1. An excess of cosmic ray electrons at energies of 300-800 GeV
- Author
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Chang, J., Adams, Jr., J.H., Ahn, H.S., Bashindzhagyan, G.L., Christl, M., Ganel, O., Guzik, T.G., Isbert, J., Kim, K.C., Kuznetsov, E.N., Panasyuk, M.I., Panov, A.D., Schmidt, W.K.H., Seo, E.S., Sokolskaya, N.V., Watts, J.W., Wefel, J.P., Wu, J., and Zatsepin, V.I.
- Subjects
Cosmic background radiation -- Evaluation -- Discovery and exploration ,Radio sources (Astronomy) -- Discovery and exploration -- Properties ,Electrons -- Properties -- Discovery and exploration ,Cosmic rays -- Atomic properties -- Discovery and exploration ,Environmental issues ,Science and technology ,Zoology and wildlife conservation ,Discovery and exploration ,Atomic properties ,Evaluation ,Properties - Abstract
Galactic cosmic rays consist of protons, electrons and ions, most of which are believed to be accelerated to relativistic speeds in supernova remnants (1-3). All components of the cosmic rays [...]
- Published
- 2008