windows::N2 (No. 41)
Links:
| Window ID | Central Freq (cm-1) | Full Width (cm-1) | No. Lines | E" (cm-1) | Altitude Range (km) | Rating | Remarks | |
|---|---|---|---|---|---|---|---|---|
| 0 | 1 | 2395.97 | 0.8 | 1 | 111 | 16 - 38 | 1 | S7 transition |
| 0 | 2 | 2403.57 | 0.8 | 1 | 143 | 16 - 40 | 1 | S8 |
| 0 | 3 | 2411.13 | 0.7 | 1 | 179 | 16 - 35 | 1 | S9 |
| 0 | 4 | 2418.65 | 0.8 | 1 | 219 | 16 - 40 | 1 | S10; interf. by wk N2O line |
Remarks:
- (0) Updated: 11.20.92, lower altitudes adjusted by R. Zander.
- (0) Interferences to worry about mostly are likely to be due to weak N2O lines
References:
- (0) Demoulin, P., et al., , Determination of absolute strengths of N2 quadrupole lines from high resolution ground based infrared solar observations, , J. Geophys. Res., .....
- (0) Rinsland, C.P., et al., The fundamental quadrupole band of 14N2: line positions from high resolution stratospheric solar absorption spectra, J. Molec. Spectrosc., .....