Turbulence, superrotation, and general circulation models of the atmosphere of Venus

被引：1
|
作者：
Izakov, M. N. [1 ]
机构：
[1] Russian Acad Sci, Space Res Inst, Moscow 117997, Russia
来源：
SOLAR SYSTEM RESEARCH | 2016年 / 50卷 / 05期
关键词：
planets; atmosphere; turbulence; anomalous convection; EXPRESS MONITORING CAMERA; MERIDIONAL CIRCULATION; QUASI-2-DIMENSIONAL TURBULENCE; 2-DIMENSIONAL TURBULENCE; GLOBAL CIRCULATION; CLOUD LEVEL; MORPHOLOGY; WAVES; MESOSPHERE; RADIATION;
D O I：
10.1134/S0038094616040031
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The data obtained in space-borne measurements and the findings of turbulence theory show that turbulence, of both small and large scales, has a decisive influence on the structure and dynamics of the atmosphere of Venus. The small-scale turbulence generates anomalous convection, while large-scale turbulence induces the return spectral flux of energy that is the main element of the superrotation mechanism in the atmosphere. Ways for improving the general circulation model of the atmosphere of Venus are proposed.
引用
收藏
页码：301 / 315
页数：15
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