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Statements

Subject Item
n2:RIV%2F00216305%3A26310%2F04%3APU47580%21RIV06-GA0-26310___
rdf:type
n9:Vysledek skos:Concept
dcterms: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 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. 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
dcterms:title
Metodika stanovení rotační teploty z molekulového spektra a její statistické zhodnocení 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
skos:prefLabel
Metodika stanovení rotační teploty z molekulového spektra a její statistické zhodnocení 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
skos:notation
RIV/00216305:26310/04:PU47580!RIV06-GA0-26310___
n5:strany
72-75
n5:aktivita
n10:P
n5:aktivity
P(GD202/03/H162)
n5:dodaniDat
n6:2006
n5:domaciTvurceVysledku
n17:5127416
n5:druhVysledku
n16:D
n5:duvernostUdaju
n20:S
n5:entitaPredkladatele
n8:predkladatel
n5:idSjednocenehoVysledku
573153
n5:idVysledku
RIV/00216305:26310/04:PU47580
n5:jazykVysledku
n14:eng
n5: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
n5:klicoveSlovo
n12:spectroscopy n12:neutral%20gas%20temperature n12:Knaus%20and%20Caye%27s%20method n12:data n12:Determination%20of%20rotational%20temperature n12:Orstein-van%20Wijkov%20method n12:pyrometric%20line n12:uncertainty%20A n12:uncertainty%20B n12:combined%20standard%20uncertainty n12:optical%20spectra n12:extended%20uncertainty
n5:kontrolniKodProRIV
[953C1F1C0B21]
n5:mistoKonaniAkce
Rennes
n5:mistoVydani
Rennes
n5:nazevZdroje
Contributed Papers of ECAMP VIII
n5:obor
n19:CF
n5:pocetDomacichTvurcuVysledku
1
n5:pocetTvurcuVysledku
1
n5:projekt
n11:GD202%2F03%2FH162
n5:rokUplatneniVysledku
n6:2004
n5:tvurceVysledku
Šormová, Hana
n5:typAkce
n18:WRD
n5:zahajeniAkce
2004-06-06+02:00
s:numberOfPages
4
n7:hasPublisher
Universite Rennes
n13:isbn
2-914771-21-5
n21:organizacniJednotka
26310