Evolving large-scale magnetic field and the global convection 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_____%2F02%3A01020147" target="_blank" >RIV/67985815:_____/02:01020147 - 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
Evolving large-scale magnetic field and the global convection on the Sun.
Original language description
The aim of the study is to demonstrate a role of dynamical properties of the large-scale magnetic flux during formation of the helical magnetic structures and a preparation of the pre-flare configurations in the solar atmosphere.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
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)<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
Article name in the collection
SOLMAG 2002. Proceedings of the magnetic coupling of the solar atmosphere euroconference and IAU colloquium 188.
ISBN
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ISSN
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e-ISSN
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Number of pages
4
Pages from-to
333-336
Publisher name
ESA Publication Division
Place of publication
Noordwijk
Event location
Santorini [GR]
Event date
Jun 11, 2002
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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