Shock drift acceleration
Creators
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.
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 18071285
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ACCELERATION; ALPHA PARTICLES; ANISOTROPY; INTERPLANETARY SPACE; KINETIC ENERGY; SHOCK WAVES; SOLAR ELECTRONS; SOLAR PROTONS; WAVE PROPAGATION
- Descriptors DEC
- BARYONS; CATIONS; CHARGED PARTICLES; ELECTRONS; ELEMENTARY PARTICLES; ENERGY; FERMIONS; HADRONS; HELIUM IONS; HYDROGEN IONS; HYDROGEN IONS 1 PLUS; IONIZING RADIATIONS; IONS; LEPTONS; NUCLEONS; PROTONS; RADIATIONS; SOLAR PARTICLES; SOLAR RADIATION; SPACE; STELLAR RADIATION