Differences between revisions 7 and 17 (spanning 10 versions)
Revision 7 as of 2016-02-23 17:40:23
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Editor: EricPalmer
Comment:
Revision 17 as of 2016-02-24 00:34:08
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Editor: EricPalmer
Comment:
Deletions are marked like this. Additions are marked like this.
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'''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. '''Navigation Uncertainties:''' 1 sigma of knowledge -- 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.
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----
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cp -av setup/H2-DS-PolyCam-Nadir/perturbed-SUMFILES/* ds/SUMFILES
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cp -av setup/H3-DS-PolyCam-Stereo-v5/perturbed-SUMFILES/* ds/SUMFILES
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/bin/cp -afv setup/registered-SUM/* ds/SUMFILES


cd base
cd scripts
ln -s XXX005.seed 0.00005.seed
ln -s XXX010.seed 0.00010.seed
ln -s XXX020.seed 0.00020.seed
cd ..

cd ds
ln -s ../setup/lsupport .
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----
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We will register the images before starting the test. We are not testing either the routine [[register]] nor the operator's ability to use it. Thus, once they are registered, we will set them into the setup directory to be used when rerunning the whole thing.


 * Setup
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 * Use Block 3 - Register === Register the new images ===
{{{
imgListName=newImagesRegister.txt
}}}
Execute [[Block 3 - Register]]


----
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 * Tile at 20cm
 * Use Block 6B - BIGMAP Tile
 * Look for correlation errors
=== Tile at 20cm ===
{{{
bigmapName=TILE20
GSD=0.00020
}}}
Execute [[Block 6B - Bigmap Tiling]]
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 * Tile at 10cm
 * Use Block 6B - BIGMAP Tile
 * Look for correlation errors
=== Iterate and Look for correlation errors ===
Execute [[Block 5 - Iterate]] -- Use the Recently Tiled scenario
{{{
find_nofitP
support/logEval.sh
}}}
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 * Tile at 5cm
 * Use Block 6B - BIGMAP Tile -- with script/XXX005 that has a more inclusive pull
 * Clean using Block 7

=== Tile at 10cm ===
{{{
bigmapName=TILE10
GSD=0.00010
}}}
Execute [[Block 6B - Bigmap Tiling]]

=== Iterate and Look for correlation errors ===
Execute [[Block 5 - Iterate]]
{{{
find_nofitP
support/logEval.sh
}}}

=== Tile at 5cm ===
{{{
bigmapName=TILE10
GSD=0.00010
}}}
Execute [[Block 6B - Bigmap Tiling]]

=== Iterate using [[Block 5 - Iterate]] and Look for correlation errors ===
Execute [[Block 5 - Iterate]]
{{{
find_nofitP
support/logEval.sh
}}}

=== Clean using Block 7 ===
Execute [[Block 7 - Clean]]

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: 1 sigma of knowledge -- 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-NOMINALS/* ds/NOMINALS
cp -av setup/H2-DS-PolyCam-Nadir/IMAGEFILES/* ds/IMAGEFILES
cp -av setup/H3-DS-PolyCam-Stereo-v5/perturbed-NOMINALS/* ds/NOMINALS
cp -av setup/H3Images/* ds/IMAGEFILES
/bin/cp -afv setup/registered-SUM/* ds/SUMFILES


cd base
cd scripts
ln -s XXX005.seed 0.00005.seed
ln -s XXX010.seed 0.00010.seed
ln -s XXX020.seed 0.00020.seed
cd ..

cd ds
ln -s ../setup/lsupport .

Get the images ready

cd ds
mv -f ../setup/new-PICTLIST.TXT PICTLIST.TXT 
rm support
ln -s ../base/support .


Register the images

We will register the images before starting the test. We are not testing either the routine register nor the operator's ability to use it. Thus, once they are registered, we will set them into the setup directory to be used when rerunning the whole thing.

  • Setup

mv -fv ../setup/registerImgList.txt make_script.in 
cp scripts/make_scriptR.seed .

Register the new images

imgListName=newImagesRegister.txt

Execute Block 3 - Register


Test

Tile at 20cm

bigmapName=TILE20
GSD=0.00020

Execute Block 6B - Bigmap Tiling

Iterate and Look for correlation errors

Execute Block 5 - Iterate -- Use the Recently Tiled scenario

find_nofitP
support/logEval.sh

Tile at 10cm

bigmapName=TILE10
GSD=0.00010

Execute Block 6B - Bigmap Tiling

Iterate and Look for correlation errors

Execute Block 5 - Iterate

find_nofitP
support/logEval.sh

Tile at 5cm

bigmapName=TILE10
GSD=0.00010

Execute Block 6B - Bigmap Tiling

Iterate using [[Block 5 - Iterate]] and Look for correlation errors

Execute Block 5 - Iterate

find_nofitP
support/logEval.sh

Clean using Block 7

Execute Block 7 - Clean

TestF3A (last edited 2016-02-26 13:54:02 by EricPalmer)