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_US
dc.description.sponsorshipResearch supported by NASA Grant No. NGL 21-002-033en_US
dc.description.urihttps://journals.aps.org/prl/abstract/10.1103/PhysRevLett.24.1193en_US
dc.format.extent4 pagesen_US
dc.genrejournal articlesen_US
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_US
dc.identifier.urihttps://doi.org/10.1103/PhysRevLett.24.1193
dc.identifier.urihttp://hdl.handle.net/11603/30491
dc.language.isoen_USen_US
dc.publisherAPSen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
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_US
dc.rightsPublic Domain Mark 1.0*
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_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0002-5317-988Xen_US

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