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Interplanetary Magnetic Field B-y Controls the Magnetopause Location

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F23%3A00573095" target="_blank" >RIV/68378289:_____/23:00573095 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216208:11320/23:10468279

  • Result on the web

    <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2023JA031303" target="_blank" >https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2023JA031303</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1029/2023JA031303" target="_blank" >10.1029/2023JA031303</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Interplanetary Magnetic Field B-y Controls the Magnetopause Location

  • Original language description

    We present a statistical study of interplanetary magnetic field (IMF) effects on the magnetopause location based on nearly 15,000 magnetopause crossings identified in the THEMIS A-E, Magion 4, Geotail, and Interball-1 satellite data. In order to exclude the dominant controlling role of the solar wind dynamic pressure, differences between observed and empirical model magnetopause distances are analyzed. We find that the magnetopause distance is significantly controlled by the IMF clock angle, not considered in the used empirical models. Furthermore, during very low Alfven Mach numbers (M-A < 4), IMF B-y component can induce a considerable dawn-dusk asymmetry of the magnetopause shape. The magnetopause distance is found to be larger in the direction of the IMF vector, that is, not only the magnitude but also the orientation of the IMF B-y component is eventually important. The obtained results are qualitatively consistent with a magnetohydrodynamic model run at the Community Coordinated Modeling Center.

  • 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

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2023

  • 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

    128

  • Issue of the periodical within the volume

    5

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    8

  • Pages from-to

    e2023JA031303

  • UT code for WoS article

    001000426400001

  • EID of the result in the Scopus database

    2-s2.0-85160418602