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pro vyhledávání: '"Marret, Alexis"'
The non-thermal particles escaping from collisionless shocks into the surrounding medium can trigger a non-resonant streaming instability that converts parts of their drift kinetic energy into large amplitude magnetic field perturbations, and promote
Externí odkaz:
http://arxiv.org/abs/2407.18978
Streaming cosmic rays can power the exponential growth of a seed magnetic field by exciting a non-resonant instability that feeds on their bulk kinetic energy. By generating the necessary turbulent magnetic field, it is thought to play a key role in
Externí odkaz:
http://arxiv.org/abs/2111.15272
The cosmic rays non-resonant streaming instability is believed to be the source of substantial magnetic field amplification. In this work we investigate the effects of the ambient plasma temperature on the instability and derive analytical expression
Externí odkaz:
http://arxiv.org/abs/2010.10237
Autor:
Marret, Alexis
Cosmic rays can power the exponential growth of a seed magnetic field by exciting instabilities that feed on the kinetic energy of the particles collective streaming motion. Of the different streaming instabilities, the non-resonant mode, also called
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_____10369::d116d05c08774c22b4bb4545d12a6540
https://theses.hal.science/tel-03850803
https://theses.hal.science/tel-03850803