Spectral index of high-energy cosmic rays by the Compton-Getting effect at solar time frame with the Tibet air shower array

Details Spectral index of high-energy cosmic rays by the Compton-Getting effect at solar time frame with the Tibet air shower array Spectral index of high-energy cosmic rays by the Compton-Getting effect at solar time frame with the Tibet air shower array

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008nuphs.175..427t&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 175, p. 427-430.

Physics

Nuclear Physics

Scientific paper

We report on the spectral index of cosmic rays around 10 TeV energy region obtained by observation of the Compton-Getting anisotropy due to the terrestrial orbital motion around the Sun with the Tibet III air shower array during the period from 1999 to 2005. The spectral index has turned out to be 2.99±0.54, which is consistent with 2.74 by the direct energy spectrum measurement. This method is a new approach to measure the spectral index and is complementary to the conventional energy spectrum measurement.

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