Magnetic and velocity fields of a solar pore

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F12%3A00386890" target="_blank" >RIV/67985815:_____/12:00386890 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201117851" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201117851</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201117851" target="_blank" >10.1051/0004-6361/201117851</a>

Result language
angličtina
Original language name
Magnetic and velocity fields of a solar pore
Original language description
Relations between the magnetic field components, line-of-sight velocities, and horizontal motions in and around a large pore are analysed to provide observational constraints on theoretical models and numerical simulations.
Czech name
—
Czech description
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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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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
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Result description