NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Research on CR-39 plastic detectors for cosmic ray astrophysicsThe sensitivity of CR-39 is a strong function of catalyst concentration during its polymerization. Normal CR-39 will detect vertically incident particles with Z/beta as low as 10. An extrapolation suggests that CR-39 with a high catalyst concentration and sensitivity to within approximate 5% can be made by a suitable choice of cure cycle and mold material. CR-39 is less sensitive than Lexan to thermal annealing of tracks but cannot tolerate background radiation levels greater than a few Mrad.
Document ID
19810028129
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Price, P. B.
(California Univ. Berkeley, CA, United States)
Shirk, E. K.
(California Univ. Berkeley, CA, United States)
Kinoshita, K.
(California Univ. Berkeley, CA, United States)
Tarle, G.
(California, University Berkeley, Calif., United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1980
Subject Category
Instrumentation And Photography
Meeting Information
Meeting: International Cosmic Ray Conference
Location: Kyoto
Country: Japan
Start Date: August 6, 1979
End Date: August 18, 1979
Accession Number
81A12533
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available