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Recording to UTAS V001B.
Using DAS profile vsop.pro.
Start experiment in good weather, and with all five track antenna in the tied array.
Reference antenna is CA01 on W104.
Re-tied at 01:02 UTC
Duriong this 1934-638 scan, from 01:07 to 01:17 phases vary by >100 degrees between ca01,2,3 and ca04,5, before returning to within ~60 degrees of each other. Will drop ca04,5 from tied array if this continues. Seemon path noise is 200~250 microns, but likely to worsen as day goes on.