Interstellar Cosmic Ray Spectra from the Nonthermal Radio Background from 0.4 to 400 MHz

dc.contributor.authorGoldstein, Melvyn
dc.contributor.authorRamaty, R.
dc.contributor.authorFisk, L. A.
dc.date.accessioned2023-11-02T17:55:04Z
dc.date.available2023-11-02T17:55:04Z
dc.date.issued1970-05-25
dc.description.abstractWe deduce the interstellar electron spectrum from the nonthermal radio background. From 200 MeV to a few GeV the spectral index is 1.8 and there is evidence for residual solar modulation. Above a few GeV, the spectrum is steeper and the intensity is similar to that observed at earth. A consistent modulation for electrons and protons of the same rigidity can be obtained by using the complete diffusion-convection energy-loss theory of solar modulation.en
dc.description.sponsorshipResearch supported by NASA Grant No. NGL 21-002-033en
dc.description.urihttps://journals.aps.org/prl/abstract/10.1103/PhysRevLett.24.1193en
dc.format.extent4 pagesen
dc.genrejournal articlesen
dc.identifierdoi:10.13016/m2x9eg-gmkq
dc.identifier.citationGoldstein, M. L., R. Ramaty, and L. A. Fisk. “Interstellar Cosmic Ray Spectra from the Nonthermal Radio Background from 0.4 to 400 MHz.” Physical Review Letters 24, no. 21 (May 25, 1970): 1193–96. https://doi.org/10.1103/PhysRevLett.24.1193.en
dc.identifier.urihttps://doi.org/10.1103/PhysRevLett.24.1193
dc.identifier.urihttp://hdl.handle.net/11603/30491
dc.language.isoenen
dc.publisherAPSen
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
dc.rightsPublic Domain Mark 1.0*
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.en
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleInterstellar Cosmic Ray Spectra from the Nonthermal Radio Background from 0.4 to 400 MHzen
dc.typeTexten
dcterms.creatorhttps://orcid.org/0000-0002-5317-988Xen

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