首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Compressible f-plane solutions to body forces, heatings, and coolings, and application to the primary and secondary gravity waves generated by a deep convective plume
【24h】

Compressible f-plane solutions to body forces, heatings, and coolings, and application to the primary and secondary gravity waves generated by a deep convective plume

机译:可压缩f-plane解决身体力量,加热和冷却,和应用程序的中小学所产生的重力波深对流柱

获取原文
获取原文并翻译 | 示例
           

摘要

We derive the analytic, linear, f-plane compressible solutions to local, interval, 3-D horizontal and vertical body forces, and heat/coolings in an isothermal, unsheared, and nondissipative atmosphere. These force/heat/coolings oscillate at the frequency, and turn on and off smoothly over a finite interval in time. The solutions include a mean response, gravity waves (GWs), and acoustic waves (AWs). The excited waves span a large range of horizontal/vertical scales and frequencies ω. We find that the compressible solutions are important for GWs with vertical wavelengths |λz|>(1to2)×πH if the depth of the force/heat/cooling is greater than the density scale height H. We calculate the primary GWs excited by a deep convective plume, ray trace them into the thermosphere, and calculate the body force/heat/coolings which result where the GWs dissipate. We find that the force/heat/cooling amplitudes are up to ~40% smaller using the compressible (as compared to the Boussinesq) GW spectra. For a typical plume, the force/heat/coolings are deeper than H and have maximum amplitudes of ~0.2 to 0.6 m/s2and ~0.06 to 0.15 K/s for solar maximum to minimum, respectively. The heat/cooling consists of dipoles at z~150-200 km and a heating at z~240-260 km. We find that the compressible solutions are necessary for calculating the secondary GWs excited by these thermospheric force/heat/coolings.
机译:我们推导出分析,线性,f-plane三维可压缩解决本地、间隔水平和垂直的身体力量,在一个等温加热/冷却,未修剪的,nondissipative气氛。力/热/冷振荡频率,,在一个有限的顺利打开或关闭间隔时间。反应,重力波(千瓦),和声波(AWs)。水平/垂直尺度和频率ω。发现可压缩解决方案重要的空间与垂直波长z | |λ>(1拽)×πH的深度力/热/冷比密度大规模高度h .我们计算主千瓦兴奋的深对流烟柱,射线跟踪热大气层,和计算体力/加热/冷却这结果千瓦消散。力/热/冷振幅~ 40%使用可压缩(相比较小布西涅斯克)GW光谱。力/热/冷比H和深入最大振幅的~ 0.2至0.6米/ s2and~ 0.06到0.15 K / s对太阳能最大到最小,分别。偶极子在z ~ 150 - 200公里,加热z ~ 240 - 260公里。解决方案是必要的计算由这些thermospheric次要空间的兴奋力/热/冷。

著录项

获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号