[evlatests] Temporal Antenna Gain Changes
Rick Perley
rperley at nrao.edu
Tue Sep 21 13:36:49 EDT 2021
The 24-hour flux density run allows us to check system performance in
many ways. One of these is checking antenna gain stability over time.
The data for this epoch was taken on a day with a large temporal
temperature change -- from about +10C at dawn to +30 in the afternoon.
As is known from past observations, this induces a large gain change in
the antenna signals. The effect varies dramatically with band. The
following table, made from examination of the switched power, shows the
effect. Shown is the maximum gain range observed over the 24 hour
period. Nearly all antennas show the same pattern and ratio.
Band Gain ratio (max/min)
L <1
S 3
C 10
X 8
Ku 20
K 20
Ka 25
Q 20
-----------------------------------------------------
Note that the high frequency bands are much more affected. The working
theory is that the gain changes are due to the temperature sensitivity
of the post-amps, which are mounted directly onto the feed horns, which
are acting as good thermal conductors to the outside temperature.
Attached are two plots showing the effect on the gains at Ku-band. The
first ('TempWind.png') shows the wind and outside temperature during the
24-hour run. The second ('TempGain.png') shows the Ku-band gain over
the same period. (These are *voltage* gains, and a low value means a
higher signal output). Note the lag between the outside temperature
minimum and maximum gain (minimum gain voltage) -- in keeping with the
idea that it's the post-amp temperature change . The scatter in the
voltage gain plots are due to the range in elevations over which the
data were taken (10 to 85 degrees) -- this is an increasingly important
effect at the higher frequencies. The four antennas shown were selected
on the basis of their flat gain curves. (Other antennas, like ea15,
ea18, and ea19 are *much* worse).
The switched power mechanism has been shown (from past runs) to be
highly effective in removing these temperature-induced gain variations.
I have not attempted to use this for these data yet, as the system was
not operating for one of the antennas, and deriving gain curves was one
of the major goals of this experiment.
*R-L Phase Changes*
VLA polarimetric calibration *requires* at least one antenna whose R-L
phase in stable. A change in the R-L phase of the phase reference
antenna is equivalent to rotating the source polarization over time.
Finding the most stable antenna is often quite a chore.
For the K-band data, I've looked at the R-L stability. Using ea28 as
the phase reference, the following two plots show four antennas showing
small changes (clearly looking like a temperature induced instability)
(GoodAnts.png), and four antenna with dramatic changes in the R-L phase
over time (BadAnts.png). Using any of these antennas for the initial
phase reference antenna will dramatically degrade the polarization
calibration accuracy (and the subsequent polarimetric imaging).
No obvious origin for the instability in these four antennas has yet
been identified.
Rick
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