1984
DOI: 10.1016/0584-8547(84)80115-9
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Diagnostical measurements in a single electrode, atmospheric pressure, microwave plasma

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Cited by 25 publications
(4 citation statements)
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“…A crucial factor limiting both the power of detection and analytical accuracy was the difficulty of introducing a sample in the form of an aerosol or a cold gas flow centrally into the plasma, because the central zones are the hottest. This is clearly shown both by gas temperatures and excitation temperatures as reported by Kirch et al [3], and by the radially resolved measurements acquired by Bings et al [4]. Efforts have been made to improve the introduction of aerosols into the CMP by use of mantle gases, enabling wall stabilization of the plasma, and by introducing the sample aerosols through parallel cylindrical channels in the axial direction near to the electrode tip.…”
Section: Microwave Plasmasmentioning
confidence: 76%
“…A crucial factor limiting both the power of detection and analytical accuracy was the difficulty of introducing a sample in the form of an aerosol or a cold gas flow centrally into the plasma, because the central zones are the hottest. This is clearly shown both by gas temperatures and excitation temperatures as reported by Kirch et al [3], and by the radially resolved measurements acquired by Bings et al [4]. Efforts have been made to improve the introduction of aerosols into the CMP by use of mantle gases, enabling wall stabilization of the plasma, and by introducing the sample aerosols through parallel cylindrical channels in the axial direction near to the electrode tip.…”
Section: Microwave Plasmasmentioning
confidence: 76%
“…At a gas pressure (P g ) of 10 Torr, figures 2 and 3 show the calibrated (see equation ( 6)) emission intensities of H α , H β , H γ and Ar-750.4 nm lines as well as the intensity ratios between these Balmer lines and the Ar line observed as functions of input microwave power. The H atom excitation temperature, T α-β H-exc , calculated from the relative intensities of the H α and H β lines via the following equation [22,23], is also plotted in figure 3. Input microwave power (W) Here, g i is the degeneracy of the state n = i and g 3 = g 3s + g 3p + g 3d = 2 + 6 + 10 = 18, g 4 = g 4s + g 4p + g 4d + g 4f = 32.…”
Section: Variations Of Relative Intensities Between H and Ar Emission...mentioning
confidence: 99%
“…on the measurement of the Stark broadening of an atomic hydrogen line. The » (486.1 nm) line was chosen because it is generally free from plasma spectral interferences, has a sufficient intensity for measurement, and has a small half-width (0.1-0.5 nm) and extensive Stark data are available for this line (31)(32)(33). Both Doppler broadening and instrumental broadening are usually negligible compared to Stark broadening (32).…”
Section: Determination Of Relative Electron (Number) Density Was Basedmentioning
confidence: 99%