"Metodika stanoven\u00ED rota\u010Dn\u00ED teploty z molekulov\u00E9ho spektra a jej\u00ED statistick\u00E9 zhodnocen\u00ED"@cs . "Metodika stanoven\u00ED rota\u010Dn\u00ED teploty z molekulov\u00E9ho spektra a jej\u00ED statistick\u00E9 zhodnocen\u00ED"@cs . "Molecular spectra contain much information about their structure, position of atoms and also about the position of nucleus. It is possible to directly compute various layers of energy's levels of the researched molecule, determine information about the electron's structure and vibrational and rotational behavior of the molecule. Expect these features it is possible to detect the present of various molecules in stars, planets and comets, higher atmosphere and intercosmic space based on the interpretationn of molecular spectra. Also it is possible to predict physical conditions in these objects. In these objects there are usually a plasma, to identify their features it is needed to diagnose the plasma by measured molecular spectra. But finding plasma's parameters from spectral lines is not easy; it is generally a very complex problem. The cause of this problem is that except information about electron's transitions there are also vibrational and rotational transitions and the molecular spectrum is a com" . "573153" . . "Methods of the determination of the rotational temperature from molecular spectra and their statistics"@en . "Universite Rennes" . . . . "1"^^ . . . "1"^^ . "2-914771-21-5" . . . "\u0160ormov\u00E1, Hana" . "4"^^ . . "Molekulov\u00E1 spektra obsahuj\u00ED \u0159adu cenn\u00FDch informac\u00ED o struktu\u0159e a vlastnostech molekul. Lze vypo\u010D\u00EDtat nap\u0159. energiov\u00E9 hladiny, z\u00EDskat informace o elektronov\u00E9 struktu\u0159e, atd. V\u011Bt\u0161ina hmoty ve vesm\u00EDru je ve stavu plazmatu a proto je t\u0159eba se zab\u00FDvat problematikou stanoven\u00ED jeho parametr\u016F z molekulov\u00FDch spekter. Spektroskopie t\u011Bchto objekt\u016F p\u0159edstavuje komplikovan\u00FD probl\u00E9m. Pro stanoven\u00ED teploty neutr\u00E1ln\u00EDho plynu z rota\u010Dn\u011B rozli\u0161en\u00E9ho molekulov\u00E9ho spektra existuje standartn\u00ED postup, kter\u00FD ale nelze pou\u017E\u00EDt uu spekter s mal\u00FDm rozli\u0161en\u00EDm. K tomu lze vyu\u017E\u00EDt numerick\u00FDch simulac\u00ED. Ve v\u0161ech p\u0159\u00EDpadech je ale nezbytn\u00E9 \u0159e\u0161it probl\u00E9m p\u0159esnosti ur\u010Den\u00ED teploty."@cs . . . "Methods of the determination of the rotational temperature from molecular spectra and their statistics"@en . . . "Methods of the determination of the rotational temperature from molecular spectra and their statistics" . "RIV/00216305:26310/04:PU47580!RIV06-GA0-26310___" . "Methods of the determination of the rotational temperature from molecular spectra and their statistics" . . "P(GD202/03/H162)" . "2004-06-06+02:00"^^ . "Molecular spectra contain much information about their structure, position of atoms and also about the position of nucleus. It is possible to directly compute various layers of energy's levels of the researched molecule, determine information about the electron's structure and vibrational and rotational behavior of the molecule. Expect these features it is possible to detect the present of various molecules in stars, planets and comets, higher atmosphere and intercosmic space based on the interpretationn of molecular spectra. Also it is possible to predict physical conditions in these objects. In these objects there are usually a plasma, to identify their features it is needed to diagnose the plasma by measured molecular spectra. But finding plasma's parameters from spectral lines is not easy; it is generally a very complex problem. The cause of this problem is that except information about electron's transitions there are also vibrational and rotational transitions and the molecular spectrum is a com"@en . . . . . "72-75" . "[953C1F1C0B21]" . "Determination of rotational temperature, neutral gas temperature, Orstein-van Wijkov method, Knaus and Caye's method, pyrometric line, uncertainty A, uncertainty B, combined standard uncertainty, extended uncertainty, optical spectra, spectroscopy, data"@en . . "Contributed Papers of ECAMP VIII" . . . "RIV/00216305:26310/04:PU47580" . . . "Rennes" . . "Rennes" . . "26310" .