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Lunar impact crater modeling using trinocular stereoscopic depth inpainting

  • Raghavendra H. Bhalerao
  • , Shirish S. Gedam
  • , Jyoti Joglekar
  • , Andres Almansa
  • Indian Institute of Technology Bombay
  • CNRS LTCI

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

In this paper a novel approach of stereoscopic depth inpainting is used to model lunar craters. In the case of lunar mission, the disparity map generation using stereoscopic images is limited by shadows inside impact craters. Impact craters are most important features on lunar surface but cannot be modeled using stereo cue alone. Taking into consideration the importance of crater modeling and limitations of stereo cue, we are proposing stereoscopic depth inpainting method as an additional method to model the lunar impact crater.

Original languageEnglish
Title of host publication2013 IEEE 2nd International Conference on Image Information Processing, IEEE ICIIP 2013
Pages1-4
Number of pages4
DOIs
Publication statusPublished - 1 Dec 2013
Externally publishedYes
Event2013 IEEE 2nd International Conference on Image Information Processing, IEEE ICIIP 2013 - Shimla, HP, India
Duration: 9 Dec 201311 Dec 2013

Publication series

Name2013 IEEE 2nd International Conference on Image Information Processing, IEEE ICIIP 2013

Conference

Conference2013 IEEE 2nd International Conference on Image Information Processing, IEEE ICIIP 2013
Country/TerritoryIndia
CityShimla, HP
Period9/12/1311/12/13

Keywords

  • depth inpainting
  • depth map
  • impact crater
  • stereo

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