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F2 sign convention
F2 sign convention
The reports of
05 April 2003 and
10 April 2003
describe the observed impact on pointing of what appears to be
an incorrect application of the F2 term of the track model.
The TCS error reported in the latter leads
to a table describing the errors
incurred. It is important that the sign convention
for this table be clear. The case of F2 is presented here.
- The tabulated version of the
track model
lists values of (F1,F2,F3) for
certain values of azimuth.
- At a position given by (azimuth,elevation) = (az,el) the value of
F2, viz. f2,az, should cause the azimuth
of the telescope to be adjusted by +f2,az*sin(el)
arcseconds on the sky in addition to the corrections applied using the
terms of the 7-parameter telescope model.
- Hopefully this term makes a correction that counteracts the
irregularities in the track at (az,el) such that a POINTING (or
FIVEPOINT) executed at this position shows the telescope
to be pointing exactly where it ought.
- The erroneous TCS, described here,
used an adjustment of +f2,az*sin(el)*cos(el).
- Thus the telescope position was in error by
delta(az) = +f2,az*sin(el)*(cos(el) - 1)
- This value is the one tabulated.
- Note that a subsequent POINTING/fivepoint would suggest that the
antenna would need moving by
     
- f2,az*sin(el)*(cos(el) - 1)
- . . . and this would be the number recorded in the pointing logs as
daz, and plotted in the various plots throughout this website.
- So, for instance, a SCUBA jiggle-map taken using the erroneous TCS
code, and ostensibly centred at (az,el), was really centred at
(az + delta(az), el), and azimuths extracted from the map should be
corrected by -delta(az) to yield 'true' azimuths.
I hope that's clear.
Iain Coulson
17 Jun 2003
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