Abstract
In this article we report the most recent advances of our knowledge of non-LTE atmospheric emissions gained from the MIPAS spectra on the Envisat satellite. These include improvements in our knowledge: of the collisional processes between the CO2 (1001), (0221), and (0201) vibrational levels; of the nascent distribution and collisional relaxation of the O3 vibrational states; and of the vibrational-vibrational energy transfer rates between H2O(020) and O2. In addition we report: the first evidence of mesospheric CH4 ν 4 7.6-μm emission; much lower non-LTE populations of the NO 2 (v3 = 1 - 4) in the daytime stratosphere than previously thought; the first experimental confirmation of the non-LTE excitation of NO(1) in the daytime stratosphere; and the first detection of the CO first hot band non-LTE emission near 4.7 μm.
| Original language | English |
|---|---|
| Pages (from-to) | 848-863 |
| Number of pages | 16 |
| Journal | Comptes Rendus Physique |
| Volume | 6 |
| Issue number | 8 |
| DOIs | |
| Publication status | Published - Oct 2005 |
| Externally published | Yes |
Keywords
- CH
- CO
- HO
- MIPAS
- NO
- Non-LTE
- O