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Injection of 40-kHz-modulated electron beam from the satellite: II. Excitation of electrostatic and whistler waves

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389005%3A_____%2F20%3A00531698" target="_blank" >RIV/61389005:_____/20:00531698 - isvavai.cz</a>

  • Alternative codes found

    RIV/68378289:_____/20:00531698

  • Result on the web

    <a href="https://www.sciencedirect.com/science/article/pii/S0273117719306106" target="_blank" >https://www.sciencedirect.com/science/article/pii/S0273117719306106</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.asr.2019.08.027" target="_blank" >10.1016/j.asr.2019.08.027</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Injection of 40-kHz-modulated electron beam from the satellite: II. Excitation of electrostatic and whistler waves

  • Original language description

    Beam-plasma interaction effects are studied during the active space experiment with electron and Xe-ion beam injections in an ionospheric plasma. Permanent 40-kHz-modulated electron beam injection occurs simultaneously with a xenon-ion beam injected by the Hall-type plasma thruster operating in a square-pulse mode (100/50 s for a job/pause duration). The unusual behavior of the background charged particle fluxes and wave activity stimulated during the beam-plasma interaction have been registered by the scientific instruments onboard Intercosmos-25 station (IK-25) and Magion-3 subsatellite. The longitudinal and electromagnetic wave instabilities and their mutual relationship are considered in order to explain the observed effects. The excitation of electrostatic waves by the electron injection has been considered for different resonance conditions near the linear stability boundary. Beam-driven electromagnetic instability is responsible for the backward-propagating whistler waves excited via cyclotron resonance. Competition of these two beam instabilities is one of the subjects of the present study.

  • 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

    10509 - Meteorology and atmospheric sciences

Result continuities

  • Project

    <a href="/en/project/EF15_003%2F0000481" target="_blank" >EF15_003/0000481: Research Center of Cosmic Rays and Radiation Events in the Atmosphere</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2020

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Advances in Space Research

  • ISSN

    0273-1177

  • e-ISSN

  • Volume of the periodical

    65

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    20

  • Pages from-to

    30-49

  • UT code for WoS article

    000509784600004

  • EID of the result in the Scopus database

    2-s2.0-85072285231