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- W2078643496 abstract "A fast method is presented for calculating the net emitted spectrum of a spherical sulphur plasma, from which the bulk of the radiation originates in the S2 B3 Σ u− → X3 Σ g− molecular transition. The radiative transfer calculation needs as input the local spectral emission and absorption coefficients of the transitions. Calculations are presented using both a quantum-mechanical (QM) and a semiclassical (SC) method for generating these coefficients. It is found that the fine structure of QM coefficients, which is absent in the smooth SC data, may have a profound influence on the transport calculation. The circumstances where this occurs are identified and discussed. Measured spectra of the sulphur lamp are presented and compared with calculations, and a number of differences are found which may be due to an incorrectly modelled temperature profile or non-local thermal equilibrium (LTE) effects." @default.
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- W2078643496 date "2002-08-21" @default.
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- W2078643496 title "Radiative transfer of a molecular S2B X spectrum using semiclassical and quantum-mechanical radiation coefficients" @default.
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- W2078643496 doi "https://doi.org/10.1088/0953-4075/35/17/302" @default.
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