Chianti-an atomic database for euv emission lines
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| Format: | Artículo científico |
| Langue: | en |
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Universidad Nacional Autónoma de México
2000
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| _version_ | 1876449075883147264 |
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| author | Enrico Landi |
| author_facet | Enrico Landi |
| contents | Chianti-an atomic database for euv emission lines Enrico Landi Física, Astronomía y Matemáticas TECH PLASMAS ATOMIC DATA LINE:FORMATION NIQUES: SPECTROSCOPIC CHIANTI consists of a critically evaluated set of atomic data and transitionprobabilities necessary to calculate the emission line spectrum of astrophysicalplasmas. The data consist of atomic energy levels, atomic radiative data such aswavelengths, weighted oscillator strengths and A values, and electron collisionalexcitation rates. A set of programs that use these data to calculate the spectrumin a desired wavelength range as a function of temperature and density is also provided.A suite of programs has been developed to carry out plasma diagnostics ofastrophysical plasmas. The state-of-the-art contents of the CHIANTI database willbe described and some of the most important results obtained from the use of theCHIANTI database will be reviewed. 2000 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57100935 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.9 |
| format | Artículo científico |
| id | redalyc_57100935 |
| institution | Redalyc |
| language | en |
| publishDate | 2000 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | Chianti-an atomic database for euv emission lines Enrico Landi Física, Astronomía y Matemáticas TECH PLASMAS ATOMIC DATA LINE:FORMATION NIQUES: SPECTROSCOPIC Chianti-an atomic database for euv emission lines Enrico Landi Física, Astronomía y Matemáticas TECH PLASMAS ATOMIC DATA LINE:FORMATION NIQUES: SPECTROSCOPIC CHIANTI consists of a critically evaluated set of atomic data and transitionprobabilities necessary to calculate the emission line spectrum of astrophysicalplasmas. The data consist of atomic energy levels, atomic radiative data such aswavelengths, weighted oscillator strengths and A values, and electron collisionalexcitation rates. A set of programs that use these data to calculate the spectrumin a desired wavelength range as a function of temperature and density is also provided.A suite of programs has been developed to carry out plasma diagnostics ofastrophysical plasmas. The state-of-the-art contents of the CHIANTI database willbe described and some of the most important results obtained from the use of theCHIANTI database will be reviewed. 2000 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57100935 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.9 |
| title | Chianti-an atomic database for euv emission lines |
| topic | Física, Astronomía y Matemáticas TECH PLASMAS ATOMIC DATA LINE:FORMATION NIQUES: SPECTROSCOPIC |
| url | https://www.redalyc.org/articulo.oa?id=57100935 |