Physics
Scientific paper
Sep 1961
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1961natur.191.1381s&link_type=abstract
Nature, Volume 191, Issue 4796, pp. 1381 (1961).
Physics
4
Scientific paper
THE general radio emission, from the Galaxy has now been accounted for as the synchrotron radiation of high-energy electrons in a magnetic field. An unsatisfactory aspect of this explanation is the relation between the observed radio spectral index α, where radio flux is proportional to (wave-length)α, and the expected energy spectrum of the cosmic-ray electrons, the number density of which should also vary exponentially according to (energy)-(1+S). In these circumstances the indices are related by α = S/2.
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