A bunch of this page isn't filled out, but all of these questions AND MORE are answered on the Internal AO Optics Troubleshooting Page, so seek your answers there!
Trigger a new reconstructor using
MAORI→WFS with both loops closed and check that
reconstructor updates after a few seconds. If not, then restart
the reconstructor from MAORI→Menu. Check the pupil on the
WFS intensity display with the reconstructor mask on and off
(the pupil should look the same).
Check windshake, check tracking errors for El and Az.
Check for possible vibration produced by
the secondary vacuum valve, the telescope drives, etc.
Check
that tip-tilt mirror is powered up.
N.B. if the TT graph shows the mirror position changing, it is
VERY likely powered up.
Check for problem with the tip-tilt mirror (broken actuator?).
Check for problem with the DM using the
WYKO interferometer. Open the WYKO hatch and look at the WYKO
when the DM loop is opened or closed. You should see the DM
move constantly in closed loop. You should also see that it is
not producing strange shapes, such as waffle or a lot of focus.
Check for calibrations: DM to lenslet, COG, SFP home problem,
WLS centering, FSS vignetting, etc.
COG file
If you see poor image quality, you can try
an old COG file (this is quick and
can be done with loops closed)
Current COG
Old COG
In this case, we decided the old COG was better than
the current one. We made the old one the default by
opening a terminal as kNobsao@kNaoserver
cdcog
cp -p 24NIRC2-N2x2.cog31Aug2016
24NIRC2-N2x2.cog
The change takes effect when one next runs Setup
Bench from AOAcq.
Check ACS snap. If you suspect the cals are fine or you see
non-diffraction limited performance, check the snap that
ACS is using (OA's are very helpful here).
Bad AO performance, even for bright star (Vmag10). Artifacts
in the image.
Problem
Bad calibrations or corrupted file for the centroid origins?
Solution
From an xterm on k2aoserver as k2obsao,
type cdcog.
Then dir will list all centroid origins
calibration files sorted by date.
The name reflects the instrument and the date.
For a NIRC2 night in NGS AO mode with the 2.4 arcsec plate
scale and 2x2 binning the default file would be
24NIRC2-N2x2.cog. Find a file with the
same name but a different date appended (e.g.,
24NIRC2-N2x2.cog16Feb2007) that you trust. In this example,
cp -p 24NIRC2-N2x2.cog16Feb2007 24NIRC2-N2x2.cog
In IDL, type LOADCOG,'24NIRC2-N2x2.cog'
The new calibration file should be loaded on the system.
Try other calibration files if necessary or use different
binning modes or plate scale.
The TT mirror and TT residual graph could show a lot of jitter.
Telescope servo-error tracking values could be large.
Problem
Many possible reasons, but the most likely are:
Tip-tilt mirror oscillations.
Problem with TT offloading: could happen when star goes through meridian.
Wind shake: do you see the same effect when you point
into the wind vs other directions?
Lots of vibrations (produced by the secondary-mirror vacuum valve?):
experience has shown it could be worse at lower elevation
Reference star is a binary or has a peculiar morphology:
2-5 arcseconds binary used as a
reference star may produce some elongation. If it is a
close binary (less than 100 mas separattion) then the
image may appear to be elongated.
PyWFS Camera (in the PyWFS status) shows red and says it is
powered off. Clicking on it and rebooting/restarting the camera
server does NOT resolve this.
Problem
Communications between the SAPHIRA and the RTC have been lost.
Solution
Connect to the RTC: ssh -X prtc@prtcserver
Type: showRTProcess. This opens a window, and
the second process from the top is partially crashed
Ctrl-c to restart the process
Connect to the PyWFS server: ssh -X
pwfs@vm-pwfsserver
Issue command: prtcRestartCOM. It kes about 5
sec, then you should be able to reacquire with the camera.