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