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
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Czech description
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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
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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
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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
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