Welcome to the new version of CaltechAUTHORS. Login is currently restricted to library staff. If you notice any issues, please email coda@library.caltech.edu
Published September 26, 2006 | Published
Book Section - Chapter Open

Cosmic ray energy changes at the termination shock and in the heliosheath

Abstract

Voyager 1 crossed the termination shock of the solar wind in December 2004 at 94 AU and currently measures the cosmic ray intensity in the heliosheath. To better understand this modulation region beyond the shock, where adiabatic energy changes should be small, we review the net effect of energy changes during the modulation process, including adiabatic deceleration in the solar wind, acceleration at the termination shock, and the possibility that stochastic acceleration in the heliosheath may also make a contribution.

Additional Information

© 2006 American Institute of Physics. This work was supported by UNAM-DGAPA grant IN106105 in Mexico, NSF grant ATM 0107181 in Maryland, NASA grant NAG5-12929 at Caltech and JPL, and the South African National Research Foundation.

Attached Files

Published - MORaipcp06.pdf

Files

MORaipcp06.pdf
Files (2.1 MB)
Name Size Download all
md5:aa1fb3a82c1f4d9076e1e4c1f37112bd
2.1 MB Preview Download

Additional details

Created:
August 22, 2023
Modified:
January 12, 2024