2008
DOI: 10.1615/hightempmatproc.v12.i3-4.30
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Advanced Thermal Plasma Modelling

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Cited by 35 publications
(37 citation statements)
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“…According to relation (4), the crucial point of the study is the treatment of the lines' intensities which depends on the lines' profiles and consequently on the broadenings effects: Doppler, Van der Waals, resonance and Stark broadenings. [41][42][43][44] The treatment of the lines is thus a complex and long step since they are numerous in thermal plasmas (15150 lines for SF 6 47 as examples. In this case, we need more than 300000 wavelengths to obtain a fine and correct description of the spectra (between 1 and 3 million wavelengths are needed if the molecular bands have to be considered; 37,48,49 the spectral resolution of the absorption coefficient cannot be taken as constant and depends on the nature of the species mixed in the plasmas (from 10 −3 nm to 10 −1 nm for SF 6 -C 2 F 4 plasmas; 48 the lines' profiles must be calculated on spectral ranges being more than 100 times the half width at half maximum.…”
Section: Estimation Of the Radiative Lossesmentioning
confidence: 99%
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“…According to relation (4), the crucial point of the study is the treatment of the lines' intensities which depends on the lines' profiles and consequently on the broadenings effects: Doppler, Van der Waals, resonance and Stark broadenings. [41][42][43][44] The treatment of the lines is thus a complex and long step since they are numerous in thermal plasmas (15150 lines for SF 6 47 as examples. In this case, we need more than 300000 wavelengths to obtain a fine and correct description of the spectra (between 1 and 3 million wavelengths are needed if the molecular bands have to be considered; 37,48,49 the spectral resolution of the absorption coefficient cannot be taken as constant and depends on the nature of the species mixed in the plasmas (from 10 −3 nm to 10 −1 nm for SF 6 -C 2 F 4 plasmas; 48 the lines' profiles must be calculated on spectral ranges being more than 100 times the half width at half maximum.…”
Section: Estimation Of the Radiative Lossesmentioning
confidence: 99%
“…An example of the divergence of the flux is shown in Fig. 5 in the case of pure SF 6 High Voltage Circuit Breaker. 45 The results were obtained with the Net Emission Coefficient (NEC), with the P1 model using the mean absorption coefficients deduced from the Rosseland or the Planck approximations, and compared to a fine resolution of the equation (3) for a given temperature profile (see the work of Randrianandraina et al 45 ) for the definition of the mean absorption coefficients, for the discretisation and the temperature profile).…”
Section: Estimation Of the Radiative Lossesmentioning
confidence: 99%
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“…To take all the effects into account would require treating the transport and reactions of each plasma species separately. This would inevitably introduce inaccuracies because of the lack of available reaction data and uncertainties about appropriate calculation of thermodynamic and transport properties [27,28].…”
Section: Numerical Modelmentioning
confidence: 99%