rs,简写为ERP)通常是指极移(Polar Motion)和日长变化(Length of Day,简写为LOD),它与岁差、章动一起构成地球定向参数(Earthorientation parameters,简写为Eop),是实现...
基于2862个网页-相关网页
International Polar Motion Service 国际极移服务
secular polar motion [天] 长期极移 ; 长年极移
polar motion service 极移服务
Annual polar motion 周年极移
IERS polar motion data IERS极移数据
But the amplitude of is only a half of that of z . Therefore it is shown that the atmosphere is the main excitation of polar motion in high frequency.
分析结果表明大气可能是极移短周期变化的主要激发源。
参考来源 - 地极运动的统计特性及其和大气的激发比较·2,447,543篇论文数据,部分数据来源于NoteExpress
以上来源于: WordNet
Polar motion is the movement of the rotation axis with respect to the crust.
极移指自转轴相对地壳的运动。
The rotation of the Earth includes precession, nutation, variations of the rotation rate and polar motion.
地球自转运动包括岁差和章动,极移和日长的变化。
Therefore, observation and research of the polar motion can provide information about global geophysical processes.
因而,对极移的观测和研究必然为全球性的地球物理现象提供着信息。
应用推荐