Interplanetary shock-bow shock interaction: Comparison of a global MHD model and observation
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F15%3A10319613" target="_blank" >RIV/00216208:11320/15:10319613 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1016/j.pss.2014.12.001" target="_blank" >http://dx.doi.org/10.1016/j.pss.2014.12.001</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.pss.2014.12.001" target="_blank" >10.1016/j.pss.2014.12.001</a>
Alternative languages
Result language
angličtina
Original language name
Interplanetary shock-bow shock interaction: Comparison of a global MHD model and observation
Original language description
A fast forward shock passing through the bow shock would generate a train of new discontinuities that differ with the distance from the Sun-Earth line. However, interplanetary (IP) shocks are often followed by a rotation of the interplanetary magnetic field (IMF) over a large angle and a presence of this rotation can modify the interaction process. The present paper analyzes in detail one IP shock where data measured by Wind are used as an input to a global BATS-R-US MHD model and the model prediction is compared with Geotail magnetosheath observations. The study is based on three runs of the global MHD model that use different modifications of upstream conditions. We have found that (1) about 45% of IP shocks is followed by a significant IMF rotationwithin 15 min after the shock ramp; (2) the IMF rotation modifies the dynamics of the magnetospheric response to the IP shock arrival; (3) a train of new discontinuities created by an interaction of the IP shock with bow shock can be iden
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
BL - Plasma physics and discharge through gases
OECD FORD branch
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Result continuities
Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
S - Specificky vyzkum na vysokych skolach<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Planetary and Space Science
ISSN
0032-0633
e-ISSN
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Volume of the periodical
115
Issue of the periodical within the volume
Sep
Country of publishing house
US - UNITED STATES
Number of pages
8
Pages from-to
4-11
UT code for WoS article
000360512300002
EID of the result in the Scopus database
2-s2.0-84938749334