查询词典 ecliptic longitude
- 与 ecliptic longitude 相关的网络例句 [注:此内容来源于网络,仅供参考]
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You now have the mean ecliptic longitude of the sun for midday of your chosen day.
你现在有指黄道经度的阳光中午,你选择了每天坐在这一边。
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Now determine the ecliptic longitude of the sun using the following formula.
现在确定黄道经度的太阳,用下列公式。
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Now with your interpolated mean ecliptic longitude of the sun , go back and do the whole calculation again.
利用这段时间,以创造插值因子,现在你插指黄道经度的太阳,回去做整计算。
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The first thing we need to do is determine the mean ecliptic longitude of the sun for your chosen day. Use this table to get a first approximation.
第一件事,我们需要做的是确定的意思,黄道经度的太阳为你的选择每天使用此表,以获得第一次逼近。
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Now we also need to determine the ecliptic longitude of perigee of the sun on this same day. This changes very slowly, thus we need know only the year to compute it with sufficient accuracy.
现在,我们还需要确定黄道经度的近地点的太阳就这同一天,这变化非常缓慢,因此,我们需要知道,只有今年来计算,它有足够的精度。
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You now have the ecliptic longitude of perigee of the sun for the mean summer solstice of your chosen year (and effectively for the entire year).
你现在有黄道经度的近地点的阳光平均夏季冬至,你选择了一年。
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VSOP87 Functions used to Compute Planeta - These functions are a VB version of the complete VSOP87 planetary theory designed to be used to in a program to compute the heliocentric ecliptic longitude, latitude and distance of the planets Mercury to Neptune over a period of several thousands of years to about 1 arcsecond of precision.
这些函数是一个VB版本的完整VSOP87行星理论,旨在一个程序中用来计算以太阳为中心的黄道的经度,纬度,以及Mercury到Neptune行星的距离(从数千年到大约1arc秒精度的周期内)。
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Synodic month 朔望月 The time taken for the moon to reappear at the same ecliptic longitude of the Sun as seen from Earth, which averages 29.53 days.
月球连续两次到达与太阳相同黄经的时间。一个朔望月平均有 29.53 日。
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Based on this, the characteristics of related celestial body positions at the occurrence time of the triggered earthquakes are studied. The distribution patterns, which have tidal_triggering physical basis, of lunar_solar ecliptic longitude differences and declinations and zenith distances are obtained.
在此基础上,对受到潮汐应力触发的地震发震时的天体位置特征进行了研究,得到了具有潮汐应力触发物理基础的地震时的月日黄经差、月日赤纬和月日天顶距的分布图像。
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This is because you used the mean ecliptic longitude of the sun for midday of your chosen day and not the actual time of the event .
现在你可以看到你的时候差别很大,从时代的一个年历,这是因为你用的意思,黄道经度的阳光中午,你选择一天,而不是实际的时候,该事件如果你希望你的计算是完美,你将需要插平均黄道经度的太阳为实际的时候,这项活动。
- 推荐网络例句
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I didn't watch TV last night, because it .
昨晚我没有看电视,因为电视机坏了。
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Since this year, in a lot of villages of Beijing, TV of elevator liquid crystal was removed.
今年以来,在北京的很多小区里,电梯液晶电视被撤了下来。
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I'm running my simile to an extreme.
我比喻得过头了。