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Evaluation of cosmic radiation exposures of flight crew for epidemiologic studies.

Authors
Waters-M; Bloom-T; Grajewski-B
Source
Arbete och Halsa 2001 Jun; 2001(10):155-157
NIOSHTIC No.
20041289
Abstract
Introduction: Flight crew are exposed to elevated levels of cosmic ionizing radiation of galactic and solar origin and are among the more highly exposed occupational groups to ionizing radiation in the U.S., with annual doses ranging from approximately 0.2-5 mSv. Cosmic radiation dose depends primarily on altitude and geomagnetic latitude and to a lesser degree on solar activity and phase of the solar cycle. NIOSH is conducting several epidemiologic studies examining the relationship between cosmic radiation exposure, among other factors, and reproductive health of female flight attendants. Estimation of historical cosmic radiation dose is an essential component of these studies. One aim of this study was to measure cosmic radiation doses on a series of flights as a function of altitude, distance flown, latitude and longitude, and to compare dose-equivalent data collected on specific flights with doses estimated using the CARI computer program developed by the Federal Aviation Administration. CARI estimates will be used for dose reconstruction for the epidemiologic studies.
Keywords
Radiation; Aircrews; Flight-personnel; Employee-exposure; Ionizing-radiation; Altitude; Magnetic-fields; Epidemiology; Exposure-assessment; Reproductive-effects; Reproductive-hazards; Reproductive-system; Women; Dose-response; Computer-models
Contact
M. Waters, National Institute for Occupational Safety and Health (NIOSH), Cincinnati, Ohio, USA
Publication Date
20010601
Document Type
Abstract
Email Address
mwaters@cdc.gov
Editors
Hagsberg-M; Knave-B; Lillienberg-L; Westberg-H
Fiscal Year
2001
NTIS Accession No.
NTIS Price
ISBN No.
9789170456077
Issue of Publication
10
ISSN
0346-7821
NIOSH Division
DSHEFS
Source Name
Arbete och Halsa (X2001 - exposure assessment in epidemiology and practice, June 10-13, 2001, Göteborg, Sweden)
State
OH
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