@inproceedings{440f05ac325c4d2b9bc4ce3782059b88,
title = "Anomalous cosmic rays in the heliosheath: Simulation with a blunt termination shock",
abstract = "We present numerical simulations modeling acceleration of ACRs at a blunt termination shock with the spiral field lines intersecting the shock multiple times. The 2-D model includes parallel and perpendicular diffusion. Our results confirm the qualitative expectations: the nose segment of the blunt shock is inefficient to accelerate particles to ACR energies, which results in a continuing increase of the ACR flux and a gradual unfolding of the ACR spectrum behind the shock, as seen by Voyager-1. We also present a simple analytically tractable test-case to illustrate physical effects at a 2-D shock with a structure along the shock-front.",
keywords = "Energetic particles, Heliosheath, Termination shock",
author = "J. K{\'o}ta and Jokipii, \{J. R.\}",
year = "2008",
doi = "10.1063/1.2982477",
language = "English (US)",
isbn = "9780735405660",
series = "AIP Conference Proceedings",
pages = "397--403",
booktitle = "Particle Acceleration and Transport in the Heliosphere and Beyond - 7th Annual International Astrophysics Conference",
note = "7th Annual International Astrophysics Conference on Particle Acceleration and Transport in the Heliosphere and Beyond ; Conference date: 07-03-2008 Through 13-03-2008",
}