Absolute ground-state nitrogen atom density in a N2/CH4 late afterglow: TALIF experiments and modelling studies
Overview & Synopsis
Following a first study on a late afterglow in flowing pure nitrogen post-discharge, we report new TALIF (Two-photon Absorption Laser-Induced Fluorescence) measurements of the absolute ground-state atomic nitrogen density N(4 S) and investigate the influence of methane introduced downstream from the discharge by varying the CH 4 mixing ratio from 0 up to 50%. The N (4 S) maximum density is about 2.2 x 10 15 cm -3 in pure N 2 for a residence time of 22 ms and does not change significantly for methane mixing ratio up to ∼ 15%, while above, a drastic decrease is observed. The influence of the residence time has been studied. A kinetic model has been developed to determine the elementary processes responsible for the evolution of the N (4 S) density in N 2 /CH 4 late afterglow. This model shows the same decrease as the experimental results even though absolute density values are always larger by about a factor of 3. In the late afterglow three-body recombination dominates the loss of N (4 S) atoms whatever the CH 4 mixing ratio. For high CH 4 mixing ratio, the destruction process through collisions with CH 3, H 2 CN and NH becomes important and is responsible for the observed decrease of the N (4 S) density.
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Document Information
| Document Title | Absolute ground-state nitrogen atom density in a N2/CH4 late afterglow: TALIF experiments and modelling studies |
|---|---|
| Author / Organization | Et Es-Sebbar, M C-Gazeau, Y Benilan, A Jolly, C D Pintassilgo |
| Subject & Discipline | Multidisciplinary Academic Open Research |
| Categories | Science & Mathematics |
| Publication Year | 2010 |
| License / Rights | Open Access / Creative Commons |
| Resource Verification | Listed PDF (Verification Pending) |
| Original Host Website |
HAL Open Science
(hal.science)
|
| File Format | application/pdf (Portable Document Format) |
| Language | EN |
| Catalog ID | DOC-83447 |
| Original Source Link | Visit Source Page on hal.science » |