From: <brett.reid_at_email.protected>
Date: Thu, 04 Oct 2007 18:19:41 +1100

 ('binary' encoding is not supported, stored as-is)
Hi Simon and all,
==============Original message text===============
On Thu, 04 Oct 2007 10:23:02 +1100 Simon Ellingsen wrote:

Hi Tasso,
..............
In terms of action item #7, I think that we already do this at Hobart
as part of standard IVS operations there is hourly monitoring of the
maser - Brett? For Ceduna its only done during VLBI experiments and
we'll have to put something in place. I would suggest that we need a
further action item here - Setup mechanism for storing the clock
monitoring data from all antennas at a centralised location. Since
there is limited point in expending effort to collect the data if its
stored in 3-4 different locations, formats etc.
.................
Regards

Simon
===========End of original message text===========

Just in relation to maser monitoring at Hobart and Ceduna.
The TAC32 software is set up to take averaged tick phases for Hobart and
Ceduna and store this once per minute. The files are kept locally. Jamie
Stevens has taken this data and automated transfer of some of it as
required to web pages etc. Warwick Wilson looks at this data for Ceduna
and Irv Diegel (Honeywell) looks at it for Hobart. In fact Irv gets all
the Hobart tick phases ftp'd to Honeywell. Jamie is experienced at
shifting these files.

Chris may have answered some of this already in his subsequent reply.

Regards,
Brett

Brett Reid
Observatory Manager, Radio Telescopes
University of Tasmania
School of Mathematics and Physics
phone + 61 3 6248 5285
email brett.reid_at_utas.<!--nospam-->edu.au
web http://www-ra.phys.utas.edu.au/~breid/
Received on 2007-10-04 17:20:07