[evlatests] [vlbatests] Phased VLA fringes!

[Deb Shepherd]

Wonderful news Vivek and Walter!    Thanks!!!!!!!


On Tue, Apr 9, 2013 at 9:22 AM, Vivek Dhawan <vdhawan at nrao.edu> wrote:

> 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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>


-- 
Debra Shepherd <dshepher at nrao.edu>
National Radio Astronomy Observatory
1003 Lopezville Rd
Socorro, New Mexico 87801
http://www.aoc.nrao.edu/~dshepher
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