a comparison of lunar images from clementine and lunar orbiter to search for new surface features or...

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The Lunar Surface: Visualizing Changes A Comparison of Lunar Images from A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search Clementine and Lunar Orbiter to Search for New Surface Features or Craters for New Surface Features or Craters Chitra Sivanandam, Roger Easton, Chitra Sivanandam, Roger Easton, Zoran Ninkov Zoran Ninkov Center for Imaging Science Center for Imaging Science Rochester Institute of Technology Rochester Institute of Technology May 8, 1998 May 8, 1998

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Page 1: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

The Lunar Surface: Visualizing Changes

A Comparison of Lunar Images from A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for Clementine and Lunar Orbiter to Search for

New Surface Features or CratersNew Surface Features or Craters

Chitra Sivanandam, Roger Easton, Zoran NinkovChitra Sivanandam, Roger Easton, Zoran NinkovCenter for Imaging ScienceCenter for Imaging Science

Rochester Institute of TechnologyRochester Institute of Technology

May 8, 1998May 8, 1998

Page 2: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

OutlineOutline

IntroductionIntroduction Proposed ObjectivesProposed Objectives Accomplished Tasks/ResultsAccomplished Tasks/Results AnalysisAnalysis ConclusionConclusion

Page 3: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

IntroductionIntroduction

Lunar Orbiter ImageryLunar Orbiter Imagery Higher Resolution (scan from a contact print)Higher Resolution (scan from a contact print) Better ground resolutionBetter ground resolution Do not have as much information on how the Do not have as much information on how the

image was takenimage was taken exact latitudes and longitudesexact latitudes and longitudes angle of the photographangle of the photograph

Page 4: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

Introduction Introduction cont’dcont’d

Clementine ImageryClementine Imagery Lower resolution, both in ground spot and in Lower resolution, both in ground spot and in

image resolutionimage resolution PDS formatPDS format Have much information on the specifics Have much information on the specifics

pertaining to imagerypertaining to imagery latitudes, longitudes, angle, etc.latitudes, longitudes, angle, etc. limited bandwidth (sensor) compared to sensitivity limited bandwidth (sensor) compared to sensitivity

of filmof film

Page 5: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

Proposed ObjectivesProposed Objectives

Create a tool to use both sets of imagesCreate a tool to use both sets of images Try to account for differences in imagery Try to account for differences in imagery

that do not translate to differences in the that do not translate to differences in the surfacesurface

Look for any differences in the surface that Look for any differences in the surface that may have occurred as a result of timemay have occurred as a result of time

Page 6: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

Accomplished Tasks/ResultsAccomplished Tasks/Results

Created a procedure using NasaView (for Created a procedure using NasaView (for Clementine images), Erdas Imagine, Clementine images), Erdas Imagine, Photoshop and code written in IDLPhotoshop and code written in IDL NasaView - to chose an appropriate section of the NasaView - to chose an appropriate section of the

16bits to use16bits to use Photoshop - convert images to tiff formatPhotoshop - convert images to tiff format Imagine - used the GCP (ground control points) Imagine - used the GCP (ground control points)

editor to create a transform to resample imageseditor to create a transform to resample images IDL - to do the differencingIDL - to do the differencing

Page 7: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

Accomplished Tasks/Results Accomplished Tasks/Results cont’dcont’d

Using IDL, created a tool to do differencing Using IDL, created a tool to do differencing trying to account for various problems with trying to account for various problems with imagery (using test images)imagery (using test images)

Page 8: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

Accomplished Tasks/Results Accomplished Tasks/Results cont’dcont’d

After doing the resampling and After doing the resampling and transformation, applied the code to imagestransformation, applied the code to images

Major differences occurred because the Major differences occurred because the Orbiter image was of a much higher Orbiter image was of a much higher resolution than the Clementine imageresolution than the Clementine image

Chose to use a low pass filterChose to use a low pass filter Invested the use of a Robert’s gradient for Invested the use of a Robert’s gradient for

edge detection prior to differencingedge detection prior to differencing

Page 9: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

Accomplished Tasks/Results Accomplished Tasks/Results cont’dcont’d

Lunar Orbiter image Using a low pass filterLunar Orbiter image Using a low pass filter

Clementine imageClementine image

Page 10: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

Accomplished Tasks/Results Accomplished Tasks/Results cont’dcont’d

Low Pass filterLow Pass filter Gaussian Filter, with a weight of 121Gaussian Filter, with a weight of 121

12321

271172

31117113

271172

12321

Page 11: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

Accomplished Tasks/Results Accomplished Tasks/Results cont’dcont’d

Robert’s GradientRobert’s Gradient

of Orbiter image of low pass imageof Orbiter image of low pass image

Page 12: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

Accomplished Tasks/Results Accomplished Tasks/Results cont’dcont’d

Robert’s Gradient for Clementine imageRobert’s Gradient for Clementine image

Page 13: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

Accomplished Tasks/Results Accomplished Tasks/Results cont’dcont’d

Difference simply Difference simply between imagesbetween images

Difference using the Difference using the low pass imagelow pass image

Page 14: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

Accomplished Tasks/Results Accomplished Tasks/Results cont’dcont’d

Resultant images using the Robert’s gradient / Resultant images using the Robert’s gradient / edge detection before actual differencingedge detection before actual differencing

Page 15: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

AnalysisAnalysis

Smaller, higher frequency differences do Smaller, higher frequency differences do not show up as much when using the low not show up as much when using the low pass filterpass filter

Overall differences due to the histograms of Overall differences due to the histograms of the images are taken care of by doing an the images are taken care of by doing an edge detectionedge detection

Page 16: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

Analysis Analysis cont’dcont’d

What is causing all of the differences?What is causing all of the differences? Most of the features from the difference images Most of the features from the difference images

exist in the Orbiter imageexist in the Orbiter image Most of the difference seems to be due to the Most of the difference seems to be due to the

differences in image resolutiondifferences in image resolution The bulk of the differences is due to the The bulk of the differences is due to the

illumination angle at the time the images were illumination angle at the time the images were takentaken

Page 17: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

ConclusionConclusion

It is possible to create a tool to work with both sets It is possible to create a tool to work with both sets of imageryof imagery

It would be more useful if the images have It would be more useful if the images have something in common (i.e. ground resolution).something in common (i.e. ground resolution).

There were too many differences between the There were too many differences between the imagery.imagery.

Basically, the region immediately near the crater Basically, the region immediately near the crater Aristarchus does not seem to have changed over Aristarchus does not seem to have changed over the last 30 years.the last 30 years.

Page 18: A Comparison of Lunar Images from Clementine and Lunar Orbiter to Search for New Surface Features or Craters The Lunar Surface: Visualizing Changes A Comparison

Senior Research: May 8, 1998

Chitra Sivanandam

THE ENDTHE ENDwww.cis.rit.edu/~cxs2479www.cis.rit.edu/~cxs2479