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Flattening of the Density Spectrum in Compressible Hall-MHD Simulations

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F21%3A00548646" target="_blank" >RIV/67985815:_____/21:00548646 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216208:11320/21:10439878

  • Result on the web

    <a href="http://hdl.handle.net/11104/0324688" target="_blank" >http://hdl.handle.net/11104/0324688</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.3390/atmos12091162" target="_blank" >10.3390/atmos12091162</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Flattening of the Density Spectrum in Compressible Hall-MHD Simulations

  • Original language description

    Observations of proton density fluctuations of the solar wind at 1 au have shown the presence of a decade-long transition region of the density spectrum above sub-ion scales, characterized by a flattening of the spectral slope. We use the proton density fluctuations data collected by the BMSW instrument on-board the Spektr-R satellite in order to delimit the plasma parameters under which the transition region can be observed. Under similar plasma conditions to those in observations, we carry out 3D compressible magnetohydrodynamics (MHD) and Hall-MHD numerical simulations and find that Hall physics is necessary to generate the transition region. The analysis of the k omega power spectrum in the Hall-MHD simulation indicates that the flattening of the density spectrum is associated with fluctuations having frequencies smaller than the ion cyclotron frequency.

  • 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

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GA19-18993S" target="_blank" >GA19-18993S: Transport of energy of solar wind variations from larger to smaller scales</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2021

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Atmosphere

  • ISSN

    2073-4433

  • e-ISSN

    2073-4433

  • Volume of the periodical

    12

  • Issue of the periodical within the volume

    9

  • Country of publishing house

    CH - SWITZERLAND

  • Number of pages

    16

  • Pages from-to

    1162

  • UT code for WoS article

    000699323800001

  • EID of the result in the Scopus database

    2-s2.0-85114735692