IFLO compression by the FAA 1350/1330 Mhz radar using lbw,lbn
29apr03
PLOTS:
lband
wide circular polarization.
lband
wide linear polarization.
lband
narrow circular polarization.
The compression of iflo/ lband receivers (lband
wide , lband narrow) was measured on 29apr03. The setup was:
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Center a band at 1415 Mhz and pass it through a 5 Mhz IF filter (centered
at 260 MHz). Square law detect the signal with a 2 usec time constant.
Sample the signal at 1 Mhz. Do this for pol A and polB. When this band
goes negative during a radar pulse, you have compression.
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Center another band at 1350,1330 Mhz. Put in a large amount of attenuation
(downstairs) so that the radar at it's peak does not go off scale on the
a/d. Do this for polA and B
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Setup the ri to sample these signals simultaneously with 12 bits, 1 usec
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To decrease the i/o rate, set the radar blanker to a 100 usec window about
the radar pulse. Use this as the ipp (trigger pulse) for the ri. Take 95
1 usec samples every ipp within this window.
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The azimuth was at 203 and the dome was at 9.5 degrees. (see az,za
dependence of the radars for an idea of how much stronger it could
get).
Three set of measurements were done
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lband wide circular polarization, (hybrid in).
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lband wide linear polarization, (hybrid out).
-
lband narrow.
The power levels were adjusted to have -40 dbm upstairs
and -52 dbm downstairs (these were the values on the power meters, the
actual values are 20 db more do to the coupler). With -52 dbm downstairs,
the fiber optics can not provide enough power to saturate the downstairs
iflo (see power
levels in the downstairs iflo). So any saturation must be occurring
upstairs.
Data was taken for 100 seconds. There were 8+ complete
rotations of the radar in this time (12 second rotation period). The 1415
Mhz samples were normalized to (sample/median(power) - 1) where the
median power was compute over the 100 seconds.
The 1350 Mhz data was searched for the peaks when
the radar was pointing at the observatory. These ipps (the 95 samples)
were then plotted. The 1350 data was normalized to full scale while the
1415 Mhz data was normalized to medianTsys -1 (so the radar 1350 scale
and the 1415 Mhz scale are not the same). Each data set has two pages:
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Fig 1.. Plots the 1350 data (smooth lines) and 1415 Mhz data (histogram
mode) for the peak ipps. Offsets have been added for plotting. When the
1415 Mhz data dips down during the positive swing of the radar, the system
is saturated.
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Fig 2. plots the 1350 Mhz data (dashed line) and the 1415 Mhz data
with no offsets. You can read the value of the compression (the negative
going lines) from here. When it reaches -1, the signal level in the 1415
Mhz band has gone to 0. -.5 would be 50% or 3 db compression.
The compression went to about 80% (-7 db) with polA a little
worse than polB.
The compression went to about 80% (-7 db) with polA a
little worse than polB
The compression went to about 80% (-7 db) with polA a
little worse than polB. One ipp (the dark red) had a large 1350 value
and small 1415 value for the entire 95 usecs.
Except for the one ipp of lbn, all of the compression recovered within
the pulse duration (5 usecs). You can see the double bumps in the
faa radar (this is the 1350 then 1330 pulses spaced by 6 usecs). The compression
actually starts to recover during the 1 usec between the 1350 and
1330 pulses.
Conclusions:
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The IFLO (connected to either lband system) is being driven into saturation
by the 1330,1350 faa radar pulses when they point at the observatory (once
every 12 seconds). The compression goes to 80% (-7 db). It is important
to realize that it is the IFLO (first mixer stage) and not the dewar/postamp
package that is being driven into saturation. The mixer chassis has about
40 db of gain and its amplifiers have the same dynamic range as those that
precede it in the postamps of the lband receivers.
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The system recovers rapidly from the compression (within the 2 usecs of
our time constant)
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There was one unexplained ipp (95 usecs) when the radar was high all the
time and the 1415 Mhz was low. It did not repeat.
processing: x101/030429/dofaa.pro
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