CDSD-4000: High-resolution, high-temperature carbon dioxide spectroscopic databank

Tashkun, S.A.; Perevalov, V. I.

doi:10.1016/j.jqsrt.2011.03.005

Cited by 240 publications

(124 citation statements)

References 84 publications

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“…The characteristic particle size was 0.1-3 µm, while particles over 5 µm in size were not practically observed [189]. On 7 August, according to ground-based observations, the AOT value at a 500 nm wavelength was as high as 6.4 in Moscow and 5.9 in Moscow environs [190]; according to satellite-borne observations, AOT (at a 500 nm wavelength) reached a maximum of 4.86 [191].…”

Section: Tropospheric Aerosol Cloud Condensation Nuclei Ice Nucleimentioning

confidence: 88%

“…The chemical composition of aerosol is thoroughly analyzed in [185]; an abnormally intensive condensation activity (Henel parameter) of the 2010 smoke (0.2-0.4) is pointed out, which proved to be significantly higher than that for the 2002 smoke (0.1-0.15) [195]. During the smoke period, almost a 20-fold increase of the amount of active condensation nuclei was revealed, which produced conditions for aerosol particle moisturizing and acid smog formation [189].…”

Section: Tropospheric Aerosol Cloud Condensation Nuclei Ice Nucleimentioning

confidence: 95%

“…Significant topic is related with modeling of potential effects of methane hydrates associated with climate warming and permafrost degradation [133,141,142,154,164,165,[169][170][171]. For long-term climate simulations and for adequate interpretation of paleoreconstructions it is necessary to develop corresponding ice sheet models [189][190][191].…”

Section: Climate Theory and Climate System Modelingmentioning

confidence: 99%

See 2 more Smart Citations

Russian National Report: Meteorology and Atmospheric Sciences

Мохов¹,

Krivolutsky²

2015

Geoinformatics Research Papers

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Section: Tropospheric Aerosol Cloud Condensation Nuclei Ice Nucleimentioning

confidence: 88%

Section: Tropospheric Aerosol Cloud Condensation Nuclei Ice Nucleimentioning

confidence: 95%

Section: Climate Theory and Climate System Modelingmentioning

confidence: 99%

See 1 more Smart Citation

Russian National Report: Meteorology and Atmospheric Sciences

Мохов¹,

Krivolutsky²

2015

Geoinformatics Research Papers

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“…The other molecules were simulated using HITRAN 2008 (Rothman et al 2013) line list cross sections) of a series of molecules of astrophysical and planetological relevance (BT2 for water (Barber et al 2006; Fig. 13), CDSD-4000 for CO 2 (Tashkun and Perevalov 2011), as well as some hot spectra for NH 3 (Hargreaves et al 2011;Yurchenko et al 2011;Zobov et al 2011;Fig. 13), HCN (Harris et al 2008;Mellau 2011) and CH 4 (Nassar and Bernath 2003;Thiévin et al 2008;Hargreaves et al 2012;Yurchenko et al, in prep.)).…”

Section: Status Of Current Databases For Hot Temperaturesmentioning

confidence: 99%

Spectroscopy of planetary atmospheres in our Galaxy

Tinetti

Encrenaz

Coustenis

2013

Astron Astrophys Rev

130

111

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About 20 years after the discovery of the first extrasolar planet, the number of planets known has grown by three orders of magnitude, and continues to increase at neck breaking pace. For most of these planets we have little information, except for the fact that they exist and possess an address in our Galaxy. For about one third of them, we know how much they weigh, their size and their orbital parameters. For less than 20, we start to have some clues about their atmospheric temperature and composition. How do we make progress from here?We are still far from the completion of a hypothetical Hertzsprung-Russell diagram for planets comparable to what we have for stars, and today we do not even know whether such classification will ever be possible or even meaningful for planetary objects. But one thing is clear: planetary parameters such as mass, radius and temperature alone do not explain the diversity revealed by current observations. The chemical composition of these planets is needed to trace back their formation history and evolution, as happened for the planets in our Solar System. As in situ measurements are and will remain off-limits for exoplanets, to study their chemical composition we will have to rely on remote sensing spectroscopic observations of their gaseous envelopes.

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“…Its estimation requires the knowledge of several data: energies of the molecular states, population number densities and degeneracy factors of the emitting states, internal partition functions, line positions, their rovibrational transition probabilities and Höln-London factors. Some of them are available in previous published papers [49][50][51][52] and in on-line databanks, [53][54][55] and can be compared with numerical software. 56,57 When data are not available for a molecular species, its radiation is neglected.…”

Section: Estimation Of the Radiative Lossesmentioning

confidence: 99%

Basic knowledge on radiative and transport properties to begin in thermal plasmas modelling

Cressault

2015

AIP Advances

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This paper has for objectives to present the radiative and the transport properties for people beginning in thermal plasmas. The first section will briefly recall the equations defined in numerical models applied to thermal plasmas; the second section will particularly deal with the estimation of radiative losses; the third part will quickly present the thermodynamics properties; and the last part will concern the transport coefficients (thermal conductivity, viscosity and electrical conductivity of the gas or mixtures of gases). We shall conclude the paper with a discussion about the validity of these results the lack of data for some specific applications, and some perspectives concerning these properties for non-equilibrium thermal plasmas. C 2015 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution 3.0 Unported License. [http://dx

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CDSD-4000: High-resolution, high-temperature carbon dioxide spectroscopic databank

Cited by 240 publications

References 84 publications

Russian National Report: Meteorology and Atmospheric Sciences

Russian National Report: Meteorology and Atmospheric Sciences

Spectroscopy of planetary atmospheres in our Galaxy

Basic knowledge on radiative and transport properties to begin in thermal plasmas modelling

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