摘要
The features of the method are as follows: Adopting an optimum average small arc to four-axis prediction,the azimuth and altitude of the tracking axis need not be adjusted during the same observation procedure.The prediction has been used for three different types of telescopes for many years and all demands of users have been satisfied.In this method,the prediction contents were more than others.Separating the unknowns,the actual equations for operation were concise,and the needed machine time was much less,even for the prediction of multistation.
The features of the method are as follows: Adopting an optimum average small arc to four-axis prediction,the azimuth and altitude of the tracking axis need not be adjusted during the same observation procedure.The prediction has been used for three different types of telescopes for many years and all demands of users have been satisfied.In this method,the prediction contents were more than others.Separating the unknowns,the actual equations for operation were concise,and the needed machine time was much less,even for the prediction of multistation.
