2013
DOI: 10.1088/1009-0630/15/9/08
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Diagnosis of Electron, Vibrational and Rotational Temperatures in an Ar/N2Shock Plasma Jet Produced by a Low Pressure DC Cascade Arc Discharge

Abstract: In this paper, a low pressure Ar/N2 shock plasma jet with clearly multicycle alternating zones produced by a DC cascade arc discharge has been investigated by an emission spectral method combined with Abel inversion analysis. Plasma emission intensity, electron, vibrational and rotational temperatures of the shock plasma have been measured in the expansion and compression zones. The results indicate that the ranges of the measured electron temperature, vibrational temperature and rotational temperature are 1.1… Show more

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Cited by 16 publications
(8 citation statements)
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“…Herein, vibrational temperature ( T vib ) is calculated from N 2 (C 3 Π u ‐B 3 Π g ) by the Boltzmann's plot. [ 71,72 ] ln(Iνν/vν'νAν'ν)=CEν'kTvib $\mathrm{ln}({I}_{{{\rm{\nu }}}^{^{\prime} }{{\rm{\nu }}}^{^{\prime\prime} }}/{v}_{{{\rm{\nu }}}^{\text{'}}{{\rm{\nu }}}^{^{\prime\prime} }}{A}_{{{\rm{\nu }}}^{\text{'}}{{\rm{\nu }}}^{^{\prime\prime} }})=C-\frac{{E}_{{{\rm{\nu }}}^{\text{'}}}}{k{T}_{\mathrm{vib}}}$where Iν'ν ${I}_{{{\rm{\nu }}}^{\text{'}}{{\rm{\nu }}}^{^{\prime\prime} }}$ and Aν'ν ${A}_{{{\rm{\nu }}}^{\text{'}}{{\rm{\nu }}}^{^{\prime\prime} }}$ are the emission intensity, and the Einstein spontaneous emission probability for the transition from the upper (quantum number ν ′) to the lower (quantum number ν ″) energy level. E ν′ is the molecular vibration energy, and C is a constant.…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…Herein, vibrational temperature ( T vib ) is calculated from N 2 (C 3 Π u ‐B 3 Π g ) by the Boltzmann's plot. [ 71,72 ] ln(Iνν/vν'νAν'ν)=CEν'kTvib $\mathrm{ln}({I}_{{{\rm{\nu }}}^{^{\prime} }{{\rm{\nu }}}^{^{\prime\prime} }}/{v}_{{{\rm{\nu }}}^{\text{'}}{{\rm{\nu }}}^{^{\prime\prime} }}{A}_{{{\rm{\nu }}}^{\text{'}}{{\rm{\nu }}}^{^{\prime\prime} }})=C-\frac{{E}_{{{\rm{\nu }}}^{\text{'}}}}{k{T}_{\mathrm{vib}}}$where Iν'ν ${I}_{{{\rm{\nu }}}^{\text{'}}{{\rm{\nu }}}^{^{\prime\prime} }}$ and Aν'ν ${A}_{{{\rm{\nu }}}^{\text{'}}{{\rm{\nu }}}^{^{\prime\prime} }}$ are the emission intensity, and the Einstein spontaneous emission probability for the transition from the upper (quantum number ν ′) to the lower (quantum number ν ″) energy level. E ν′ is the molecular vibration energy, and C is a constant.…”
Section: Resultsmentioning
confidence: 99%
“…Herein, vibrational temperature (T vib ) is calculated from N 2 (C 3 Π u -B 3 Π g ) by the Boltzmann's plot. [71,72]…”
Section: Methodsmentioning
confidence: 99%
“…For Ar excited states, they are produced by electron impact, heavy particle impact, and radiative processes [35]. They are in excitation equilibrium and follow the Boltzmann distribution [36]. We use T exc instead of T e to estimate ζ. ζ > 1 represents overpopulation of CH(A), while ζ < 1 represents the opposite.…”
Section: Discussionmentioning
confidence: 99%
“…In our work, OES is utilized to determine the electron excitation temperature. The electron excitation temperature (T exc ) can be determined by the Boltzmann-plot method, which employs the relative intensity of two or more spectral lines using the following equation [21]:…”
Section: Theory Of Oesmentioning
confidence: 99%