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Bow Shock Eigenmodes and Their Interconnection with Magnetospheric Resonances

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F22%3A10456507" target="_blank" >RIV/00216208:11320/22:10456507 - isvavai.cz</a>

  • Result on the web

    <a href="https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=LehxfIgf7U" target="_blank" >https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=LehxfIgf7U</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1134/S1063776122030116" target="_blank" >10.1134/S1063776122030116</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Bow Shock Eigenmodes and Their Interconnection with Magnetospheric Resonances

  • Original language description

    Resonant modes with frequencies 0.02-10 mHz are detected from the bow shock (BS) to the outer magnetosphere, with the nature of the resonances at frequencies 0.02-0.25 mHz being still unexplained. We propose a BS model in the form of a circular plate free along the outer edge that predicts resonant modes at frequencies 0.02-0.3 mHz or lower. We demonstrate the detection of these model resonant modes based on data from five satellites, with the resonance near 0.1 mHz predicted by the model being observed in the magnetosheath continuously for 17 hours downstream of both parallel and perpendicular shocks. Resonant BS modes produce three-wave nonlinear cascades that realize a broadband coherent coupling with resonances both near and inside the magnetopause. In our opinion, it is the coherent nature of the processes in an extended region with different linear resonant eigenmodes that determines the fairly new, nonlinear-cascade, approach to an efficient conversion of the energy of an inflow when interacting with an obstacle. This seems important for the entire nonlinear physics. We also provide arguments suggesting the possibility of resonant mode self-generation in the closed BS/magnetopause loop with a feedback in the form of narrow Poynting vector pulses at the cost of solar wind energy.

  • 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/GA21-26463S" target="_blank" >GA21-26463S: Magnetopause processes, their drivers and consequences</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2022

  • 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 Experimental and Theoretical Physics

  • ISSN

    1063-7761

  • e-ISSN

    1090-6509

  • Volume of the periodical

    134

  • Issue of the periodical within the volume

    3

  • Country of publishing house

    RU - RUSSIAN FEDERATION

  • Number of pages

    6

  • Pages from-to

    321-326

  • UT code for WoS article

    000789845600008

  • EID of the result in the Scopus database

    2-s2.0-85129261880