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- W2113751495 abstract "Kinetic streaming instabilities, such as the Weibel instability, occur in various HED plasma setups. Such instabilities generate strong (sub-equipartition) magnetic fields which reside at small, sub-Larmor scales. Efficient electron acceleration to relativistic energies is not uncommon in such environments. Spectra of radiation emitted by these relativistic electrons can deliver a wealth of information about the internal structure of such “Weibel turbulence”. The small-scale fields simultaneously drive the particle transport via pitch-angle diffusion. Both effects are related and can be used to diagnose the plasma state. We study such a relation between transport and radiation in subLarmor-scale turbulence via numerical simulations and analysis." @default.
- W2113751495 created "2016-06-24" @default.
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- W2113751495 date "2012-12-31" @default.
- W2113751495 modified "2023-09-24" @default.
- W2113751495 title "Transport properties and radiation production in plasmas with sub-LArmor-scale magnetic turbulence" @default.
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