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Electron-Ion Temperature Equilibration in Collisionless Shocks: The Supernova Remnant-Solar Wind Con...

Electron-Ion Temperature Equilibration in Collisionless Shocks: The Supernova Remnant-Solar Wind Con...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1458526291

Electron-Ion Temperature Equilibration in Collisionless Shocks: The Supernova Remnant-Solar Wind Connection

About this item

Full title

Electron-Ion Temperature Equilibration in Collisionless Shocks: The Supernova Remnant-Solar Wind Connection

Publisher

Dordrecht: Springer Netherlands

Journal title

Space science reviews, 2013-10, Vol.178 (2-4), p.633-663

Language

English

Formats

Publication information

Publisher

Dordrecht: Springer Netherlands

More information

Scope and Contents

Contents

Collisionless shocks are loosely defined as shocks where the transition between pre-and post-shock states happens on a length scale much shorter than the collisional mean free path. In the absence of collision to enforce thermal equilibrium post-shock, electrons and ions need not have the same temperatures. While the acceleration of electrons for i...

Alternative Titles

Full title

Electron-Ion Temperature Equilibration in Collisionless Shocks: The Supernova Remnant-Solar Wind Connection

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_1458526291

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1458526291

Other Identifiers

ISSN

0038-6308

E-ISSN

1572-9672

DOI

10.1007/s11214-013-9999-0

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