2014
DOI: 10.1063/1.4863119
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Experimental study on the emission spectra of microwave plasma at atmospheric pressure

Abstract: An experimental study on microwave plasma at atmospheric pressure was conducted by employing optical emission spectroscopy. Based on a microwave plasma generation device developed for nanoparticle synthesis, we studied the influence of input microwave power and gas flow rate on the optical emission behaviors and electron temperature of plasma using Ar, He, and N 2 as working gas, respectively. The physics behind these behaviors was discussed. The results are useful in characterizing microwave plasma at atmosph… Show more

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Cited by 20 publications
(13 citation statements)
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“…The ratio decreases again with distance after its maximum at position 5. As is well known, the intensity ratio ( I 763.7 nm / I 772.7 nm ) can be used to calculate excited electron temperature, which is determined by the electric field . Hence, the intensity ratio is an indicator for the electric field.…”
Section: Resultsmentioning
confidence: 99%
“…The ratio decreases again with distance after its maximum at position 5. As is well known, the intensity ratio ( I 763.7 nm / I 772.7 nm ) can be used to calculate excited electron temperature, which is determined by the electric field . Hence, the intensity ratio is an indicator for the electric field.…”
Section: Resultsmentioning
confidence: 99%
“…Therefore, the intensity ratio of 391.4 to 337.1 nm is an indicator for electron temperature, which is positively proportional to electric field strength. [22,55] Hence, electric field strength can be reflected from an intensity ratio of 391.4 to 337.1 nm. This method has also been reported in Paris et al [49] To implement a precise investigation of the spatial distribution of field strength for D p2 , spectra are captured with a spatial resolution better than 0.1 mm.…”
Section: Resultsmentioning
confidence: 99%
“…As mentioned above, the serpentine trajectory of the streamer presents a peak near an ion cloud and E reaches a minimum in front of an ion cloud. Primarily determined by E, [59,85] T e reaches a minimum once in front of a peak of the snake-like plume. Moreover, as a function of E, the first Townsend ionization coefficient (α) dominates the secondary electron avalanches (electron production process).…”
Section: Methodsmentioning
confidence: 99%