Spectral Line Shapes in Plasmas
Line-shape analysis is one of the most important tools for diagnostics of both laboratory and space plasmas. Its reliable implementation requires sufficiently accurate calculations, which imply the use of analytic methods and computer codes of varying complexity, and, necessarily, varying limits of...
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| Format: | Book Chapter |
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| Published: |
MDPI - Multidisciplinary Digital Publishing Institute
2015
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| Online Access: | Get Fullteks DOAB: description of the publication |
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| LEADER | 02077naaaa2200265uu 4500 | ||
|---|---|---|---|
| 001 | doab_20_500_12854_59825 | ||
| 005 | 20210212 | ||
| 020 | |a 9783906980829 | ||
| 020 | |a 9783906980812 | ||
| 041 | 0 | |a English | |
| 042 | |a dc | ||
| 245 | 1 | 0 | |a Spectral Line Shapes in Plasmas |
| 260 | |b MDPI - Multidisciplinary Digital Publishing Institute |c 2015 | ||
| 300 | |a 1 electronic resource (232 p.) | ||
| 506 | 0 | |a Open Access |2 star |f Unrestricted online access | |
| 520 | |a Line-shape analysis is one of the most important tools for diagnostics of both laboratory and space plasmas. Its reliable implementation requires sufficiently accurate calculations, which imply the use of analytic methods and computer codes of varying complexity, and, necessarily, varying limits of applicability and accuracy. However, studies comparing different computational and analytic methods are almost non-existent. The Spectral Line Shapes in Plasma (SLSP) code comparison workshop series [1] was established to fill this gap. Numerous computational cases considered in the two workshops organized to date (in April 2012 and August 2013 in Vienna, Austria) not only serve the purpose of code comparison, but also have applications in research of magnetic fusion, astrophysical, laser-produced plasmas, and so on. Therefore, although the first workshop was briefly reviewed elsewhere [2], and will likely be followed by a review of the second one, it was unanimously decided by the participants that a volume devoted to results of the workshops was desired. It is the main purpose of this special issue. | ||
| 540 | |a Creative Commons |f https://creativecommons.org/licenses/by/4.0/ |2 cc |4 https://creativecommons.org/licenses/by/4.0/ | ||
| 546 | |a English | ||
| 653 | |a Zeeman effect | ||
| 653 | |a code comparison | ||
| 653 | |a spectral line shapes | ||
| 653 | |a Stark effect | ||
| 653 | |a line broadening | ||
| 856 | 4 | 0 | |a www.oapen.org |u http://books.mdpi.com/pdfview/book/123 |7 0 |z Get Fullteks |
| 856 | 4 | 0 | |a www.oapen.org |u https://directory.doabooks.org/handle/20.500.12854/59825 |7 0 |z DOAB: description of the publication |