[daip] [Fwd: ACCOR output]
lincoln greenhill
greenhill at cfa.harvard.edu
Wed Apr 22 00:23:33 EDT 2009
Thank you Craig. Your detailed recollection is very helpful.
Best,
L.
Craig Walker wrote:
> I looked at the actual power levels in the BBCs for that run and they
> were low, and variable, in channels 5 and 7 (higher frequencies LCP).
> These are the power levels after the autoleveling and should be nearly
> constant. I'm not sure of the reason, but presumably the power coming
> down from the antenna was lower than it should have been. With low
> autoleveled powers, the clipper levels will not be at the right fraction
> of total power and you will see exactly what your plot shows. Hopefully
> the ACCOR corrections will do what is needed to fix things up. There
> will be a small loss of SNR, but I don't think it should be very bad.
> But you might want to avoid using those channels as part of your
> absolute amplitude calibration (ANTUSE in CALIB).
>
> I checked a later run of your project and don't see any sign of the
> problem. I presume whatever the trouble was, it got fixed. The system
> does let the operators know about low power, but it is likely to take
> site tech intervention to fix it and that would generally not be done
> during a run.
>
> Cheers,
>
> Craig
>
>
>
>
> Ingyin Zaw wrote:
>> The expt was in Jan. 2008. Thanks,
>> Ingyin
>>
>> On Tue, 21 Apr 2009, lincoln greenhill wrote:
>>
>>> Dear Leonid, Craig,
>>>
>>>
>>> Attached is a plot showing output from ACCOR (3 VLBA stations, 8 IFs
>>> overplotted) for a 22 GHz phase referencing expt in Nov. 2004.
>>>
>>> We used solint = -0.25 .
>>>
>>> I have not previously see the signature shown here for OV, where 2 of
>>> 8 IFs
>>> show a rapid and systematic variation in sampler statistics. Is the
>>> behavior familiar? Do you know what could cause it?
>>>
>>> Best, L.
>
--
Lincoln J. Greenhill Harvard-Smithsonian Center for Astrophysics
Office: 1 617-495-7194 60 Garden St, Cambridge, MA 02138
Cell: 1 617 851 8918 E-mail: greenhill at cfa.harvard.edu
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