Stereophotoclinometry for Navigation - Dr. Eric E. Palmer
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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
Photoclinometry Same surface material (and albedo) Brightness determined by angle to the Sun (incidence)
• 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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