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Correlation & Logistics
We operate the correlator 80 hours per week, from which time
system testing and development must also come. Our basic unit of
correlation is usually a tape pass. Our control software is best suited
to continuous tape motion; reasonably short gaps in the schedule are
``waited out" in real time. Preparation for a pass, assuming the tapes
are pre-positioned to approximately the correct footage, is
9 minutes
(for thin tape, passes are typically either 22 or 44 minutes).
This preparation time includes:

- calculations: parsing the VEX file, selecting stations/scans
to include, and computing the a priori model.

- tape manipulation: going to a priori footage,
positioning the heads transversely
such that they read tracks with
an expected time-on-tape (i.e.,
one within the bounds of the requested scans), positioning the tape
longitudinally such that the time-on-tape corresponds to the initial scan time,
and waiting until the slowest
tape is ready.
When correlation of the
experiment is finished we review the output, looking for any necessary
recorrelations that weren't caught in the course of the original correlation.
The shift to thin-tape-only operation has improved
playback quality; this together with the excision of TRM byte slips has
markedly reduced the amount of passes requiring recorrelation.
Once all recorrelations are exhausted, we
make a variety of information available to the PI (as described in
§3.3),
and arrange for shipment of the resulting FITS data.
Unless contacted by the PI to the contrary,
we aim to release an experiment's tapes four weeks
after the PI is notified of the experiment's completion, in order to ensure the supply
of tapes in the pool remains replenished for future observations -- which
is of increased importance now that the EVN has moved to thin-tape-only
operation.
Besides the review products mentioned below, the PI of course may also
discuss the experiment/correlation with the
responsible JIVE support scientist and/or
arrange for visiting
JIVE for help in data reduction if desired. Specific programs exist to
provide financial support for European
PIs from non-EVN institutes and their collaborators to encourage visits
to EVN institutes, including JIVE -- see the EVN web page under the ``Access
to the EVN" menu item.
Next: Post-correlation Data Review
Up: Operational Overview
Previous: Pre-correlation
Bob Campbell
2003-09-22