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Magnetic Fields in Young SNRs
Published online by Cambridge University Press: 19 July 2016
Extract
There are two very important properties of the magnetic fields in supernova remnants which we wish to emphasize: 1) The net radial orientation of the magnetic vectors throughout the shell and 2) an apparent gradual increase in the fractional polarization with evolutionary age.
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- 3. Magnetic Fields in and around Supernova Remnants
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- Copyright © Kluwer 1990