Differences between revisions 15 and 16
Revision 15 as of 2015-11-24 17:56:50
Size: 4827
Editor: DianeLambert
Comment:
Revision 16 as of 2015-11-25 13:44:01
Size: 5328
Editor: DianeLambert
Comment:
Deletions are marked like this. Additions are marked like this.
Line 1: Line 1:
Test 11: ReferencePeaks = Test 11: ReferencePeaks =

== Aim and Objectives ==

'''Purpose of test:''' To evaluate SPC's ability to represent a simplified 'boulder' which has a constant 20 degree slope.

'''Additional Objectives'''
 * To investigate the effect of including various combinations of viewing conditions, specifically:
  * Variation of spacecraft azimuth;
  * Variation of sun zenith (incidence);
  * Variation of spacecraft zenith (emission angle);
 * To investigate the effect of the number of images and viewing conditions.
Line 4: Line 15:

Test 11: ReferencePeaks

Aim and Objectives

Purpose of test: To evaluate SPC's ability to represent a simplified 'boulder' which has a constant 20 degree slope.

Additional Objectives

  • To investigate the effect of including various combinations of viewing conditions, specifically:
    • Variation of spacecraft azimuth;
    • Variation of sun zenith (incidence);
    • Variation of spacecraft zenith (emission angle);
  • To investigate the effect of the number of images and viewing conditions.

Take PIT020 as the only maplet in MAPLIST.TXT. Generate 5cm images of the topography (which is based at TAG Site 1). Then we build a MAPLET, saving the MAPLETs flatMapVect at several states.

Simple Variations

Groups of images - (adjusted for 5cm)

  • Test11A - Detailed Survey. Eric (Has 11 images, very low in sample space)
  • Test11B - Min Orbit B (by hand, calculate the minimum requirement)
  • Test11C - Average Orbit B (use a random Orbit B solution with 3 unique observation/illumination conditions)
  • Test11D - Best Orbit B (as we did before)
  • Test11E - Optimum Collection (as we did before)

Name

Sun Az

Sun Zenith

S/C Az

S/C Zenith

Optimum Collection1

0, 90, 180, 270

45

every 20

45

Optimum Collection2

135

30

every 20

45

  • Test11X - Criss Cross (combine both of these sets)

Name

Sun

S/C Az

S/C Zenith

Criss Cross 1

80, 60, 40, 20, 0, -20, -40, -60, -80

45

45

Criss Cross 2

45

0, 180

80, 60, 40, 20, 0

Variations

Spacecraft Azimuth Variations

Name

Sun

S/C Az

S/C Zenith

RMS w/trans

Test11F

45, 0, -45

every 20

45

Test11G

45, 0, -45

every 30

45

Test11H

45, 0, -45

every 45

45

Test11I

45, 0, -45

every 60

45

Test11J

45, 0, -45

every 90

45

Sun Variations

Name

Sun

S/C Az

S/C Zenith

RMS w/trans

Test11K

30

every 45

45

Test11L

30 -30

every 45

45

Test11M

-45, -45

every 45

45

Test11N

30, 0, -30

every 45

45

Test11P

45, 30, 0, -30, -45

every 45

45

Test11Q

60, 45, 30, 0, -30, -45, -60

every 45

45

Test11R

60, 30, -30, -60

every 45

45

Spacecraft Zenith Variations

Name

Sun

S/C Az

S/C Zenith

Total Number of Images

Test11S

45, 0, -45

every 45

0, 30, 60

80

Test11T

45, 0, -45

every 45

0, 20, 40, 60

112

Test11U

45, 0, -45

every 45

0, 15, 30, 45, 60

144

Hill Data

I have created the following hills for testing

  • REGION - Includes lots of craters and a few 20 deg peaks

Truth Maplets

  • -8.027 262.768
  • T11TRU.MAP - already built. It has the truth heights loaded from PIT020.
  • T11TRU.TXT -- Text file of the maplet. Use for plotting transits
  • t11-truth.obj -- OBJ file for testing using CompareOBJ

Testing Maplets

  • -8.027 262.768
  • Build a model MAPLET using TAG Site 1 center position (5cm resolution and Q=49). Do not load a base map for topography
  • Create MOD20#, which # is the test number (letter)
  • Align the images with the key location at 50/50.
  • Build template with 100
  • (Skip until close to perfect) -- Do an auto align
  • Build height using the iteration template
  • Do flatMapVec and rename it to mod-20#-1
  • Do compMapVec between MOD20# and T11TRU
  • Repeat as necessary

Iteration Template

0
0
44
2
8                fill no data with shape slope
7
.01
6
y
y
1                condition with overlapping maps
2                condition with existing topo
.01
6
y
y
0                begin integration
.025
100
0
v
1
u
1
o                overlaps
RECENT
n
1
i
r
n
n

Useful copy/paste stuff

echo CENTER | /usr/local/localBin/flatMapVec 
 /usr/local/localBin/compMapVec MAPFILES/CENTER MAPFILES/T11TRU.MAP
~/eval/bin/Maplet2FITS MAPFILES/CENTER fit
 ~/eval/bin/FITS2OBJ --local fit center.obj
 ~/eval/bin/CompareOBJ    --compute-optimal-translation-and-rotation   center.obj newtru.obj 
convert  LMRK_DISPLAY1.pgm display.jpg
mkdir step02
cp CENTER.TXT MAPFILES/CENTER.MAP step02

gnuplot
set term x11
set style data lines
plot 'NEW020.TXT' u 0:50 lw 3 lc 0, 'CENTER.TXT' u 0:50 
set output 'out.png' 
set term png
replot
unset output
set term x11
exit

mv out.png mod20f.obj MOD20F.TXT comp.txt display.jpg step2

Save States

The goal is to see the evolution of the model over time. You can stop iterations once the peak and base are stable. The most likely tool to evaluate if the model has reached it best fit will be transit.

Save the flatMapVect statistics at the following number of iterations

  • 1st
  • 2nd
  • 3rd
  • 5th
  • 10th
  • 15th
  • 20th
  • 50th (if needed)
  • 100th (if needed)
  • 200th (if needed)

Examples

Example of a 14 degree peak, measured at difference locations

Example of a 20 degree peak, measured over time

ReferencePeaks_dep Deprecated Reference Peaks (If at 1st you dont succeed...)

ReferencePeaks (last edited 2016-01-05 16:52:29 by DianeLambert)