[evla-sw-discuss] System design decisions needed for Widar
Barry Clark
bclark at nrao.edu
Tue Sep 22 11:33:13 EDT 2009
Dave Harlan points out another decision that needs to be made and
documented - When is the configuration information sent to Widar.
Should it be sent only when it changes, or every scan on general
principles.
Barry Clark wrote:
> There are several issues to be decided about what we want the system
> to look like in the long and intermediate term so we know what
> general direction to take in the short run.
>
> 1. Flags from the telescopes.
> The long term route is clear - they should be collected by MCAF
> and inserted into the SDM. There are problems with doing this
> in the short term because of a breakdown in the colaboration
> with ALMA.
> Alternatives in the short term are
> A. Have MCAF put the flags in a temporary flag table in the SDM
> which may or may not morph into the final flag table when ALMA
> is interested in talking about it. Table would be handled by
> the CASA filler in 'transparent mode', and a special CASA program
> written to run after the filler to compute the flags and put them
> in the measurement set.
> B. Writing a separate flag handling program to bundle them up, label
> them appropriately, and ship them off to the CBE to apply as
> baseline based flags. (Suffers the disadvantage of creating a new
> data route that will be abandoned in the long run.)
>
> 2. Setting the filter requantizer gains
> Alternatives are
> A. Continuous ALC. I would strongly recommend that the ALC loop be
> based on an integration boxcar synchronous and conterminous with
> integrations. Anything else is just too hard to keep track of.
> Then the station board product is the requantizer gain, which must
> be recorded every integration to be able to tie things together.
> B. ALC for each scan. (My favorite.) This is the way the attenuators
> in the T304s are set. In this case, the output of the station
> board is the requantizer gain once per scan (used for bandpass
> stitching), and the requantizer power. This option raises the
> question of by what route the station board is notified that a
> new scan is occurring.
> C. Set gains to a standard value. Then the output of the station board
> is the requantizer power, used for converting to correlation
> coefficients. This runs into trouble when subbands have very different
> power levels.
> In any of these cases we probably need a program to collect the outputs
> from the station boards, package them up and send somewhere useful. The
> 'somewhere useful' probably includes MCAF to include in the SDM. Even if
> we decide that these data products are to be used in the CBE, rather than
> CASA, they probably need to be included in the SDM to provide a record of
> what was done.
>
> At a guess, we'll end up doing all three options above. C is what we
> have now and is therefore the default, B produces the easiest data to
> process, so we are likely to want to do it for now, and A may be insisted
> upon by a solar observer if we ever have one.
>
> 3. System/Noise source application.
> I believe it is generally agreed that the ratio of system to cal be
> included in the SDM for application during post processing. This
> probably implies a listener within the correlator system to collect
> these, package them, and export to MCAF. Again, I strongly urge that
> these be collected and recorded once per integration.
>
> 4. Are correlation coefficients useful?
> From a sufficiently high level abstract viewpoint, the answer is no.
> Calibration is done by dividing each subband by the subband gain, and
> then multiplying that whole combined spectrum by a number that converts
> it to Janskys. This number is derived by looking at the "best"
> subband (least interference, best known cal) and dividing by the
> measured cal power (that is, cal on minus cal off), and multiplying
> by the Tcal for that subband. This converts the measure correlations
> into kelvin. One then multiplies by the antenna effective area which
> converts them into Janskys. (but see footnote) The power level out
> of the requantizer nowhere enters in this description of calibration.
> On the other hand, for various intermediate operations, particularly
> in telcal, having correlation coefficients, derived by dividing the
> measured correlations by the power out of the requantizer, really
> simplifies things by not having to worry about changes in power level
> across the time of its calculations.
> If we decide correlation coefficients are useful, it raises the question
> of when they are calculated - in the CBE or later in the stream. (If
> this division is done in the CBE, we will have to have the power of
> undoing it later, since, as noted above, correlation coefficients are
> not used in the calibration process.)
>
> 5. Delay residuals.
> The see-sawing of phase across the band due to the delay cogging is
> alleged to be a problem, and it probably is at some very high dynamic
> range, and becomes a nuisance in more ordinary observations. We
> should plan to correct it, although it is not clear to me that there
> is a very high current priority on correcting it. I can see two
> ways of making the correction.
> A. Make available the delay polynomials used at observe time, and
> replicate the calculations done on the station board to estimate
> the mean phase slope residuals during the integration to calculate
> the correction. The delay polynomials may be captured from the
> Executor multicast or relayed from the station board, or from the
> polynomial distributor.
> B. The station board may be taxed with the job of producing the average
> and RMS delay error over the integration, and this can be provided as
> one of the station board products. A rough calculation indicates that
> correcting the delay by the mean error and the amplitude by the RMS
> error should be sufficient even for quite high dynamic ranges.
> In either case, the correction may be done in the CBE, or later, in CASA,
> determining whether the data stream is sent to the CBE or to the SDM.
>
> 6. Tcal.
> We probably, in the long run, need cal spectra. If we decide we do,
> probably the most reasonable place to store them is in a new table
> in the evlaparm database. We might need a receiver serial number
> in the main parameters table to simplify the situation if a receiver
> is removed from one antenna and installed in another, though it would
> not be too complicated to keep track of this by hand. The question
> that arises is who reads the table - Executor or MCAF. (One might
> also palm this off on Scheduler.) If the Executor, when should it
> be read - every scan? However, as noted above, we really need a Tcal
> only for one subband for each sampler. If we get properly organized,
> we can probably live with the existing system for a long time.
>
> 7. Scans and subscans.
> The CBE must know about scans and subscans, obviously. It is currently
> told about them directly by the Executor. Is this intended to be the
> final route, or is this a temporary expedient? If permanent, we need
> to know the information to be added to let the CBE sort out the multiple
> subarray case. Also, as mentioned above, it is perhaps expedient to be
> able to tell subband filters "This is a new scan - set your output power
> level to something sensible." This clearly has to go through the VCI
> interface - any problems with that? We need to decide the message content.
> In particular, we would rather like to send a single message, and have
> the ConfigurationMapper keep track of what station boards to forward
> it to.
> (also see footnote 2)
>
> 8. How does correlator configuration information get from the OPT to
> the correlator?
> The plan is for the scheduler to produce an Executor script and
> correlator configuration documents. I can see two ways for the
> documents to get to the correlator.
> A. The scheduler may write files containing the documents and insert
> the file names in the script. The Executor would then send the
> document to the VCI as needed, either through a socket or by passing
> a file name, as the current human interface to the ConfigurationMapper
> does.
> B. The scheduler creates a queue of correlator configuration times,
> and delayed processes that wake up and send configurations to the
> VCI at the appropriate times.
> It seems to me that A is the best way to do this. Among several other
> reasons, it trivially permits human edited scripts, which would be a
> bear via route B.
>
> 9. How does configuration information get from the OPT to the CBE?
> This is the ConfigurationMapper, whether one chooses to call it that
> or not. If you choose to write it as a separate entity, you will
> have to worry a lot about communication protocols between the two
> pieces. From an ethereal plane, one might simply recommend
> combining ConfigurationMapper and the CBE master. Even on a less
> ethereal plane, it would seem to me better to make it as much as
> possible one piece, so that things currently only in the CBE
> master get put in ConfigurationMapper, like a list of available nics
> and ports would be kept in the ConfigurationMapper. Then the
> ConfigurationMapper can organize sending the addresses to the
> baseline boards. It will also have to pass along to the CBE slave
> processes what it has done, and what processing they need to do.
> (Note: here I am interfering in an area I know nothing about, so
> the content may be inane, but something needs to be decided and
> written down.)
>
> Footnote 1. Instead of simply the switched power, sending along
> (Pon - Poff)/(Pon + Poff)*(Requantizer_Power)/Requantizer_Gain
> cancels a few mildly annoying fiddly corrections.
>
> Footnote 2. Despite the fact that scan_number, subscan_number are
> hermetic within the BDF/SDM system and do not leak out, Rich and
> Martin have been urging to have the Executor provide them, on the
> grounds that associating data via an integer is nicer than via the
> floating point time. It is reasonable for the Executor to do this,
> but one would prefer not to unless the current direct communication
> scheme to the CBE is the long term one.
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