Stereophotoclinometry for Navigation - Dr. Eric E. Palmer

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Stereophotoclinometry for Navigation - Dr. Eric E. Palmer
Stereophotoclinometry for
       Navigation
        Dr. Eric E. Palmer
Stereophotoclinometry for Navigation - Dr. Eric E. Palmer
What is
            Stereophotoclinometry
•   A suite of tools designed to generate a shape model (Digital Elevation Model)
    using all imagery possible
•   Blends the best parts of Stereo with 2D Photoclinometry to minimize the errors
    of each
      •   Stereo: Sets absolute distance
      •   Photoclinometry: Allows a wider range of emission and illumination
          conditions
•   Solves for topography and albedo, allowing any illumination and observation
    condition to provide useful data

                            Real                  Model
Stereophotoclinometry for Navigation - Dr. Eric E. Palmer
Photoclinometry
         Same surface material (and albedo)
Brightness determined by angle to the Sun (incidence)
Stereophotoclinometry for Navigation - Dr. Eric E. Palmer
How It Works
• What to you do with ……
     Same feature but unrelated angles
What is in common?
Real

Model
We build a world
• Pick a point
• Build a 99x99 pixel
  “maplet” around it
• Align every image
  that intersects this
  maplet
• Solve for slope x,
  slope y and albedo
Generate Small Maps
     Center point determined
            by stereo

                               Interstitial heights by
                                  photoclinometry
•   Combine the maplets to form a whole object
•   Iterate to smooth the maplets until a
    common solution
67P Churyumov–Gerasimenko
Performance
•   Build DEM down to image resolution

      •   In special cases, we can extrapolate by a factor of two

•   Error is “on the order” of the image resolution

      •   SPC registers all image to a mean of one pixel

•   For ORex (at 5km orbit).

      •   Spacecraft uncertainty:
SPC’s improves standard
              stereo
•   Stereo is limited with observation conditions

      •   Maximum stereo angle between images ~ 40°

      •   Requires very similar illumination

•   SPC

      •   Resizes and orthorectifies every image

      •   Generates a model image for every image that is illuminated with
          matching conditions

            •   This step requires topography and albedo

      •   Allows every image to be used to extract topographic information
SPC’s improves standard
         photoclinometry
•   2D solutions — 1D solutions could cause error if the
    line was not allow the maximum slope. SPC avoids
    this because it solves for the entire surface

•   Solve for albedo — Standard photoclinometry
    assumes a uniform albedo. SPC solves for the albedo
    on a pixel-to-pixel basis.

•   Multiple images — SPC uses multiple images taken
    with different phase angles. This reduces the impact
    of noise, cosmic rays, blur and the photometric
    response of the surface.
Sonoita, Arizona
Real Image - 0.6 m/pix   SPC Model - 1.5 m/pix
Karpinskiy Crater
Lunar regional DEMLROC
                   withImage                                               SPCm/px.
                        grid overlay. Image above has been down-sampled to 10  Model

                                                                              72.69° N 166.76° E
Building Features
•   Start with a global model

•   Using nominal flight path, identify
    footprint (with uncertainty) for each
    NavCam image

•   Select features in expected NavCam
    footprint and identify them in existing
    images

    •   Low emission angles provide the best

    •   Suggest 3 to 5 features

        •   Want them spread across the field
            of view
Example of OREx Feature
                (P3808)
Rocks/boulders are good for
humans, but poor choices for
shape models. Small errors
in height result in large errors
when casting shadows

                                   Feature

                                   TAG Site
 3cm/pixel
Source Image

Example P3808

       3D Perspective View
•   Average Correlation 0.8160   Rendered Image
•   38 Images (1.2 to 6cm)
•   125 Pixels wide
•   GSD 3.2 cm
Source Image

           Accuracy
•   Two components that must be correct

     •   3D position in space. This is considered
         the normal concept of accuracy. Is the
         model in the correct location in space.
                                                      Rendered Image
     •   Correlation. To do TRN, the rendered
         images must be similar to the NavCam
         images. If they are not, then the feature
         cannot be uniquely identified.

           •   Failed to identify is poor

           •   Incorrectly identify must be avoided
Quality
•   Correlation scores indication how close the rendered image matches the actual image.

•   Issues impacting correlation score

    •   Large rocks hurt — craters are fine

    •   Albedo features are very useful

    •   Unsampled imagery observing conditions

               0.60                           0.69                      0.78

                        Example Correlation Scores
Types of Images
   “Albedo” Image           Topographic Image
 Incidence angle ~ 0        Incidence angle > 0
Emission Angle - flexible   Emission Angle > 30
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