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Understanding Cassini RPWS Antenna Signals Triggered by Dust Impacts

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F19%3A00508230" target="_blank" >RIV/68378289:_____/19:00508230 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216208:11320/19:10405946

  • Result on the web

    <a href="https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2019GL084150" target="_blank" >https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2019GL084150</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1029/2019GL084150" target="_blank" >10.1029/2019GL084150</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Understanding Cassini RPWS Antenna Signals Triggered by Dust Impacts

  • Original language description

    Electric field antennas are capable of detecting dust impacts in different space environment. We analyze the dust impact signals detected by the Cassini Radio and Plasma Wave Science (RPWS) instrument at different locations around Saturn and compare them with dust impact signals simulated in laboratory conditions and numerically. The spacecraft potential, the size and capacitance of the impacted element, and ambient plasma have a strong effect on the amplitude and the shape of impact signals, providing important clues to understanding the signal generation mechanism. The voltage signal on the antenna is due to the separation of the impact generated charges, which occurs as electrons and ions can either escape (at different speeds) or be collected by the impacted element depending on the spacecraft potential.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10305 - Fluids and plasma physics (including surface physics)

Result continuities

  • Project

    <a href="/en/project/LTAUSA17066" target="_blank" >LTAUSA17066: Experimental investigations and computer modeling of dusty processes in space</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2019

  • 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 Letters

  • ISSN

    0094-8276

  • e-ISSN

  • Volume of the periodical

    46

  • Issue of the periodical within the volume

    20

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    10

  • Pages from-to

    10941-10950

  • UT code for WoS article

    000497365500002

  • EID of the result in the Scopus database

    2-s2.0-85074616301