Quasi-linear heating and acceleration in bi-Maxwellian plasmas

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F13%3A00423982" target="_blank" >RIV/67985815:_____/13:00423982 - isvavai.cz</a>
Alternative codes found
RIV/68378289:_____/13:00425931
Result on the web
<a href="http://dx.doi.org/10.1063/1.4846955" target="_blank" >http://dx.doi.org/10.1063/1.4846955</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1063/1.4846955" target="_blank" >10.1063/1.4846955</a>

Result language
angličtina
Original language name
Quasi-linear heating and acceleration in bi-Maxwellian plasmas
Original language description
Quasi-linear acceleration and heating rates are derived for drifting bi-Maxwellian distribution functions in a general nonrelativistic case for arbitrary wave vectors, propagation angles, and growth/damping rates. The heating rates in a proton-electron plasma due to ion-cyclotron/kinetic Alfvén and mirror waves for a wide range of wavelengths, directions of propagation, and growth or damping rates are explicitly computed.
Czech name
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Czech description
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Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2013
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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