Published 1985 | Version v1
Book

Shock drift acceleration

Description

This is a review of the fundamental physics of the interactions of charged particles treated individually while they interact with fast mode magnetohydrodynamic shocks. Numerical simulation and analytical theory are used to develop predictions of the expected characteristics of this process strong upstream anisotropies directed along the magnetic field and downstream anisotropies tending to be peaked more perpendicular to the field; relatively more of the enhancement of higher-energy particles occurring upstream; sensitive dependence on shock normal to magnetic field angle of the efficiency of energization. Observations which display all of the above characteristics are reviewed. Also discussed is the relationship of shock drift acceleration to the models for stochastic transport of charged particles in the vicinity of shocks. Extensions of this work in both the observational and theoretical approaches are discussed. 41 references

Additional details

Additional titles

Augmented title (English)
Of charged particles in interstellar space

Publishing Information

Publisher
American Geophysical Union.
Imprint Place
Washington, DC (USA)
Imprint Title
Collisionless shocks in the heliosphere: Reviews of current research
Journal Page Range
p. 271-285.