MHD flows at astropauses and in astrotails

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00440041" target="_blank" >RIV/67985815:_____/14:00440041 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.5194/ap-1-51-2014" target="_blank" >http://dx.doi.org/10.5194/ap-1-51-2014</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.5194/ap-1-51-2014" target="_blank" >10.5194/ap-1-51-2014</a>

Result language
angličtina
Original language name
MHD flows at astropauses and in astrotails
Original language description
Our goal is to provide a proper representation and classification of counter-flow config- urations and counter-flow interfaces in the frame of fluid theory. In addition we calculate flows and large-scale electromagnetic fields based on which the large-scale dynamics and its role as possible background for parti- cle acceleration, e.g., in the form of anomalous cosmic rays, can be studied. We find that for the definition of the boundaries, which are determining the astropause shape, the number and location of magnetic null points and stagnation points is essential. Multiple separatrices can exist, forming a highly complex environment for the interstellar and stellar plasma.
Czech name
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Czech description
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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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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2014
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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