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Comparison of Observed and Modeled Magnetic Fields in the Earth's Magnetosheath

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F20%3A00536925" target="_blank" >RIV/67985815:_____/20:00536925 - isvavai.cz</a>

  • Alternative codes found

    RIV/68378289:_____/20:00536925

  • Result on the web

    <a href="https://doi.org/10.1029/2019JA027705" target="_blank" >https://doi.org/10.1029/2019JA027705</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1029/2019JA027705" target="_blank" >10.1029/2019JA027705</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Comparison of Observed and Modeled Magnetic Fields in the Earth's Magnetosheath

  • Original language description

    Observations of the magnetic field for two passages through the Earth's magnetosheath are used for comparison with two simple models of the magnetosheath field that describe it as a potential field. We apply the Kobel and Fluckiger (1994, https://doi.org/10.1029/94JA01778) model and the Romashets and Vandas (2019, https://doi.org/10.1029/2006JA012072) model complemented with the Jelinek et al. (2012, https://doi.org/10.1029/2011JA017252) empirical determination of the bow shock and magnetopause shapes and positions. The models yield a satisfactory match to observations when the positions and shapes of the bow shock and the magnetopause are controlled by the instantaneous solar wind upstream dynamic pressure and the instantaneous upstream interplanetary magnetic field vector is taken into account.

  • 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/GA17-06065S" target="_blank" >GA17-06065S: Solar wind variations and their impact on magnetospheric dynamics</a><br>

  • 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

    2169-9402

  • e-ISSN

  • Volume of the periodical

    125

  • Issue of the periodical within the volume

    3

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    16

  • Pages from-to

    e2019JA027705

  • UT code for WoS article

    000535389600036

  • EID of the result in the Scopus database

    2-s2.0-85082311941