Spatio-temporal evolution of the nonresonant instability in shock precursors of young supernova remn...
Spatio-temporal evolution of the nonresonant instability in shock precursors of young supernova remnants
About this item
Full title
Author / Creator
Publisher
Ithaca: Cornell University Library, arXiv.org
Journal title
Language
English
Formats
Publication information
Publisher
Ithaca: Cornell University Library, arXiv.org
Subjects
More information
Scope and Contents
Contents
A nonresonant cosmic-ray-current-driven instability may operate in the shock precursors of young supernova remnants and be responsible for magnetic-field amplification, plasma heating and turbulence. Earlier simulations demonstrated magnetic-field amplification, and in kinetic studies a reduction of the relative drift between cosmic rays and therma...
Alternative Titles
Full title
Spatio-temporal evolution of the nonresonant instability in shock precursors of young supernova remnants
Authors, Artists and Contributors
Author / Creator
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_journals_2071194931
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2071194931
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1705.04261
