Plasma wave observations with Cassini at Saturn

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F16%3A00465509" target="_blank" >RIV/68378289:_____/16:00465509 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1002/9781119066880.ch22" target="_blank" >http://dx.doi.org/10.1002/9781119066880.ch22</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1002/9781119066880.ch22" target="_blank" >10.1002/9781119066880.ch22</a>

Result language
angličtina
Original language name
Plasma wave observations with Cassini at Saturn
Original language description
Since the Cassini spacecraft arrived at Saturn in 2004, the Radio and Plasma Wave Science (RPWS) investigation has detected a variety of radio and plasma waves in the magnetosphere of Saturn, including whistler mode chorus and hiss, lightning-produced whistlers, high latitude auroral hiss, electrostatic electron cyclotron harmonic (ECH), upper hybrid resonance (UHR) and Langmuir wave emissions, Z- and O-mode narrowband emissions, and Saturn kilometric radiation (SKR). A number of these emissions often exhibit intensity modulations with periods ranging from about 10.6 to 10.8 hours. Plasma waves have also been detected in association with the Saturnian moons, including Enceladus and Rhea. We will review these observations and discuss the properties of the various waves.
Czech name
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Czech description
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Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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