Secular variations of OH nightglow emission and of the OH intensity-weighted temperature induced by gravity-wave forcing in the MLT region

被引:17
作者
Huang, Tai-Yin [1 ]
Hickey, Michael [2 ]
机构
[1] Penn State Univ Lehigh Valley, Dept Phys, Fogelsville, PA 18051 USA
[2] Embry Riddle Aeronaut Univ, Coll Arts & Sci, Daytona Beach, FL 32114 USA
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
OH chemistry; gravity wave; airglow; wave packet; secular variation;
D O I
10.1016/j.asr.2007.10.020
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Secular variations of OH airglow (8,3) band and of the intensity-weighted temperature induced by a gravity wave packet at three latitudes in the northern hemisphere in the Mesosphere/Lower Thermosphere region are investigated using a 2-D, time-dependent, fully nonlinear OH chemistry-dynamics model. A net-cycled average survives due to wave transience and dissipation. The integrated OH (8,3) volume emission rates show a 20 percent increase induced by the wave packet. The corresponding intensity-weighted temperature shows an initial increase up to 2 percent then a gradual decrease for the remainder of the simulation time by the same wave packet. These secular variations could be mistaken as long-period or short-period waves in the airglow observations. Therefore, care must be taken when analyzing the data from observations. (C) 2007 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:1477 / 1486
页数:10
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