耗散大气中风场对内重力波传播的影响  

THE INFLUENCE OF BACKGROUND WINDS ON INTERNAL GRAVITY WAVES IN DISSIPATIVE ATMOSPHERE

作　　者：丁锋[1] 万卫星[1] 袁洪[1] 

机构地区：[1]中国科学院武汉物理与数学研究所,430071

出　　处：《空间科学学报》2000年第2期129-135,共7页Chinese Journal of Space Science

基　　金：国家自然科学基金!49604061;国家杰出青年基金!49525407

摘　　要：使用考虑大气耗散的射线跟踪算法，计算了风场作用下重力波的传播情况．结果表明，风场对快速重力波分量影响较小，但对反射和传播区域的慢速波的影响较大，表现在顺风时使反射区范围缩小，逆风时使反射区范围扩大．在传播区，顺风场使慢速波分量的传播距离变小，传播高度降低，而逆风则使慢速重力波分量的传播距离明显增大，传播高度上升．分析表明，重力波传播的丰富多样性是由风场对波的衰减和反射等滤波作用引起的．By using ray-tracing method, features of propagation of internal gravity wavesunder the influence of winds are calculated- The results indicate that the cut-offregion of gravity waves seems not affected by winds, while reflecting and propagat-ing regions are significantly innuenced. The reflecting region reduces when gravitywaves propagate downwind and expands when against wind. In propagating region,propitions winds shorten the attenuation distance of slow gravity waves and reducetheir propagating height, while converse winds lengthen the attenuation distance ofslow gravity waves and rise the attenuation height. Further analysis shows that thediversity of gravity wave propagation features is caused by the effect of winds onthe processes of gravity wave attenuation and reflection.

关 键 词：射线跟踪 重力波衰减 背景风场 大气重力波传播 

分 类 号：P401[天文地球—大气物理学与大气环境]