Southern polar UW Pic is showing violent oscillations! From periodic monitoring it was clear that UW Pic had reached a stage of elevated brightness, from the usual mag 16-17 to around 15 and below. Snapshot CCD measurements at CBA-Pretoria during 2001-2002 showed this polar at magnitudes in the range 16-17 and sometimes around 15.7. Two recent observations, after the solar conjunction, gave the following magnitudes: UW Pic 20020919.100 (UT) 15.0CR UW Pic 20020924.093 (UT) 14.7CR Timeseries photometry in unfiltered mode, performed during the latter part of last night (Sep 24-25), showed strong oscillations between magnitudes 14.3 and 15.6 with a periodicity of 0.0425d. The photometric measurements were done with a cycle period of 1 minute using the CBA Pretoria set-up of which the observing details follow:. The on-line cv atlas describes UW Pic (Pic1, RX J0531-4624) as an AM Her star with a magnitude range between 16.4V-17.2V and a period of 0.09268 (1994). It can be expected that fast photometry at the 10 sec level (and below) will reveal much more detailed action. Unfortunately this cannot be done at the Bronberg observatory. With my best regards, Berto CCD observations of 19-25 September 2002 observer: Berto Monard MLF, Pretoria, South Africa Bronberg observatory / CBA Pretoria location: -25 º 54' 48", 28º 26' 44"E, altitude 1590m instrumentation: LX200 12" f/4.2 with ST-7E, unfiltered conditions: clear with moon Note: Reported CR magnitudes result from differential photometry to non-red comparison stars with R magnitudes (directly or derived) from published photometric data or traceable to UCAC1 (comparison stars selected from USNO-A2.0 data on the basis of non-red colour and reliability of the data).