Cosmic-ray diffusion in a sectored magnetic field in the distant heliosheath

Very high intensities of galactic cosmic rays measured by Voyager 1 in the heliosheath appear to be incompatible with the presence of a modulation "wall" near the heliopause produced by a pile up of the heliospheric magnetic field. We propose that the modulation wall is a structure permeab...

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Bibliographic Details
Published in:arXiv.org 2013-02
Main Authors: Florinski, V, Alouani-Bibi, F, Kota, J, Guo, X
Format: Article
Language:English
Subjects:
Cosmic rays
Dependence
Galactic cosmic rays
Heliopause
Heliosphere
Magnetic fields
Magnetic permeability
Magnetic sectors
Model testing
Modulation
Particle energy
Topology
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Summary:Very high intensities of galactic cosmic rays measured by Voyager 1 in the heliosheath appear to be incompatible with the presence of a modulation "wall" near the heliopause produced by a pile up of the heliospheric magnetic field. We propose that the modulation wall is a structure permeable to cosmic rays as a result of a sectored magnetic field topology compressed by plasma slowdown on approach to the heliopause and stretched to high latitudes by latitudinal flows in the heliosheath. The tightly folded warped current sheet permits efficient cosmic-ray transport in the radial direction via a drift-like mechanism. We show that when stochastic variations in the sector widths are taken into account, particle transport becomes predominantly diffusive both along and across the magnetic sectors. Using a test-particle model for cosmic rays in the heliosheath we investigate the dependence of the diffusion coefficients on the properties of the sector structure and on particle energy.
ISSN:2331-8422
DOI:10.48550/arxiv.1302.2927