A 3-D look into the atmosphere?

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F10%3A00049542" target="_blank" >RIV/00216224:14310/10:00049542 - isvavai.cz</a>
Result on the web
<a href="http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=7915275" target="_blank" >http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=7915275</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1017/S1743921310008550" target="_blank" >10.1017/S1743921310008550</a>

Result language
angličtina
Original language name
A 3-D look into the atmosphere?
Original language description
The atmospheres of chemically peculiar stars can be highly structured in both the horizontal and vertical dimensions. While most prevalent in the magnetic stars, these structures can also exist in non-magnetic stars. In addition to providing an importantwindow to understanding the physical processes at play in these complex atmospheres, they can also be exploited to study stellar pulsations. This article reviews contributions to the session "A 3D look into the atmosphere" of the Joint Discussion "Progress in understanding the physics of Ap and related stars". It is divided into 3 sections: "Magnetic field and surface structures", "Pulsations in the atmospheres of roAp stars/inversions", and "Spectral synthesis/atmospheric models".
Czech name
—
Czech description
—

Project
<a href="/en/project/IAA301630901" target="_blank" >IAA301630901: Spectral energy distribution of hot stars and its variability</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

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

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