Numerical modeling study of the momentum deposition of small amplitude gravity waves in the thermosphere
Numerical modeling study of the momentum deposition of small amplitude gravity waves in the thermosphere
复制标题
热层小振幅重力波动量沉积的数值模拟研究
DOI:
10.5194/angeo-31-1-2013
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发表时间:
2013-01
期刊:
影响因子:
--
通讯作者:
S. L. Vadas
中科院分区:
文献类型:
--
作者:
刘晓;J. Xu;J. Yue;S. L. Vadas
We study the momentum deposition in the ther- mosphere from the dissipation of small amplitude gravity waves (GWs) within a wave packet using a fully nonlinear two-dimensional compressible numerical model. The model solves the nonlinear propagation and dissipation of a GW packet from the stratosphere into the thermosphere with re- alistic molecular viscosity and thermal diffusivity for various Prandtl numbers. The numerical simulations are performed for GW packets with initial vertical wavelengths ( z) rang- ing from 5 to 50 km. We show that z decreases in time as a GW packet dissipates in the thermosphere, in agreement with the ray trace results of Vadas and Fritts (2005) (VF05). We also find good agreement for the peak height of the mo- mentum flux (zdiss) between our simulations and VF05 for GWs with initial z 2H in an isothermal, windless back- ground, where H is the density scale height. We also confirm that zdiss increases with increasing Prandtl number. We in- clude eddy diffusion in the model, and find that the momen- tum deposition occurs at lower altitudes and has two sep- arate peaks for GW packets with small initial z. We also simulate GW packets in a non-isothermal atmosphere. The net z profile is a competition between its decrease from vis- cosity and its increase from the increasing background tem- perature. We find that the wave packet disperses more in the non-isothermal atmosphere, and causes changes to the mo- mentum flux and z spectra at both early and late times for GW packets with initial z 10 km. These effects are caused by the increase in T in the thermosphere, and the decrease in T near the mesopause.
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