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Measurement of LET distribution and dose equivalent on board the space shuttle STS-65

Authors :
Jun Kikuchi
Shunji Nagaoka
Koichi Ogura
Takayoshi Hayashi
Ryuichi Takeuchi
Gautam D. Badhwar
Mitsuyasu Kato
Tadayoshi Doke
Nobuyuki Hasebe
Source :
Radiation Measurements. 26:935-945
Publication Year :
1996
Publisher :
Elsevier BV, 1996.

Abstract

Space radiation dosimetry measurements have been made on board the Space Shuttle STS-65 in the Second International Microgravity Laboratory (IML-2). In these measurements, three kinds of detectors were used; one is a newly developed active detector telescope called "Real-time Radiation Monitoring Device (RRMD)" utilizing silicon semi-conductor detectors and others are conventional detectors of thermoluminescence dosimeters (TLDs) and CR-39 plastic track detectors. Using the RRMD detector, the first attempt of real-time monitoring of space radiation has been achieved successfully for a continuous period of 251.3 h, giving the temporal variations of LET distribution, particle count rates, and rates of absorbed dose and dose equivalent. The RRMD results indicate that a clear enhancement of the number of trapped particles is seen at the South Atlantic Anomaly (SAA) without clear enhancement of dose equivalent, while some daily periodic enhancements of dose equivalent due to high LET particles are seen at the lower geomagnetic cutoff regions for galactic cosmic ray particles (GCRs). Therefore, the main contribution to dose equivalent is seen to be due to GCRs in this low altitude mission (300 km). Also, the dose equivalent rates obtained by TLDs and CR-39 ranged from 146.9 to 165.2 microSv/day and the average quality factors from 1.45 to 1.57 depending on the locations and directions of detectors inside the Space-lab at this highly protected orbit for space radiation with a small inclination (28.5 degrees) and a low altitude (300 km). The LET distributions obtained by two different detectors, RRMD and CR-39, are in good agreement in the region of 15-200 keV/mm and difference of these distributions in the regions of LET15 keV/mm and LET200 keV/mm can be explained by considering characteristics of CR-39 etched track formation especially for the low LET tracks.

Details

ISSN :
13504487
Volume :
26
Database :
OpenAIRE
Journal :
Radiation Measurements
Accession number :
edsair.doi.dedup.....7a14121a699589f6b288b9002d3fdbf9
Full Text :
https://doi.org/10.1016/s1350-4487(96)00095-9