Dynamo model with thermal convection and free-rotating inner core.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985530%3A_____%2F02%3A03020038" target="_blank" >RIV/67985530:_____/02:03020038 - 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
Dynamo model with thermal convection and free-rotating inner core.
Original language description
The 2.5D approach is used to solve the dynamo model in the Boussinesq approximation. Thermal convection in a fast rotating spherical shell with a free-rotatin inner core is considered. In all cases the inner core rotates slightly faster than the outer boundary of the shell. The presented dynamo model reverses regularly without any external impulse.
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
DE - Earth magnetism, geodesy, geography
OECD FORD branch
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Result continuities
Project
<a href="/en/project/IAA3012006" target="_blank" >IAA3012006: Boussinesq approximation of the hydromagnetic dynamo of the Earth</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2002
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
50
Issue of the periodical within the volume
10/11
Country of publishing house
NL - THE KINGDOM OF THE NETHERLANDS
Number of pages
6
Pages from-to
1117-1122
UT code for WoS article
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EID of the result in the Scopus database
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