PERFORMANCE MONITORING AND ASSESSMENT WEEKLY MEETING #5 Tuesday June 5, 1990, 1:30 - 3:30 p.m. Goddard Space Flight Center, Building 8, 3rd Floor Management Conference Center N303 [Excerpt from the minutes as circulated by e-mail, file dated 11 June 1990. Only the OTA/wavefront items and the meeting schedule are reproduced; attendee contact details omitted.] PMA Status - Keith Kalinowski ... The first monthly PMA meeting will be a joint SWG/HST Users Committee/PMA monthly to be held June 27 in Building 22 Room 365. ... Executive Summary (extract) Bob Basedow reported on the current OTA status. He presented results of analysis on the FGS's, the Optical Control System/Wavefront Sensors and the Thermal system. ... The Image size is ~ 0.7 arcsecs and the wavefront is estimated at: Focus ~ 2 waves, astigmatism ~.2 waves, coma ~ 4 waves, and spherical is ~ .2 waves. There are currently no significant thermal anomalies. OTA STATUS - Bob Basedow, HDOS OCS/WAVEFRONT Status o Focus currently best achievable using FGSs (Bootstrap Phase A) o FGS data indicates image size ~0.7 asecs o WFPC data consistent with this, but shows central 0.15 asec core o HDOS Phase retrieval algorithm applied to PC image of 6/3/90 o Wavefront estimated at: FOCUS ~ 2 WAVES o-p ASTIGMATISM ~0.2 WAVES o-p COMA ~4 WAVES o-p SPHERICAL ~0.2 WAVES o-p o Estimate probably significantly affected by WFPC optics, especially central obscuration alignment The phase retrieval model does not account for the WFPC optics, and therefore cannot reproduce the PSF's. Nutuation of the annulus around the peak of the PSF, is attributed to the mis-alignment of the secondary mirror. OBA is a package which finds the aberrations given a PSF Measured PSF's are taken from the WF/PC Have Fit "1st Light" WFC PSF and a PC PSF Ongoing Analysis: Find cause of skirt around PSF (pupil vignette) Field Dependence in WF/PC CCD arrays Further algorithm refinement WFPC REPORT There was no one available to report on the status of the WFPC.