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Inferred Cosmic-Ray Spectrum from Fermi Large Area Telescope gamma-Ray Observations of Earth's Limb
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2014 (English)In: Physical Review Letters, ISSN 0031-9007, E-ISSN 1079-7114, Vol. 112, no 15, 151103- p.Article in journal (Refereed) Published
Abstract [en]

Recent accurate measurements of cosmic-ray (CR) species by ATIC-2, CREAM, and PAMELA reveal an unexpected hardening in the proton and He spectra above a few hundred GeV, a gradual softening of the spectra just below a few hundred GeV, and a harder spectrum of He compared to that of protons. These newly discovered features may offer a clue to the origin of high-energy CRs. We use the Fermi Large Area Telescope observations of the gamma-ray emission from Earth's limb for an indirect measurement of the local spectrum of CR protons in the energy range similar to 90 GeV-6 TeV (derived from a photon energy range 15 GeV-1 TeV). Our analysis shows that single power law and broken power law spectra fit the data equally well and yield a proton spectrum with index 2.68 +/- 0.04 and 2.61 +/- 0.08 above similar to 200 GeV, respectively.

Place, publisher, year, edition, pages
2014. Vol. 112, no 15, 151103- p.
Keyword [en]
Energy-Spectrum, Helium Spectra, Emission, Galaxy, Atmosphere, Proton, Albedo, Model, Egret
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:kth:diva-145581DOI: 10.1103/PhysRevLett.112.151103ISI: 000334597300003Scopus ID: 2-s2.0-84898959342OAI: oai:DiVA.org:kth-145581DiVA: diva2:723729
Funder
Knut and Alice Wallenberg Foundation
Note

QC 20140611

Available from: 2014-06-11 Created: 2014-05-23 Last updated: 2017-12-05Bibliographically approved

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