Semiempirical modeling of large-scale flow on the Sun.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F01%3A01010067" target="_blank" >RIV/67985815:_____/01:01010067 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Semiempirical modeling of large-scale flow on the Sun.
Original language description
Image of the 2-D large-scale flow on the sphere is derived from the trajectories of the independent fee testing particles driven by the derived velocity field. The horizontal flow displays a velocity gradient and an eddy structure. The sllow- and long-lived temporal evolution of the low structures is descibed.
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
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2001
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Solar Physics
ISSN
0038-0938
e-ISSN
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Volume of the periodical
199
Issue of the periodical within the volume
2
Country of publishing house
NL - THE KINGDOM OF THE NETHERLANDS
Number of pages
16
Pages from-to
251-266
UT code for WoS article
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EID of the result in the Scopus database
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