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Intense plasma wave emissions associated with Saturn's moon Rhea

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F11%3A10108203" target="_blank" >RIV/00216208:11320/11:10108203 - isvavai.cz</a>

  • Alternative codes found

    RIV/68378289:_____/11:00367417

  • Result on the web

    <a href="http://dx.doi.org/10.1029/2011GL049219" target="_blank" >http://dx.doi.org/10.1029/2011GL049219</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1029/2011GL049219" target="_blank" >10.1029/2011GL049219</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Intense plasma wave emissions associated with Saturn's moon Rhea

  • Original language description

    Measurements by the Cassini spacecraft during a close flyby of Saturn's moon Rhea on March 2, 2010, show the presence of intense plasma waves in the magnetic flux tube connected to the surface of the moon. Three types of waves were observed, (1) bursty electrostatic waves near the electron plasma frequency, (2) intense whistler-mode emissions below one half of the electron cyclotron frequency, and (3) broadband electrostatic waves at frequencies well below the ion plasma frequency. The waves near the electron plasma frequency are believed to be driven by a low energy (similar to 35 eV) electron beam accelerated away from Rhea. Their bursty structure is believed to be due to a nonlinear process similar to the three-wave interaction that occurs for Langmuir waves in the solar wind. The whistler-mode emissions are propagating toward Rhea and are shown to be generated by the loss-cone anisotropy (at parallel cyclotron resonance energies around 230 eV) caused by absorption of electrons at t

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BL - Plasma physics and discharge through gases

  • OECD FORD branch

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Others

  • Publication year

    2011

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Geophysical Research Letteres

  • ISSN

    0094-8276

  • e-ISSN

  • Volume of the periodical

    38

  • Issue of the periodical within the volume

    19

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    7

  • Pages from-to

    "L19204", 1-7

  • UT code for WoS article

    000295976200005

  • EID of the result in the Scopus database