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Measurement of LET distribution and dose equivalent on board the space shuttle STS-65.
Hayashi, T; Doke, T; Kikuchi, J; Takeuchi, R; Hasebe, N; Ogura, K; Nagaoka, S; Kato, M; Badhwar, G D.
Afiliação
  • Hayashi T; Advanced Research Center for Science and Engineering, Waseda University, Tokyo, Japan.
Radiat Meas ; 26(6): 935-45, 1996 Nov.
Article em En | MEDLINE | ID: mdl-11540526
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 LET < 15 keV/mm and LET > 200 keV/mm can be explained by considering characteristics of CR-39 etched track formation especially for the low LET tracks.
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Coleções: 01-internacional Base de dados: MEDLINE Assunto principal: Prótons / Voo Espacial / Monitoramento de Radiação / Transferência Linear de Energia / Atividade Solar / Radiação Cósmica País/Região como assunto: America do sul Idioma: En Revista: Radiat Meas Assunto da revista: RADIOLOGIA Ano de publicação: 1996 Tipo de documento: Article País de afiliação: Japão País de publicação: Reino Unido
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Coleções: 01-internacional Base de dados: MEDLINE Assunto principal: Prótons / Voo Espacial / Monitoramento de Radiação / Transferência Linear de Energia / Atividade Solar / Radiação Cósmica País/Região como assunto: America do sul Idioma: En Revista: Radiat Meas Assunto da revista: RADIOLOGIA Ano de publicação: 1996 Tipo de documento: Article País de afiliação: Japão País de publicação: Reino Unido