The Heliospheric Termination Shock
Abstract
The heliospheric Termination Shock is the largest (by dimension) shock in the heliosphere. It is believed that it is also the strongest shock and is responsible for the generation of the Anomalous Cosmic Ray component in the heliosphere. This chapter review the gross properties and observations of the Termination Shock. It is structured as follows: 1. The heliosphere, providing the heliospheric stage for Termination Shock formation, 2. The argument for a heliospheric Termination Shock, 3. The global heliospheric system, 4. Termination Shock properties, 5. Observations: the Voyager passages, radio observations, plasma waves and electron beams, traces of plasma and magnetic field, energetic particles, galactic cosmic rays, Termination Shock particles, the anomalous cosmic ray component, 6. Conclusions.
Cite
@article{arxiv.0807.4170,
title = {The Heliospheric Termination Shock},
author = {R. A. Treumann and C. H. Jaroschek},
journal= {arXiv preprint arXiv:0807.4170},
year = {2008}
}
Comments
20 pages, 8 figures, review paper