UC知道英语翻译，急急急啦 谢谢万分啦
来源：百度知道 编辑：UC知道 时间：2024/05/27 13:35:40
Figure 3 shows that the aberration-corrected metrics taken from Kingston lay within ±5 arc-s. There are several
outlier cases where the satellite streak is faint, or lies near a star, making endpoint determination difficult. Efforts to
minimize these errors are being undertaken with the automated system. Biases in right ascension and declination
were 0.32 and -0.74 arc-s. Sigmas were 3.0 and 1.9 arc-s in each coordinate. It is welcome to see that the CD shows
biases less than 1 arc-s, suggesting that the CCD shutter timing events are well modeled.
A noted performance limitation of the CD is the relatively high amount of failed astrometry on the GPS images.
There were 181 GPS images recorded, of which only 138 were solved by Pinpoint. This is attributable to the high
degree of telescope pointing error experienced at the Kingston site during the observation session. Once the pointing
error exceeds one half field of view (~11 arc-m) Pinpoint will fa
outlier cases where the satellite streak is faint, or lies near a star, making endpoint determination difficult. Efforts to
minimize these errors are being undertaken with the automated system. Biases in right ascension and declination
were 0.32 and -0.74 arc-s. Sigmas were 3.0 and 1.9 arc-s in each coordinate. It is welcome to see that the CD shows
biases less than 1 arc-s, suggesting that the CCD shutter timing events are well modeled.
A noted performance limitation of the CD is the relatively high amount of failed astrometry on the GPS images.
There were 181 GPS images recorded, of which only 138 were solved by Pinpoint. This is attributable to the high
degree of telescope pointing error experienced at the Kingston site during the observation session. Once the pointing
error exceeds one half field of view (~11 arc-m) Pinpoint will fa
图3中的失常校正数据显示，从金斯敦采取裁员± 5弧š。有几个
异常情况下连胜微弱的卫星，或附近恒星的谎言，使端点决心困难。努力
尽量减少这些错误正在采取的自动化系统。偏差在赤经及赤纬
为0.32和-0.74弧š。 Sigmas分别为3.0和1.9弧在每个坐标S。这实在是可喜地看到，裁谈会显示
偏差小于1弧秒，这表明CCD的快门时间事件都有很好的模型。
阿裁谈会注意到性能的限制，是在GPS图像无法天体金额相对较高。
共有181个全球定位系统的图像记录，其中只有138个是由Pinpoint公司解决。这是由于高
望远镜指向的程度时，在现场观测会议金斯敦经验的错误。一旦指向
误差，超过半数的观点场（〜11弧米）的Pinpoint要失败的天体测量的解决方案。在错误的指向
金斯敦传感器观察到的7弧一些帧并成功地解决分钟高（由于
主要是指这些旧的模型观测）。虽然这可能指向错误是可以接受的
该天体测量软件，它是复杂的程序性错误，其望远镜指向的角度看
没有真正的日期的TOD（）协调，而是元J2000直接输入该系统。此错误增加了约3
弧分的指向误差。最后，怀疑该望远镜镜配合机械弯曲芒特
附件偶尔增加了额外的错误的指向，导致这些数据的总误差超过11
弧米的Pinpoint施加限制。