Evolution of Umbral Dots and Penumbral Grains

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F10%3A00355591" target="_blank" >RIV/67985815:_____/10:00355591 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Evolution of Umbral Dots and Penumbral Grains
Original language description
On 27 February 2007, Hinode SOT/SP acquired a time series of full-Stokes spectra of a regular, medium-sized sunspot NOAA 10944 located near the center of the solar disk. The inversion code SIR (Ruiz Cobo and del Toro Iniesta 1992, ApJ 398, 375) was applied to these data and a 3-h long time series of 34 spatial 3D maps of plasma parameters in the umbra and penumbra were computed. The temporal and spatial resolutions are 5.5 min and 0 :0032, respectively. A simultaneous series of SOT/BFI G-band images wasutilized for complementary measurements of horizontal motions and sizes of small-scale features.
Czech name
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Czech description
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Project
<a href="/en/project/IAA300030808" target="_blank" >IAA300030808: Interaction of moving plasma with magnetic fields in the solar photosphere</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year
2010
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Magnetic Coupling between the Interior and Atmosphere of the Sun
ISBN
978-3-642-02858-8
ISSN
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e-ISSN
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Number of pages
2
Pages from-to
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Publisher name
Springer
Place of publication
Berlin
Event location
Bangalore
Event date
Dec 2, 2008
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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