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VLF Transmitter Signals Observed by the Cluster Spacecraft Over a Wide Range of Latitudes

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F25%3A00617310" target="_blank" >RIV/68378289:_____/25:00617310 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216208:11320/25:10510153

  • Result on the web

    <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2024JA033621" target="_blank" >https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2024JA033621</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1029/2024JA033621" target="_blank" >10.1029/2024JA033621</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    VLF Transmitter Signals Observed by the Cluster Spacecraft Over a Wide Range of Latitudes

  • Original language description

    Very low frequency transmitter signals can penetrate through the ionosphere and propagate in the inner magnetosphere, being observed by spacecraft instruments with sufficient frequency resolution and range. We use 23 years of measurements performed by the Waves of High frequency and Sounder for Probing of Electron density by Relaxation instrument on board the four Cluster spacecraft at frequencies up to 80 kHz to investigate the observed wave intensities. The transmitter signals are about an order of magnitude more intense during the night than during the day, and they are apparently confined within the plasmasphere. The extensive latitudinal coverage of the measurements allows us to investigate frequency cut-offs observed in the transmitter spectra. These are mostly in line with nonducted propagation, but occasional partial ducting seems to be necessary to explain signals spanning otherwise inaccessible regions. Finally, we compare the observed intensity patterns with the calculations of Starks et al. (2020), . Although overall agreement is obtained, the observed wave intensities tend to be a factor of about 2-3 lower than the calculated intensities.

  • 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

    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

    2025

  • 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

    2169-9402

  • Volume of the periodical

    130

  • Issue of the periodical within the volume

    2

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    13

  • Pages from-to

    e2024JA033621

  • UT code for WoS article

    001419373600001

  • EID of the result in the Scopus database

    2-s2.0-85218980535