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Predictive model of magnetosheath plasma flow and its validation against Cluster and THEMIS data

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F12%3A00378977" target="_blank" >RIV/68378289:_____/12:00378977 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.5194/angeo-30-973-2012" target="_blank" >http://dx.doi.org/10.5194/angeo-30-973-2012</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.5194/angeo-30-973-2012" target="_blank" >10.5194/angeo-30-973-2012</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Predictive model of magnetosheath plasma flow and its validation against Cluster and THEMIS data

  • Original language description

    An analytical model of magnetosheath plasma flow is described and compared with a large dataset of magnetosheath ion flow velocity measurements from Cluster and THEMIS spacecraft. The model is based on previous works by Kobel and Fluckiger (1994) and G´enot et al. (2011) and has been modified to overcome the restrictions of these models on the shape of model magnetopause and bow shock. Our model is compatible with any parabolic bow shock model and arbitrary magnetopause model. The model is relatively simple to implement and computationally inexpensive, and its only inputs are upstream solar wind parameters. Comparison with observed data yields a good correspondence: median error in the direction of flow velocity is comparable with the instrumental error, and flow magnitude is predicted with a reasonable accuracy (relative error in flow speed was less than 25% for 86.5% of observations).

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/GAP209%2F12%2F2394" target="_blank" >GAP209/12/2394: The role of low frequency plasma waves in large scale dynamics of planetary magnetospheres</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2012

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Annales Geophysicae

  • ISSN

    0992-7689

  • e-ISSN

  • Volume of the periodical

    30

  • Issue of the periodical within the volume

    6

  • Country of publishing house

    DE - GERMANY

  • Number of pages

    10

  • Pages from-to

    973-982

  • UT code for WoS article

    000305838500007

  • EID of the result in the Scopus database