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Conjugate Observations of Quasiperiodic Emissions by the Van Allen Probes Spacecraft and Ground-based Station Kannuslehto

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F20%3A00536255" target="_blank" >RIV/68378289:_____/20:00536255 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216208:11320/20:10413875

  • Result on the web

    <a href="https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2020JA027793" target="_blank" >https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2020JA027793</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1029/2020JA027793" target="_blank" >10.1029/2020JA027793</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Conjugate Observations of Quasiperiodic Emissions by the Van Allen Probes Spacecraft and Ground-based Station Kannuslehto

  • Original language description

    Whistler mode waves observed in the Earth's inner magnetosphere at frequencies between about 0.5 and 4 kHz which exhibit a nearly periodic time modulation of the wave intensity are called quasiperiodic (QP) emissions. Conjugate measurements of QP events at several different locations can be used to estimate their spatial extent and spatiotemporal variability. Results obtained using conjugate QP measurements provided by the ground-based station Kannuslehto (L approximate to 5.5) and the Van Allen Probes spacecraft (L shells between about 1.1 and 6.5) between September 2012 and November 2017 are presented. Altogether, 26 simultaneously detected events were analyzed. The event modulation periods and frequency-time structures were generally the same at all observation points. Spatial separations of the spacecraft and the ground-based station during conjugate observations are typically within about 40 degrees in azimuth and from about 1 to 3 in L shell. RBSP consistently observes events at lower L shells than Kannuslehto, with the event occurrence primarily inside of the plasmasphere. Ratios of Poynting fluxes observed by the spacecraft and on the ground are used to evaluate event intensity variations related to the spacecraft position. It is found that the intensity decreases considerably both at low L shells and outside of the plasmasphere. Finally, an event containing a gap in its frequency-time structure related to a sudden change of its properties is analyzed in detail.

  • 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

    2020

  • 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

    125

  • Issue of the periodical within the volume

    6

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    13

  • Pages from-to

    e2020JA027793

  • UT code for WoS article

    000545696000015

  • EID of the result in the Scopus database

    2-s2.0-85087064080