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20010418/9 report

Empirical correction tested again - changes continue


Grade 5 weather (tau_cso > 0.25, but seeing tolerable) was used to check the empirical correction (installed on 20010314). The map16 method was used with Mars as the source, with the empirical correction enabled :

  • from (az,el) = (144,37) at HST 02:13 to (216,37) at 06:41.
  • transit occurred at HST 04:27 at an elevation of 47 degrees.
  • data was taken beyond azimuth 216 but the analysis failed after 391 of the 420 data had been processed : messages about temporary space problems. The data loss is tolerable however.
The seeing was reported by Ed as beeing between 0.4" and 0.7" : the value reported by mapsum was a static 0.298, which is unbelievable.

The pointing residuals are displayed below :

The azimuth performance is reasonable, with an rms scatter of 1.0" being not much more than the average seeing. The elevation residuals show a 5" excursion between azimuths 178 and 194, centred at about azimuth 186. This is an intolerable error and must cause concern for all data taken around transit in the last month.

The data were corrected for the extant empirical correction (of 14 March). The plot below shows how the data would look if taken with the empirical correction disabled :

The plot maybe only shows that the empirical correction needs redefining. A repeat of this run with the empirical correction disabled will be requested tonight.

Two theories (by Dean Shutt) pertain as to the root cause of this error :

  1. Elevation imbalance - the theory being that slight errors in the balancing of the antenna cause hysteretical response in the friction drives. The theory holds that the amplitude of the hysteresis should be proportional to the imbalance.
  2. Elevation encoder collar slippage - the encoder is connected via a collar to the elevation axis. The bolt connections need only allow one micron of slop to produce the amplitude effect seen in these tracking data.
Testing the first is easiest : weights (of order 100kg ?) can be added or removed from the antenna. The second requires a tightening of bolts, some of which are inaccessible without complete removal, and replacement, of the encoder. In each case the acid test is repeating the tracking experiment. This was scheduled for the E&C time during first shifts mid-June, but I feel I must recommend moving these activities forwards : the current behaviour of the telescope is too poorly controlled to provide reliable results in the azimuth range 175 - 190 (and presumably at corresponding azimuths around transit in the north).

19th April 2001

The map16 method was applied to Mars again - this time with the empirical correction disabled :

  • from (az,el) = (153,42) at HST 02:45 to (221,34) at 06:39.
  • transit occurred at HST 04:19 at an elevation of 47 degrees.
The seeing was about 0.6", tau_cso ~ 0.10. The pointing residuals are displayed below :

The azimuth residuals have a raw rms scatter of 1.3", which is significantly larger than the seeing, but which is due almost entirely to its steady change throughout the period : a straight line fit to the data shows a slope of 0.05"/degree, with a rms about the line of 0.75". This behaviour may need addressing, but it is beyond the scope of the current issue.

The elevation residuals show much evolution over the previous measures on 14 March :

  • the overall level change is now 10" cf 7"
  • the width of the effect may now reach from azimuth 160 to 210
  • the midpoint is becoming harder to establish, but is well fit by az=190 (see the fit below) - again, up from the 185 of last time.
But the big surprise is the spike at azimuth 185 - a new feature (even as compared to yesterday's results), which, combined with the changes listed above, reflect a significant qualitative, as well as quantitative, change in the transit behaviour.

The necessity for action could not be clearer, and it is fortunate perhaps that we had planned, yesterday, to take immediate remedial action.

New empirical correction installed

The plot below shows the above data with a new empirical correction S-curve superimposed in green.

The elevation residuals corrected by the new curve are also shown in green. They amount to no more than a second or two outside the azimuth range 180-190. This new empirical correction (the S-curve shown above) was installed at 15:40 HST 19 April. The validity of this curve may be shortlived given the engineering scheduled for 19 April. Observers are encouraged to avoid these azimuths and to perform regular local pointing whenever possible.

Because of the proximity of SPIFI to the elevation encoder a reduced plan of maintenance is to be performed today (19 April):



Date: Thu, 19 Apr 2001 09:20:40 -1000
From: Dean Shutt 
Subject: Details of today's elevation encoder work

Confirming our discussion of this morning:

We will not remove the elevation encoder today.  There simply is not
enough room to do this properly with SPIFI in place.  However, Vernon
and Tomas are enroute to the summit to perform the following work:

   1.  Tighten the eight bolts holding one side of the encoder coupling. 
       These can be accessed through the hole in the elevation bearing.

   2.  Tighten the encoder anti-rotatation pin.  The encoder is held in
       place circumferentially by a spring loaded bolt which bears on a
       plate. Should this device be slightly loose, or the spring broken
       or crushed, the encoder would have a slight circumferential play.

       Note that at the diameter of the encoder only approx. 1 micron of
       circumferential play is required to cause a 1 arc second change in
       elevation on the sky.  

   3.  Inspect the coarse encoder gear and elevation overspeed sensor for
       freedom.  Abnormal friction in this area would also contribute to
       the observed effect.

Having accomplished the above, we will have addressed all the likely
problems in this area excepting the bolts on the blind side of the
encoder flange.  Tightening of these requires removal of the encoder as
originally proposed.

I would ask that the transit tracking test be performed at the most
convenient time between now and Monday morning.  If the S effect has
disappeared or been significantly reduced I suggest we do nothing
further immediately.  We can remove the residual effect in software and
see if the required correction changes over time.  If the testing
reveals the S effect is still large we will remove the encoder assembly
for inspection and tightening of the blind coupling bolts on Monday. If
THAT does not resolve the problem, we will think harder ...

As discussed, the change in shape, amplitude, and zero crossing of the S
correction over time is characteristic of a frictional effect.  For this
reason, and because the measured changes in response bear no
relationship to known elevation balance changes, I do not believe we
should pursue the "unbalance windup" theory until after completion of
the above work.

Dean


14:00 HST : Vernon reports visual inspection completed, no obvious motion of bolts during attempts to tighten them, but that the encoder anti-rotation rods were tightened (item 2 above).


19 April 2001

An elevation encoder zero-point change of 133" resulted from the engineering today. After the pointing model was updated accordingly, a further transit tracking test was performed on 3c279, with the empirical correction disabled, as follows :

The seeing was about 0.5", tau_cso ~ 0.05. The pointing residuals (daz in white, del in red) are displayed below :

The green line is the fit determined form the Mars data earlier in the day, and the green dots are the residuals of the new data about the green line. The performance is essentially indistinguishable from that before the engineering. Even the excursions in both daz & del at azimuth 215 are similar to those seen in the earlier data : although of secondary concern they suggest that more extensive runs will be necessary to fully characterise the tracking behaviour.

20 April 2001

The elevation encoder is scheduled to be removed and replaced with a spare on Monday 23 April, with afternoon/evening checks on the zero-point and transit tracking characteristics.


Iain Coulson
Latest Update : 20 Apr 2001
Contact: Iain Coulson. Updated: Sat Nov 6 18:00:23 HST 2004

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