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Low energy cosmic ray studies from a lunar baseStudies of cosmic ray nuclei with energies less than about 7 GeV/nucleon in low earth orbit are hampered by the geomagnetic field. Even in high inclination orbits these effects can be significant. The lunar surface (or lunar orbit) provides an attractive site for carrying out low energy cosmic ray studies which require large detectors. The rationale and requirements for this type of experiment are described.
Document ID
19910071932
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Wiedenbeck, Mark E.
(Chicago, University IL, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1990
Subject Category
Space Radiation
Meeting Information
Meeting: NASA Workshop
Location: Stanford, CA
Country: United States
Start Date: May 19, 1989
End Date: May 20, 1989
Sponsors: Stanford University, NASA, Lunar Planetary Institute
Accession Number
91A56555
Funding Number(s)
CONTRACT_GRANT: NGL-14-001-005
Distribution Limits
Public
Copyright
Other

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