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| rdf:type
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| Description
| - 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
- 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)
- Molekulová spektra obsahují řadu cenných informací o struktuře a vlastnostech molekul. Lze vypočítat např. energiové hladiny, získat informace o elektronové struktuře, atd. Většina hmoty ve vesmíru je ve stavu plazmatu a proto je třeba se zabývat problematikou stanovení jeho parametrů z molekulových spekter. Spektroskopie těchto objektů představuje komplikovaný problém. Pro stanovení teploty neutrálního plynu z rotačně rozlišeného molekulového spektra existuje standartní postup, který ale nelze použít uu spekter s malým rozlišením. K tomu lze využít numerických simulací. Ve všech případech je ale nezbytné řešit problém přesnosti určení teploty. (cs)
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| Title
| - Metodika stanovení rotační teploty z molekulového spektra a její statistické zhodnocení (cs)
- Methods of the determination of the rotational temperature from molecular spectra and their statistics
- Methods of the determination of the rotational temperature from molecular spectra and their statistics (en)
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| skos:prefLabel
| - Metodika stanovení rotační teploty z molekulového spektra a její statistické zhodnocení (cs)
- Methods of the determination of the rotational temperature from molecular spectra and their statistics
- Methods of the determination of the rotational temperature from molecular spectra and their statistics (en)
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| skos:notation
| - RIV/00216305:26310/04:PU47580!RIV06-GA0-26310___
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| http://linked.open.../vavai/riv/strany
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| http://linked.open...avai/riv/aktivita
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| http://linked.open...avai/riv/aktivity
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| http://linked.open...vai/riv/dodaniDat
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| http://linked.open...aciTvurceVysledku
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| http://linked.open.../riv/druhVysledku
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| http://linked.open...iv/duvernostUdaju
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| http://linked.open...titaPredkladatele
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| http://linked.open...dnocenehoVysledku
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| http://linked.open...ai/riv/idVysledku
| - RIV/00216305:26310/04:PU47580
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| http://linked.open...riv/jazykVysledku
| |
| http://linked.open.../riv/klicovaSlova
| - 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)
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| http://linked.open.../riv/klicoveSlovo
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| http://linked.open...ontrolniKodProRIV
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| http://linked.open...v/mistoKonaniAkce
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| http://linked.open...i/riv/mistoVydani
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| http://linked.open...i/riv/nazevZdroje
| - Contributed Papers of ECAMP VIII
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| http://linked.open...in/vavai/riv/obor
| |
| http://linked.open...ichTvurcuVysledku
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| http://linked.open...cetTvurcuVysledku
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| http://linked.open...vavai/riv/projekt
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| http://linked.open...UplatneniVysledku
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| http://linked.open...iv/tvurceVysledku
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| http://linked.open...vavai/riv/typAkce
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| http://linked.open.../riv/zahajeniAkce
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| number of pages
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| http://purl.org/ne...btex#hasPublisher
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| https://schema.org/isbn
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| http://localhost/t...ganizacniJednotka
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