EMIC wave interaction with relativistic electrons and heavy ions in inner magnetosphere
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F12%3A00426538" target="_blank" >RIV/68378289:_____/12:00426538 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
EMIC wave interaction with relativistic electrons and heavy ions in inner magnetosphere
Original language description
We analyze the full kinetic linear dispersion relations of electromagnetic ion-cyclotron (EMIC) waves in thermal plasmas with multiple ion components and temperature anisotropies, characteristic for the equatorial inner magnetosphere. We nd that in the full kinetic description EMIC waves can be generated inside the /stop bands", where they cannot exist in the coldplasma approximation. Besides, the wave spectrum is limited in wave numbers: all wave numbers above k p=vA experience strong cyclotron damping. Furthermore, we show that in the cyclotron resonance condition between EMIC waves and relativistic electrons the wave frequency is negligible.
Czech name
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Czech description
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Classification
Type
O - Miscellaneous
CEP classification
DG - Atmospheric sciences, meteorology
OECD FORD branch
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Result continuities
Project
<a href="/en/project/LG11032" target="_blank" >LG11032: COSPAR 2011-2013</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů