We start recording the IM for the Yellow pupil @ 150Hz.
REC: 100modesOK
Then we close the loop at 1kHz.
TN |
Notes |
20140510_202224 |
new Snapshot procedure, closed loop with 100 modes |
20140510_202306 |
" |
20140510_202355 |
old Snapshot, closed loop on 100 modes, gain 0.1 |
20140510_202424 |
" |
20140510_202941 |
new SN, open loop |
20140510_203003 |
" |
20140510_203025 |
old SN, open loop |
20140510_203740 |
old SN, CL 100 modes, gain 0.5 |
20140510_203813 |
new SN, CL 100 modes, g 0.5 |
20140510_203840 |
" |
We try to set UDP port 10002 to receive the
tubone data from ASM. Fail!
TN |
Notes |
20140510_211438 |
CL, g 0.1, no TT correction |
20140510_211457 |
" |
20140510_211517 |
" |
20140510_211554 |
CL, g=0.5, no TT |
20140510_211637 |
" |
20140510_211734 |
" |
20140510_211931 |
CL, g=0.5, no TT, jitter loop closed |
20140510_211950 |
" |
20140510_212014 |
" |
20140510_221516 |
CL 150 modes, g=0.2, 1kHz, no jitter |
20140510_223440 |
CL 150 modes, g=0.35 on TT, 0.25 on HO |
20140510_223506 |
" |
We recalibrated the amplitude of the modes, each mode is weighted by the slope rms recorded during the IM acquisition. The weighting coefficients are stored here:
/home/argos/calib/DX/aarb/aoloop/amp_calibrated.fits
So all the new IM have the modal amplitudes optimized:
TN |
Notes |
Rec |
20140510_231120 |
CL 150 modes, g 0.5 on TT, 0.4 on HO |
150modes_optimized.fits |
20140510_231149 |
" |
" |
20140510_231225 |
" |
" |
We switch to
BLUE pupil.
REC: 50modes_ol_blue, 150modes_blue
TN |
Notes |
20140511_000000 |
CL 150 modes, 1kHz |
20140511_000054 |
OL |
DARK: 20140511_000552
17:12 VNC crash...