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S2
The S2 system has been developed in Canada to support
the Orbiting VLBI missions VSOP and Radioastron, in addition to ground
based astronomy. It is based on VCR technology and is relatively
inexpensive. It is being used in Australia on the AT and at a number
of other sites around the world.
SCHED supports observations on telescopes that have S2
recorders and are controlled through the Field System (FS9.3.7 or
higher). This is also done by creating a *.skd file in the VEX
format (see section on MkIV).
The telescopes are characterized by RECORDER = S2 and CONTROL = VEX. Currently DAR = VLBA is completely supported
(it could be possible to also implement DAR = MKIV). For any
other DAR SCHED will attempt to schedule the observation with
a ``standard'' S2 mode, not using any knowledge on the content of the
``user signal''.
The modes supported for DAR = VLBA can be derived from a
document ``Compatibility of S2 and VSOPT recordings at S2 and VSOPT
Correlators'' by R. Wietfeldt, available at
ftp::s2.sgl.ists.ca:pub/s2/svlbi/s2vsop_compat_memo_v*.ps.Z.
Because the S2 recorders work in a way conceptually different from
VLBA (or MkIV) recorders, the user should bear the following in mind
when scheduling for S2 recorders.
Please note that no operational tests with SCHED and S2 recorders
have been completed yet, except for VSOP recording. Recently (Dec 2000)
it was discovered that observations that use more than 1 group of
transports (thus not VSOP modes) would not switch groups. This should
have been fixed.
- The S2 recorder internally works with a number of recorders
which each have one head and track. The S2 box uses 1, 2, 4 or 8
recorders depending of the mode. In SCHED this is characterized by
setting TPMODE to the number of groups will be used by the S2
recorder.
- The concept of fan-in or fan-out does not apply to S2 recorders
in SCHED.
- Tape lengths for S2 tapes are specified as the length for
standard US VCR recording in seconds. Thus, when the VCR
cassette has 120 (minutes) on the label the tape lengths is 7200
(ft) in SCHED. European buyers should be careful; a ST-120 tape
presumably is labeled SE-180, but should still be scheduled with
TPLENGTH = 7200. The S2 LP is obtained by using low density for
which the TPSPEEDL = 6.3 (ips) and SLP by using TPSPEEDH
= 4.2 (ips). These speeds are chosen in order to simulate that a
120 minute cassette will last for 7200*12/(6.3*60)=229
minutes, consistent with the S2 documentation. For high
density the same tape lasts for 343 minutes per group (multiply by
TPMODE to get the total time).
- S2 tape motion is supposed to be ``adaptive''. The S2 recorders
should start 2.5 minutes before a scan, stop only 0.1 minutes after
the scan and generally continue to spin if any gaps are shorter than
2.6 minutes. This is the default and only mode of control for S2
recorders through SCHED.
Next: Wide Band VLBA and
Up: Recording Systems.
Previous: NON-VLBA Telescopes with VLBA
Contents
Craig Walker
2006-06-08