2016 IEEE Conference on Electrical Insulation and Dielectric Phenomena (CEIDP) 2016
DOI: 10.1109/ceidp.2016.7785532
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Quantitative visualization of gas temperature distribution in atmospheric DC glow corona by spectral image processing

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Cited by 2 publications
(7 citation statements)
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“…Figure 5 shows the intensity ratio of SPS(0, 2)tail/SPS(0, 2)head as a function of the T g . 26) The spectra of SPS(0, 2)tail and SPS(0, 2)head were acquired, which can be represented by the following approximation:…”
Section: Resultsmentioning
confidence: 99%
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“…Figure 5 shows the intensity ratio of SPS(0, 2)tail/SPS(0, 2)head as a function of the T g . 26) The spectra of SPS(0, 2)tail and SPS(0, 2)head were acquired, which can be represented by the following approximation:…”
Section: Resultsmentioning
confidence: 99%
“…T g of Hermstein's glow corona discharge was acquired from the intensity ratio between the tail and head of the N 2 second positive system band (0, 2) [SPS(0, 2)tail/SPS(0, 2)head]. 25,26) The rotation temperature of N 2 is usually equivalent to the T g under atmospheric conditions. SPS(0, 2)tail/SPS(0, 2)head was calculated for each pixel to acquire the T g distribution of Hermstein's glow corona discharge based on the previously determined relationship between SPS(0, 2)tail/SPS(0, 2)head and T g .…”
Section: Spectral Image Processing Methodsmentioning
confidence: 99%
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