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Evidence for confinement of low-energy cosmic rays ahead of interplanetary shock waves

โœ Scribed by R. A. R. Palmeira; F. R. Allum

Publisher
Springer
Year
1973
Tongue
English
Weight
619 KB
Volume
30
Category
Article
ISSN
0038-0938

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The discovery using ASCA that the featureless X-ray spectrum from the shell of SN 1006 is produced by shock-accelerated TeV electrons, and is thus an indicator of cosmic ray acceleration, has sparked a search for X-ray spectral evidence for cosmic ray acceleration in other remnants, as well as much