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Correlation of Individual Cosmic Ray Nuclei With the Observation of Light Flashes By Apollo AstronautsA nuclear emulsion detector known as the Apollo Light Flash Moving Emulsion Detector (ALFMED) was designed: 1) to record tracks of primary cosmic rays; 2) to provide time-of-passage information via a relative plate translation technique; 3) to provide particle trajectory information; and, 4) to fit into a masklike device that could be located about the head and eyes of an astronaut. An ALFMED device was worn by an astronaut observing light flashes for 60 minutes on each of the last two Apollo missions. During the Apollo 17 experiment seventeen separate flashes were reported by the observer. With one-third of the total plate area completely analyzed, two definite correlations have been found between Z > 8 cosmic ray nuclei traversing an eye and the reports of visual sensations.
Document ID
19760044009
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
L S Pinsky
(University of Houston Houston, United States)
W Z Osborne
(University of Houston Houston, United States)
J V Bailey
(Johnson Space Center Houston, United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1975
Publication Information
Publication: 14th International Cosmic Ray Conference: Conference Papers, München, Germany, August 15-29, 1975
Publisher: Max Planck Institute for Extraterrestrial Physics
Volume: 9
Subject Category
Instrumentation and Photography
Report/Patent Number
CONF-750805
Meeting Information
Meeting: 14th International Cosmic Ray Conference
Location: München
Country: DE
Start Date: August 15, 1975
End Date: August 29, 1975
Sponsors: Max Planck Institute for Extraterrestrial Physics, International Union of Pure and Applied Physics
Accession Number
76A26975
Funding Number(s)
CONTRACT_GRANT: NGR-44-005-041
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Technical Review
NASA Technical Management
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