Metodika stanovení rotační teploty z molekulového spektra a její statistické zhodnocení

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216305%3A26310%2F04%3APU47580" target="_blank" >RIV/00216305:26310/04:PU47580 - isvavai.cz</a>

Výsledek na webu

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DOI - Digital Object Identifier

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Jazyk výsledku

angličtina

Název v původním jazyce

Methods of the determination of the rotational temperature from molecular spectra and their statistics

Popis výsledku v původním jazyce

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 s

Název v anglickém jazyce

Methods of the determination of the rotational temperature from molecular spectra and their statistics

Popis výsledku anglicky

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 s

Druh

D - Stať ve sborníku

CEP obor

CF - Fyzikální chemie a teoretická chemie

OECD FORD obor

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Projekt

<a href="/cs/project/GD202%2F03%2FH162" target="_blank" >GD202/03/H162: Pokročilé směry ve fyzice a chemii plazmatu</a><br>

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Rok uplatnění

2004

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název statě ve sborníku

Contributed Papers of ECAMP VIII

ISBN

2-914771-21-5

ISSN

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e-ISSN

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Počet stran výsledku

4

Strana od-do

72-75

Název nakladatele

Universite Rennes

Místo vydání

Rennes

Místo konání akce

Rennes

Datum konání akce

6. 6. 2004

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

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