Skip Navigation

This Article
Right arrow Full Text (PDF)
Right arrow Alert me when this article is cited
Right arrow Alert me if a correction is posted
Services
Right arrow Email this article to a friend
Right arrow Similar articles in this journal
Right arrow Alert me to new issues of the journal
Right arrow Add to My Personal Archive
Right arrow Download to citation manager
Right arrow Search for citing articles in:
ISI Web of Science (16)
Right arrowRequest Permissions
Google Scholar
Right arrow Articles by O'Brien, K.
Right arrow Articles by Sauer, H.H.
Right arrow Search for Related Content
PubMed
Right arrow Articles by O'Brien, K.
Right arrow Articles by Sauer, H.H.
Social Bookmarking
 Add to CiteULike   Add to Connotea   Add to Del.icio.us  
What's this?

Radiation Protection Dosimetry 45:145-162 (1992)
© 1992 Oxford University Press

The Exposure of Aircraft Crews to Radiations of Extraterrestrial Origin

K. O'Brien, W. Friedberg, F.E. Duke, L. Snyder, E.B. Darden Jr. and H.H. Sauer

Galactic cosmic rays and energetic particles from solar particle events produce radiation levels at aircraft altitudes that have recently become a matter of concern to relevant government organisations, aircraft crews and airline management. The radiation levels have been calculated throughout the atmosphere using the code LUIN and the results incorporated in the code CARRIER which will integrate the dose equivalent rates to which a flight has been exposed from takeoff to landing, yielding the total dose equivalent to the crew and passengers. Radiation dose equivalents for a number of air carrier routes have been determined from this source and corresponding health risks have been calculated using standard risk coefficients. Radiation dose equivalents have been calculated for a number of solar particle events, and in detail for the 29 September 1989 event, all at high latitudes, for a range of aircraft altitudes. Owing to their unpredictability and variability, solar particle events have not been incorporated into CARRIER. However, once an event has occurred and its spectrum has been determined, the worldwide time-dependent distribution of the resulting dose equivalents can be calculated.


Add to CiteULike CiteULike   Add to Connotea Connotea   Add to Del.icio.us Del.icio.us    What's this?


This article has been cited by other articles:


Home page
Radiat Prot DosimetryHome page
M. Takada, B. J. Lewis, M. Boudreau, H. Al Anid, and L. G. I. Bennett
MODELLING OF AIRCREW RADIATION EXPOSURE FROM GALACTIC COSMIC RAYS AND SOLAR PARTICLE EVENTS
Radiat Prot Dosimetry, June 19, 2007; (2007) ncm214v1.
[Abstract] [Full Text] [PDF]


Home page
Radiat Prot DosimetryHome page
P. Goldhagen, J. M. Clem, and J. W. Wilson
The energy spectrum of cosmic-ray induced neutrons measured on an airplane over a wide range of altitude and latitude
Radiat Prot Dosimetry, August 1, 2004; 110(1-4): 387 - 392.
[Abstract] [Full Text] [PDF]



Disclaimer: Please note that abstracts for content published before 1996 were created through digital scanning and may therefore not exactly replicate the text of the original print issues. All efforts have been made to ensure accuracy, but the Publisher will not be held responsible for any remaining inaccuracies. If you require any further clarification, please contact our Customer Services Department.