Changes between Initial Version and Version 1 of docs/CommissioningPlan/P2.6

Timestamp:

03/05/20 12:29:08 (5 years ago)

Author:

kradhakrishnan

Comment:

--

docs/CommissioningPlan/P2.6

@@ +1 @@
+== P2.6 Measurement of NCPA == 
+•       **Phase**               :       2  
+•       **Status**              :       Draft    
+•       **Category**            :       Daytime calibration (C3)
+•       **Recurrence**  :       after instrument installation at telescope platform
+•       **Duration**            :       3 hour(s)
+**Description**
+•       Measure the Non-Common Path Aberrations (NCPA).
+**Prerequisites**
+•       RR mounted and SHARK-NIR aligned to telescope.
+**Procedure**
+•       In closed-loop, we optimize the PSF shape on SCICAM using the trial & error algorithm used by LBTO team during LUCI calibrations changing M2 reference shape applying modes coefficients.
+•       We also perform the phase-diversity tests using the same light source and look at the NCPA output produced.
+•       Depending on the two results and the quality of PSF, we may choose one or the other or the combination of both.
+•       Note that we may do this for different elevation angles.
+**Success criteria**
+•       NCPA estimated and applied on the ASM? (how often we do this? Every night?
+•       Satisfactory PSF quality with closed-loop and get a new and improved daytime telescope model for SHARK-NIR?
+**Notes**
+•       See activity 8.1 in AD4 for more details. 
+**LBTO support**
+•       Mount the RR on SX
+•       Support from LBTI?
+**Associated SHARK-NIR personnel**
+•       JF, LM, MdP, MM (from AZ)
+**Date performed and by whom**