= F3A - Baseline Testing Model = '''Goal:''' Establish the baseline for evaluation of the shape model degradation or improvement. == Test Set Up == '''Data:''' Shape model 3.7 and 3.8 images, both global and TAG sites. Perturbed SPICE kernels. '''Start:''' Nolan Shape Model '''Navigation Uncertainties:''' TBD (Due 24 July 2015)-- The uncertainties will be added to the SPK and CK as done for the component test: a constant arc for the spacecraft position, changed at every OD, and a random pointing error at every observation, unrelated to the previous observation's error. If provided, we will use expected performance rather than requirements for the baseline. '''Image Error:''' We are not using significant error for the images during this phase. It will only include a shot noise and pedestal. '''Lens Distortion:''' N/A For PolyCam and MapCam, we are not applying lens distortion. '''Build:''' Build the shape model, saving several very specific models along the way: * Appch1: Far Approach 1.5m GSD global, computed with 1.5m MAPLETS -- Q=256 * Appch2: Best Effort Approach, 75cm GSD global, computed with 75cm MAPLETS * 75cm1: 75 cm Global: 75cm GSD global, computed with 35cm MAPLETS * 35cm1: 35 cm Global: 35cm GSD of TAG Site 1 It will be computed with 2.5 cm MAPLETS. 100x100 meters == Directory Setup == If needed to start {{{ rsync --delete -hapvP ormacsrv1.lpl.arizona.edu:/Volumes/Data1/spc-test/F3A/ps/ ps }}} Make fresh and copy needed DS files over {{{ cd F3A ls ds # should not exist rsync -hapvP ps/ ds rm ds/IMAGEFILES # symbolic link cp -av base/IMAGEFILES ds cp -av setup/H2-DS-PolyCam-Nadir/perturbed-SUMFILES/* ds/SUMFILES cp -av setup/H2-DS-PolyCam-Nadir/perturbed-NOMINALS/* ds/NOMINALS cp -av setup/H2-DS-PolyCam-Nadir/IMAGEFILES/* ds/IMAGEFILES cp -av setup/H3-DS-PolyCam-Stereo-v5/perturbed-SUMFILES/* ds/SUMFILES cp -av setup/H3-DS-PolyCam-Stereo-v5/perturbed-NOMINALS/* ds/NOMINALS cp -av setup/H3Images/* ds/IMAGEFILES }}} Get the images ready {{{ cd ds mv -f ../setup/new-PICTLIST.TXT PICTLIST.TXT }}} == Register the images == * Use Block 3 - Register == Test == * Tile at 20cm * Use Block 6B - BIGMAP Tile * Look for correlation errors * Tile at 10cm * Use Block 6B - BIGMAP Tile * Look for correlation errors * Tile at 5cm * Use Block 6B - BIGMAP Tile -- with script/XXX005 that has a more inclusive pull * Clean using Block 7