首页> 外文期刊>Geophysical Research Letters >Wind-induced seasonal angular momentum exchange at Titan's surface and its influence on Titan's length-of-day
【24h】

Wind-induced seasonal angular momentum exchange at Titan's surface and its influence on Titan's length-of-day

机译:风在泰坦表面的季节性角动量交换及其对泰坦日长的影响

获取原文
获取原文并翻译 | 示例
           

摘要

Titan's substantial obliquity and the global extent of the Hadley circulation give rise to seasonal variation in the mean zonal wind speed and direction in the geostrophic lower troposphere, causing an exchange of a substantial amount of angular momentum between the surface and atmosphere. The wind-induced seasonal length-of-day variation calculated using the global wind profile predicted by a Titan general circulation model (GCM) amounts to 30 s in the absence of a deep subsurface ocean decoupling the outer ice shell from the ice mantle and similar to 400 s in the presence of a deep subsurface ocean. This effect should give rise to longitudinal offsets of surface landmarks by similar to 10 km and similar to 100 km, respectively, in comparison to predicted positions based on a constant rotation rate, and may be detectable by Cassini imaging.
机译:土卫六的大倾角和哈德利环流的全球范围使对流层低层对流层的平均纬向风速和风向产生季节性变化,从而在地表和大气之间交换了大量角动量。在没有深层地下海洋将外层冰壳与冰幔耦合的情况下,利用泰坦全环流模型(GCM)预测的全球风廓线计算的风致季节日变化量为30 s存在深层地下海洋的情况下持续400 s。与基于恒定旋转速率的预测位置相比,此效果应分别引起表面界标的纵向偏移大约10 km和近似100 km,并且可以通过卡西尼成像检测到。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
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