The effect of sub-pixel slope variations on photoclinometry

Richard J. Greenberg, Marita Morris, Mark A. Foley

Research output: Contribution to journalArticle

1 Citation (Scopus)

Abstract

Sub-pixel slope variations can have significant effects on the intensity of light scattered from a planetary surface. As a result, determination of the surface slope from the apparent brightness of a given pixel can be confounded by uncertainly in such variations. Under a wide range of conditions, the average slope across the pixel may be different from what is inferred by photoclinometry. Because topography is derived from photoclinometry by integrating the slope across an image composed of many pixels, topographic elevation could in principle be distorted considerably by this effect. As actually applied, photoclinometry generally includes strategies designed to mitigate these effects substantially. Nevertheless, the potential always exists for unknown variations in the character of sub-pixel topography (among other uncertainties such as albedo variations) to introduce errors. The results shown here show the importance of the mitigating strategies and of considering the magnitude of uncertainties in determination of topography.

Original languageEnglish (US)
Pages (from-to)348-350
Number of pages3
JournalIcarus
Volume214
Issue number1
DOIs
StatePublished - Jul 2011

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photogrammetry
pixel
pixels
slopes
topography
planetary surfaces
planetary surface
albedo
brightness
effect

Keywords

  • Data reduction techniques
  • Geological processes
  • Geophysics
  • Image processing
  • Photometry

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

The effect of sub-pixel slope variations on photoclinometry. / Greenberg, Richard J.; Morris, Marita; Foley, Mark A.

In: Icarus, Vol. 214, No. 1, 07.2011, p. 348-350.

Research output: Contribution to journalArticle

Greenberg, Richard J. ; Morris, Marita ; Foley, Mark A. / The effect of sub-pixel slope variations on photoclinometry. In: Icarus. 2011 ; Vol. 214, No. 1. pp. 348-350.
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