beaujean, R, Heinrich, W
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Sprache:eng
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Zusammenfassung:Radiation measurements made onboard the MIR Orbital Station have spanned nearly a decade and covered two solar cycles, including one of the largest solar particle events, one of the largest magnetic storms, and a mean solar radio flux level reaching 250×10 4 Jansky that has been observed in the last 40 years. The cosmonaut absorbed dose rates varied from about 450 μGy day −1 during solar minimum to approximately half this value during the last solar maximum. There is a factor of about two in dose rate within a given module, and a similar variation from module to module. The average radiation quality factor during solar minimum, using the ICRP-26 definition, was about 2.4. The drift of the South Atlantic Anomaly was measured to be 6.0±0.5°W, and 1.6±0.5°N. These measurements are of direct applicability to the International Space Station. This paper represents a comprehensive review of Mir Space Station radiation data available from a variety of sources.
ISSN:1350-4487
1879-0925
DOI:10.1016/S1350-4487(02)00072-0