Summary and conclusions
It has been pointed out that cosmic γ-rays have something to say about the origin of cosmic-ray particles. Although the statistical precision of the data and the directional accuracy of the satellite-borne detectors operated so far have been poor, useful results have been achieved already.
It is the reviewers' view that the situation at present concerning cosmic-ray origin is as follows:
-
(i)
Cosmic-ray protons below 10 GeV or so, which produce the majority of γ-rays in the region 300–5000 MeV, are produced mainly in our Galaxy. The evidence against an extragalactic origin seems strong; there would then be consistency with the conclusions that the particles above 3x1011 eV (up to 1019 eV) are also mainly Galactic, an observation that comes from anisotropy measurements.
-
(ii)
The recent observations of changes of spectral shape of the γ-ray spectrum with changes of longitude and latitude add weight to the idea of Galactic origin. The details are not clear but a composite model involving supernova remnant acceleration preferentially in Galactic spiral arms and spectral modification by Galactic winds looks promising. The changes appear to relate to both electrons and protons.
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(iii)
There is still evidence for an excess cosmic-ray intensity in the nearby Loop I SNR and the magnitude of the excess is of the order of that expected in terms of contemporary shock acceleration theory, again both electrons and protons are involved.
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(iv)
There is weak but finite evidence for an excess cosmic-ray intensity in some local giant molecular clouds, the increase in intensity being greatest for those particles producing γ-rays of energy below about 150 MeV, presumably electrons.
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Van Der Walt, D.J., Wolfendale, A.W. Gamma rays and the origin of cosmic rays. Space Sci Rev 47, 1–45 (1988). https://doi.org/10.1007/BF00223236
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DOI: https://doi.org/10.1007/BF00223236