Distribution of polygon characteristic scale in Martian patterned ground terrain in the northern hemisphere using the Fourier transform

T. Orloff, M. Kreslavsky, E. Asphaug

Research output: Contribution to journalArticle

3 Citations (Scopus)

Abstract

Permafrost patterned ground forms on the surface of nearly all landscapes between 50°N and 70°N on Mars. This landform appears in satellite imagery as an interconnected network of polygonal shapes. Previous studies used geomorphologic observations to characterize patterned ground terrains on Mars. These classification systems prove useful but suffer from somewhat subjective methods. We find objective analysis of the polygons comprising patterned ground terrains on the surface of Mars feasible using High Resolution Imaging Science Experiment imagery acquired from orbit. We perform a two-dimensional Fourier transform on 124 images of patterned surfaces to characterize the spatial scale pertinent to scenes and analyze the distribution of these properties on the surface of Mars between 50°N and 70°N. We find two distinct sets of polygons: large polygons which form below 60°N and small polygons primarily above 60°N with exception for sites within Acidalia Planitia. Our findings show similar trends to those found in previous studies but also fundamental differences in the populations of polygons above and below 60°N. The polygons within 60°N-70°N share roughly the same polygonal scale, implying that seasonal temperature change is not the only factor forcing polygon development as previous models found. In some cases, our method indicates the presence of multiple scales of polygons, although it cannot quantify the larger scale. This method in conjunction with observational analysis improves our ability to characterize surfaces and examine patterned ground terrains on Mars. Key Points Fourier transforms of Martian patterned ground yield reliable characterizations Fourier transforms of patterned ground give results similar to previous surveys The characteristic spatial scale is a proxy for polygon diameter

Original languageEnglish (US)
Pages (from-to)1558-1566
Number of pages9
JournalJournal of Geophysical Research E: Planets
Volume118
Issue number7
DOIs
StatePublished - 2013

Fingerprint

patterned ground
polygons
Northern Hemisphere
polygon
Fourier transform
Fourier transforms
mars
Mars
Landforms
Permafrost
Satellite imagery
Orbits
landforms
permafrost
distribution
satellite imagery
Imaging techniques
imagery
landform
Experiments

Keywords

  • Mars
  • patterned ground

ASJC Scopus subject areas

  • Geochemistry and Petrology
  • Geophysics
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science

Cite this

Distribution of polygon characteristic scale in Martian patterned ground terrain in the northern hemisphere using the Fourier transform. / Orloff, T.; Kreslavsky, M.; Asphaug, E.

In: Journal of Geophysical Research E: Planets, Vol. 118, No. 7, 2013, p. 1558-1566.

Research output: Contribution to journalArticle

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