1948
DOI: 10.1016/s1062-2896(49)80088-2
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Temperature measurement on complex flames by sodium line reversal and sodium D line intensity contour studies

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1952
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Cited by 7 publications
(2 citation statements)
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“…One methodology, that of using a line reversal method has also been used to a limited extent. This method relies on the emission of characteristic spectral lines within a flame as observed through a spectroscope [21], to determine the temperature of a complex combustion process, but unfortunately, could only account for the intermediate temperatures within the various zones of the flame. Emission spectroscopy has also been utilized successfully on rocket propellants [22][23][24][25][26] where the high temperature have generally been of a steady or quasi-steady state condition and not of a transitory nature such as proposed in this study.…”
mentioning
confidence: 99%
“…One methodology, that of using a line reversal method has also been used to a limited extent. This method relies on the emission of characteristic spectral lines within a flame as observed through a spectroscope [21], to determine the temperature of a complex combustion process, but unfortunately, could only account for the intermediate temperatures within the various zones of the flame. Emission spectroscopy has also been utilized successfully on rocket propellants [22][23][24][25][26] where the high temperature have generally been of a steady or quasi-steady state condition and not of a transitory nature such as proposed in this study.…”
mentioning
confidence: 99%
“…This pyrométrie reading is taken through the same train of absorption, both atmospheric and instrumental, as caused the reversal of the spectral line, so that the measured brightness temperature of the sun would equal the integrated temperature of the flame along the line through which the solar radiation had passed. 11 Further investigation of this effect might also be of profit for purely astronomical purposes, such as investigation of solar limb…”
mentioning
confidence: 99%