[evlatests] Phased VLA fringes!
Vivek Dhawan
vdhawan at nrao.edu
Tue Apr 9 11:22:55 EDT 2013
Thanks to Walter, and "real time" DIFX, (2 hours/GByte transfer), the VLA
clock was found at +1704 usec on April 5th. Backtracking to projects in
March, Paul Dyer has in short order found all the missing fringes.
expt Date usec. BW
ty028a Apr 05 1704 1 MHz
bb321N Mar14 1667 128
bb321L Mar13 1667 128
bk178c Mar01 1670 16
The offsets may depend more on bandwidth (we have seen this before)
than on time elapsed since March 01. No offset is seen in the monitor
point (VLA_GPS to clock) in the master LO.
The ~2msec offset is not apparent on the VLA internally, but now we
must find out how and why it happens. It may also be that the regular
VLA data is fine, but the VDIF stream has slipped relative to it.
I don't know if that is even a legal thought.
Tests must be devised, anyone have ideas?
I will set up another real-time session soon.
Relatively less significant mysteries remain:
The 4 subbands have (sometimes) different delays and amplitudes,
especially on bk178 (centaurus A) but that I am attributing to the
channels being badly phased. Chan 1 is sometimes lower amplitude.
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