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Theories of Growth and Propagation of Parallel Whistler-Mode Chorus Emissions: A Review

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F24%3A00573219" target="_blank" >RIV/68378289:_____/24:00573219 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216208:11320/24:10477705

  • Result on the web

    <a href="https://link.springer.com/article/10.1007/s10712-023-09792-x" target="_blank" >https://link.springer.com/article/10.1007/s10712-023-09792-x</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1007/s10712-023-09792-x" target="_blank" >10.1007/s10712-023-09792-x</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Theories of Growth and Propagation of Parallel Whistler-Mode Chorus Emissions: A Review

  • Original language description

    The significant role of nonlinear wave-particle interactions in the macrodynamics and microdynamics of the Earth's outer radiation belt has long been recognised. Electron dropouts during magnetic storms, microbursts in atmospheric electron precipitation, and pulsating auroras are all associated with the rapid scattering of energetic electrons by the whistler-mode chorus, a structured electromagnetic emission known to reach amplitudes of about 1% of the ambient magnetic field. Despite the decades of experimental and theoretical investigations of chorus and the recent progress achieved through numerical simulations, there is no definitive theory of the chorus formation mechanism, not even in the simple case of parallel (one-dimensional) propagation. Here we follow the evolution of these theories from their beginnings in the 1960s to the current state, including newly emerging self-consistent excitation models. A critical review of the unique features of each approach is provided, taking into account the most recent spacecraft observations of the fine structure of chorus. Conflicting interpretations of the role of resonant electron current and magnetic field inhomogeneity are discussed. We also discuss the interplay between nonlinear growth and microscale propagation effects and identify future theoretical and observational challenges stemming from the two-dimensional aspects of chorus propagation.

  • 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

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2024

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Surveys in Geophysics

  • ISSN

    0169-3298

  • e-ISSN

    1573-0956

  • Volume of the periodical

    45

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    DE - GERMANY

  • Number of pages

    54

  • Pages from-to

    1-54

  • UT code for WoS article

    001000326800001

  • EID of the result in the Scopus database

    2-s2.0-85160832199