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Telescope tracking, e

The tracking accuracy is dependent upon the time resolution of the PDP-encoder interface, which is 100Hz, and the angular speed of a source across the sky. This latter reaches a maximum for a source transiting close to the zenith, and to track accurately through the zenith itself would require infinitely fast computing. A general limit for tracking is currently 85 elevation. Transit here occurs at a rate of about 500 /sec, implying a pointing resolution, in azimuth, of 5 . This falls to 2 at 75 elevation, and to 1 at 65 elevation, or to 1 at 85 elevation and 20 from transit. This ought to define our pointing zone of avoidance, but pointing is done in this region. We do not ascribe errors from this source but note that data from this zone be treated with caution.

The resolution of the track model causes residual errors where the track changes on scales smaller than the resolution. As shown later, 1 resolution models left considerable residuals in this regard, but our newer models have reduced this to perhaps 0.1 rms.



Iain Coulson
Wed Mar 5 11:31:29 HST 1997