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Spatial distribution of Langmuir waves observed upstream of Saturn's bow shock by Cassini

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F16%3A00464282" target="_blank" >RIV/68378289:_____/16:00464282 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216208:11320/16:10334335

  • Result on the web

    <a href="http://dx.doi.org/10.1002/2016JA022912" target="_blank" >http://dx.doi.org/10.1002/2016JA022912</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1002/2016JA022912" target="_blank" >10.1002/2016JA022912</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Spatial distribution of Langmuir waves observed upstream of Saturn's bow shock by Cassini

  • Original language description

    We present the spatial distribution and spectral properties of Langmuir waves observed upstream of Saturn's bow shock by the Cassini spacecraft. The entire 10 kHz wideband data set obtained between June 2004 and December 2014 has been analyzed using an automated procedure. Almost 106 waveform snapshots with intense narrowband emissions in the frequency range of 1–10 kHz were detected. A typical wave spectrum exhibits a single intense peak (62% of all selected waveforms). However, spectra with a superposition of two (25%) or more (13%) intense peaks are also observed. Using magnetic field observations and a model of the bow shock, plasma wave activity across Saturn's foreshock has been mapped. The plasma wave occurrence increases steeply behind the tangent magnetic field line, i.e., the sunward foreshock boundary, and rises with increasing distance from the tangential line into the downstream region. The single peak spectra are observed across the entire foreshock, while more complicated spectra are more likely measured deeper inside the foreshock and closer to the bow shock. We confirm that the most intense waves occur close to the tangent point and decrease both deeper in the foreshock and along the tangential line.

  • 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

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2016

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Journal of Geophysical Research: Space Physics

  • ISSN

    2169-9380

  • e-ISSN

  • Volume of the periodical

    121

  • Issue of the periodical within the volume

    8

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    14

  • Pages from-to

    7771-7784

  • UT code for WoS article

    000385811500032

  • EID of the result in the Scopus database

    2-s2.0-84983453525