视差的

The parallactic refraction between the stars and the satellite is small and well determinate, except for the irregular stellar movements known as erratics.

除了通称为不规律星体运之外，恒星和卫星之间视差折光差微小，而且是容易测定。

Using this method, isopachic fractional fringe orders can be measured with compensator, and the parallax and drift of fringe pattern can be eliminated.

用这个方法，可通过补偿测定等和线分数条纹，可消除条纹图案视差和浮，全息底板可用白光照再现干涉应力图像。