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The real telescope : A-frames, SERVO, lumps and bumps

In reality, however, the track is irregular in profile. As the antenna moves over it the 4 supporting wheels will each move up or down, particularly with respect to the other wheel on the same side of the antenna. The two wheels on each side are part of an A-frame, whose apex is one end of the elevation axis. Motion of the wheels thus causes that end of the elevation axis to rock up or down, forward or backward, in the plane of the A-frame. This causes the elevation axis to be moved in the (aero-)nautical directions of roll (the right end of the elevation axis rises w.r.t. the left, or vice versa) and yaw (the right end moves forwards w.r.t. the left, or vice versa).

The top of the A-frame also rotates on an axis perpendicular to the plane of the A-frame, which would cause the elevation axis to pitch if it was fixed to the top of the A-frame. However, the elevation axis is free to rotate within the bearings atop the A-frames, and its orientation is determined using the encoder fixed to the right-hand A-frame. During normal observing the SERVO system is ON, allowing for orientation of the elevation axis w.r.t. the right-hand A-frame. Pitch affects the elevation pointing only.

The track comprises 14 segments, of two sizes (see the notes to Table 1), which have their own peculiar profiles, abut imperfectly, and sit atop a layer of grout whose longevity is questionable. The track profile as a function of azimuth must be described by a look-up table at sufficently high angular resolution. The profile is likely to change with time, either gradually, as the grout crumbles beneath it, or abruptly, following a change in loading, or following an earthquake, for instance. The profile must necessarily be measured in the advent of any such event, and, in any case, on a regular basis.

The track segments were surveyed in 1991 by a crew from the SERC Council of Works unit in Swindon and showed deviations from planes of about + 0.015 inches, with abutment errors typically 0.005 - 0.010 inches. Inclinometry measurements made of the (8-metre long) beams joining the front and back legs of the antenna show corresponding tilts of about + 10" as the antenna moves in azimuth, although there is probably a dynamic interaction between the antenna wheels and the track which prevents a strict correlation between the (static) track profile survey measurements and the inclinometry measurements made at the same azimuths. These effects propagate to errors in the pointing of the telescope of roughly the same magnitude, 10".

The inclinometry project aims to correct the pointing of the JCMT for the effects of the track profile, and, as part of the Pointing Project, to keep pointing errors in azimuth and elevation to 1" r.m.s. ( Pointing Project Meeting No.1, 940201)



next up previous contents
Next: Geometrical and Structural Up: The need for Previous: The ideal telescope



Iain Coulson
Thu Mar 13 14:59:48 HST 1997