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 (2)
Right arrowRequest Permissions
Google Scholar
Right arrow Articles by Domingo, C.
Right arrow Articles by Vidal-Quadras, A.
Right arrow Search for Related Content
PubMed
Right arrow Articles by Domingo, C.
Right arrow Articles by Vidal-Quadras, A.
Social Bookmarking
 Add to CiteULike   Add to Connotea   Add to Del.icio.us  
What's this?

Radiation Protection Dosimetry 34:13-16 (1990)
© 1990 Oxford University Press

Ultra Heavy Ion LET Determination with Solid State Nuclear Track Detectors

C. Domingo, C. Baixeras, F. Fernández and A. Vidal-Quadras

The Ultra Heavy Cosmic Ray Experiment, on board the LDEF spacecraft, will provide the first statistically significant sample of relativistic Z ( 65 cosmic ray ions. This information is essential in order to determine the cosmic ray flux of such particles. If we know the linear energy transfer (LET) of these particles, it is possible to calculate their contribution to the total dose to which an in-orbit experiment or a manned space mission will be exposed. Solid state nuclear track detector stacks can give us information about the LET of ultra heavy ions in a particular environment. Several polycarbonate and polyethylene teraphtalate (PET) stacks have been exposed in an accelerator to different ultra heavy beams for calibration. A study of LET has been carried out and it has been found that some corrections to the classical expression should be introduced in order to reproduce the experimental data.


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




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.