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DOI http://dx.doi.org/10.1103/PhysRev.116.445
Title COSMIC-RAY NEUTRON ENERGY SPECTRUM
Creator/Author Hess, W.N. ; Patterson, H.W. ; Wallace, R. ; Chupp, E.L.
Publication Date1959 Oct 15
OSTI IdentifierOSTI ID: 4187052
Other Number(s)Journal ID: PHRVA; Other: 0031-899X
Resource TypeJournal Article
Resource RelationJournal Name: Physical Review (U.S.) Superseded in part by Phys. Rev. A, Phys. Rev. B: Solid State, Phys. Rev. C, and Phys. Rev. D; Journal Volume: Vol: 116; Other Information: Orig. Receipt Date: 31-DEC-60
Research OrgUniv. of California, Berkeley; Univ. of California, Livermore
SubjectPHYSICS; ATMOSPHERE; COSMIC RADIATION; COSMIC RAY STARS; DETECTION; DISTRIBUTION; EARTH; ENERGY; ENERGY RANGE; FISSION; GEOMAGNETIC COORDINATES; INSTRUMENTS; INTERACTIONS; LEVELS; MAGNETIC FIELDS; MEASURED VALUES; NEUTRONS; NUCLEONS; STANDARDS; THERMAL NEUTRONS
Description/AbstractThe cosmic-ray neutron energy spectrum in the equilibrium region of the atmosphere was measured with several different calibrated detectors from thermal energies to about 1 Bev at 44 deg north magnetic latitude and up to 40,000 feet. By combination of the data from these measurements with those from other experiments, a complete differential energy spectrum is obtained which shows the characteristic maximum near thermal energies and a roughly 1/E variation up to about 100 kev. The presence of a second maximum in the spectrum near 1 Mev is attributed to the evaporation neutrons from stars, and above this energy up to 800 Mev the spectrum falls off as E/sup -1.4/. (auth)
Country of PublicationCountry unknown/Code not available
LanguageEnglish
FormatMedium: X; Size: Pages: 445-57
System Entry Date2009 Dec 14

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