NASA NTRS · 19950053664
The termination shock: Physical processes
Abstract
A brief overview of the physics thought to determine the properties of the heliospheric termination shock is given and the central role of hot interstellar pick-up ions and cosmic rays is emphasized.
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Zank, G. P., Cairns, I. H., Webb, G. M.. 1995-01-01. The termination shock: Physical processes. https://ntrs.nasa.gov/citations/19950053664
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