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Geophysical Research Letters
Article . 2003 . Peer-reviewed
License: Wiley Online Library User Agreement
Data sources: Crossref
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Origin of the polygons and the thickness of Vastitas Borealis Formation in Western Utopia Planitia on Mars

Authors: Kenji Yoshikawa;

Origin of the polygons and the thickness of Vastitas Borealis Formation in Western Utopia Planitia on Mars

Abstract

Many middle scale (about 100m cracking space) polygons are located between the area of the giant polygons and the thumbprint terrains in Western Utopia Planitia. Most of the patterns are located on Vastitas Borealis Formation. The polygonal patterns have frequently been associated with collapsed features, such as a covered trough like features(the width of the underground crack is approximately 400–500 m). The thickness of the surface materials (6–12 m), where polygonal patterns occur, was calculated based on the space of cracking relationship. Polygonal networks with strongly oriented features and parallel to the contour line are likely caused by structural (geological) origin as well as bending forces from the center of the basin.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
20
Top 10%
Average
Average
gold