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Viscous Flow Features (Mars)

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Encyclopedia of Planetary Landforms

Definition

Viscous flow feature (VFF) is “an umbrella term for all glacial-type formations exhibiting evidence of viscous flow” (Souness et al. 2012). VFF is defined (in broad sense) as “primary or secondary lobate features of the material (typically in alcoves), lineations on the surface (both parallel and transverse to the slope on which the material flows), compressional ridges or extensional troughs, ridges at the flow front or base of the slope, or other general evidence that the material flowed around or over obstacles such as craters or mounds” (Milliken et al. 2003). In general, they are elongated flow-like features composed of ice and rock mixture in the middle latitude region of Mars.

Viscous flow refers to viscous or ductile downslope flow (Souness et al. 2011). Subtypes are probably in close interrelationships (Souness et al. 2012).

Synonyms and Examples

Amazonian-aged glacial landsystems; Cold-based glacial features; Integrated LVF/LDA/CCF glacial landsystem; Midlatitude...

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References

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Correspondence to Henrik Hargitai .

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Hargitai, H. (2014). Viscous Flow Features (Mars). In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_596-1

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  • DOI: https://doi.org/10.1007/978-1-4614-9213-9_596-1

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