Weakly or Strongly Nonlinear Mesoscale Dynamics Close to the Tropopause?Source: Journal of the Atmospheric Sciences:;2018:;volume 075:;issue 004::page 1215DOI: 10.1175/JAS-D-17-0063.1Publisher: American Meteorological Society
Abstract: AbstractRecently, it has been discussed whether the mesoscale energy spectra in the upper troposphere and lower stratosphere are generated by weakly or strongly nonlinear dynamics. A necessary condition for weak nonlinearity is that the Rossby number Ro ≡ |?z|/f ? 1, where ?z is the vertical vorticity and f is the Coriolis parameter. First, it is shown that Ro can be estimated by integration of the rotational wavenumber energy spectrum Er. Then divergence and rotational energy spectra and their ratio, R ≡ Ed/Er, are calculated from the Measurement of Ozone and Water Vapor by Airbus In-Service Aircraft (MOZAIC) dataset, and it is shown that at least 1000 flight segments are needed to obtain converged results. It is found that R < 1 in the upper troposphere, ruling out the hypothesis that the spectra are produced by inertia?gravity waves with frequencies larger than f. In the lower stratosphere R is slightly larger than unity. An analysis separating between land and ocean data shows that Ed and temperature spectra have somewhat larger magnitude over land compared to ocean in the upper troposphere?a signature of orographically or convectively forced gravity waves. No such effect is seen in the lower stratosphere. At midlatitudes the Rossby number is on the order of unity and at low latitudes it is larger than unity, indicating that strong nonlinearities are prevalent. Also the temperature spectra, when converted into potential energy spectra, have larger magnitude than predicted by the weakly nonlinear wave hypothesis.
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| contributor author | Li, Qiang | |
| contributor author | Lindborg, Erik | |
| date accessioned | 2019-09-19T10:07:04Z | |
| date available | 2019-09-19T10:07:04Z | |
| date copyright | 2/7/2018 12:00:00 AM | |
| date issued | 2018 | |
| identifier other | jas-d-17-0063.1.pdf | |
| identifier uri | http://yetl.yabesh.ir/yetl1/handle/yetl/4261719 | |
| description abstract | AbstractRecently, it has been discussed whether the mesoscale energy spectra in the upper troposphere and lower stratosphere are generated by weakly or strongly nonlinear dynamics. A necessary condition for weak nonlinearity is that the Rossby number Ro ≡ |?z|/f ? 1, where ?z is the vertical vorticity and f is the Coriolis parameter. First, it is shown that Ro can be estimated by integration of the rotational wavenumber energy spectrum Er. Then divergence and rotational energy spectra and their ratio, R ≡ Ed/Er, are calculated from the Measurement of Ozone and Water Vapor by Airbus In-Service Aircraft (MOZAIC) dataset, and it is shown that at least 1000 flight segments are needed to obtain converged results. It is found that R < 1 in the upper troposphere, ruling out the hypothesis that the spectra are produced by inertia?gravity waves with frequencies larger than f. In the lower stratosphere R is slightly larger than unity. An analysis separating between land and ocean data shows that Ed and temperature spectra have somewhat larger magnitude over land compared to ocean in the upper troposphere?a signature of orographically or convectively forced gravity waves. No such effect is seen in the lower stratosphere. At midlatitudes the Rossby number is on the order of unity and at low latitudes it is larger than unity, indicating that strong nonlinearities are prevalent. Also the temperature spectra, when converted into potential energy spectra, have larger magnitude than predicted by the weakly nonlinear wave hypothesis. | |
| publisher | American Meteorological Society | |
| title | Weakly or Strongly Nonlinear Mesoscale Dynamics Close to the Tropopause? | |
| type | Journal Paper | |
| journal volume | 75 | |
| journal issue | 4 | |
| journal title | Journal of the Atmospheric Sciences | |
| identifier doi | 10.1175/JAS-D-17-0063.1 | |
| journal fristpage | 1215 | |
| journal lastpage | 1229 | |
| tree | Journal of the Atmospheric Sciences:;2018:;volume 075:;issue 004 | |
| contenttype | Fulltext |