Evolution of small-scale structures in and around a large solar pore.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F02%3A01020171" target="_blank" >RIV/67985815:_____/02:01020171 - 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
Evolution of small-scale structures in and around a large solar pore.
Original language description
The evolution of a filamentary structure adjecent to a large solar pore was studied. A clockwise rotation of this structure around the center of the pore was observed. It was found that the filamentary structure was different from a normal penumbra.
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
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Continuities
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
Solar variabiliy: from core to outer frontiers.
ISBN
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ISSN
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e-ISSN
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Number of pages
4
Pages from-to
435-438
Publisher name
ESA Publication Division
Place of publication
Noordwijk
Event location
Praha [CZ]
Event date
Sep 9, 2002
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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