Radiative transfer in solar prominences
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00452637" target="_blank" >RIV/67985815:_____/15:00452637 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1007/978-3-319-10416-4_5" target="_blank" >http://dx.doi.org/10.1007/978-3-319-10416-4_5</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/978-3-319-10416-4_5" target="_blank" >10.1007/978-3-319-10416-4_5</a>
Alternative languages
Result language
angličtina
Original language name
Radiative transfer in solar prominences
Original language description
We describe the basics of the NLTE radiative-transfer theory applied to typical prominence conditions and demonstrate why the NLTE approach is necessary. Starting from the simplest 1D slab models, we gradually move to more complex problems which include2D transfer, importance of partial redistribution in the formation of resonance lines and details of multilevel problems including the most up-to-date numerical methods for constructing NLTE models. We also mention some recent achievements in prominencemodeling (e.g. magnetic dips, radiative equilibrium models, oscillations), although detailed description of such results is the subject of other chapters.
Czech name
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Czech description
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Classification
Type
C - Chapter in a specialist book
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Book/collection name
Solar Prominences
ISBN
9783319104157
Number of pages of the result
29
Pages from-to
103-130
Number of pages of the book
488
Publisher name
Springer
Place of publication
Cham
UT code for WoS chapter
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