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Measurement of cosmic ray positron and negatron spectra between 50 and 800 MeVA balloon-borne magnetic spectrometer was used to measure the spectra of cosmic ray positrons and negatrons at energies between 50 and 800 MeV. Comparisons of the separate positron and negatron spectra observed near the earth with their expected intensities in interstellar space can be used to investigate the complex (and variable) interaction of galactic cosmic rays with the expanding solar wind. The present measurements, which have established finite values or upper limits for the positron and negatron spectral between 50 and 800 MeV, have confirmed earlier evidence for the existence of a dominant component of negatrons from primary sources in the galaxy. The present results are shown to be consistent with the hypothesis that the positron component is in fact mainly attributable to collisions between cosmic ray nuclei and the interstellar gas. The estimate of the absolute intensities confirm the indications from neutron monitors that in 1972 the interplanetary cosmic ray intensities were already recovering toward their high levels observed in 1965.
Document ID
19740008402
Document Type
Thesis/Dissertation
Authors
Daugherty, J. K.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 3, 2013
Publication Date
January 1, 1974
Subject Category
Space Radiation
Report/Patent Number
X-660-74-16
NASA-TM-X-70580
Funding Number(s)
CONTRACT_GRANT: NGL-21-002-033
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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