Abstract
Recent observations of CH4 and HF from the UARS Halogen Limb Occulation Experiment (HALOE) suggest that vigorous descent occurs within the polar winter vortex with "mesospheric' values of CH4 evident down to 30 mbar. This study shows that a highly accurate two-dimensional model advection scheme coupled with a modern radiation scheme, parameterized planetary and gravity wave drag algorithms can produce trace distributions consistent with HALOE observations. The modeled tracer distribution within the polar vortex is found to be principally dependent on the strength of dynamic drag in the middle atmosphere and the strength of the planetary wave forcing. -from Authors
| Original language | English |
|---|---|
| Pages (from-to) | 11,669-11,684 |
| Journal | Journal of Geophysical Research |
| Volume | 100 |
| Issue number | D6 |
| DOIs | |
| State | Published - 1995 |