Encyclopedia of Planetary Landforms

2015 Edition
| Editors: Henrik Hargitai, Ákos Kereszturi

Reversing Dune

Reference work entry
DOI: https://doi.org/10.1007/978-1-4614-3134-3_305

Definition

“A dune that tends to develop unusual height but migrates only a limited distance because seasonal shifts in direction of the dominant wind cause it to move alternately in nearly opposite directions” (Jackson 1997, p. 545).

Description

Reversing dunes are intermediate in character between star and transverse dunes. They are similar to transverse dunes but have a secondary slip face which develops periodically and is oriented in an opposite direction from that of the primary slip face (McKee 1979).

Subtype

Sigmoidal dune. S-shaped or straight, triangular (Tsoar 2001), steep-sided, sharp-crested dune which is formed in response to alternating and opposing winds of roughly equal velocities (Holm 1957; Stone 1967; Edgell 2006) (Fig. 1).
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References

  1. Edgell HS (2006) Arabian deserts: nature, origin and evolution. Springer, DordrechtCrossRefGoogle Scholar
  2. Fenton LK (2005) Potential sand sources for the dune fields in Noachis Terra, Mars. J Geophys Res 110:E11004. doi:10.1029/2005JE002436CrossRefGoogle Scholar
  3. Fenton LK, Bandfield JL, Ward AW (2003) Aeolian processes in Proctor Crater on Mars: sedimentary history as analyzed from multiple data sets. J Geophys Res 108(E12):5129. doi:10.1029/2002JE002015CrossRefGoogle Scholar
  4. Fenton LK, Toigo AD, Richardson MI (2005) Aeolian processes in Proctor Crater on Mars: mesoscale modeling of dune-forming winds. J Geophys Res 110:E06005. doi:10.1029/2004JE002309Google Scholar
  5. Holm DA (1957) Sigmoidal dunes – a transitional form. (abs). Geol. Soc. America Bull 68(12) 2, 1746Google Scholar
  6. Jackson JA (ed) (1997) Glossary of Geology, 4th edn. Am. Geol. Inst, Alexandria, p 769Google Scholar
  7. McKee ED (1979) Introduction to a study of global sand seas. In: McKee ED (ed) A study of global sand seas. U.S. geological survey professional paper, U.S. Govt. Print. Off., Washington vol 1052. pp 1–19Google Scholar
  8. Silvestro S, Di Achille G, Ori GG (2010) Dune morphology, sand transport pathways and possible source areas in east Thaumasia Region (Mars). Geomorphology 121:84–97. doi:10.1016/j.geomorph.2009.07.019CrossRefGoogle Scholar
  9. Silvestro S, Fenton LK, Michaels TI, Valdez A, Ori GG (2012) Interpretation of the complex dune morphology on Mars: dune activity, modelling and a terrestrial analogue. Earth Surf Proc Land 37(13):1424–1436. doi:10.1002/esp.3286CrossRefGoogle Scholar
  10. Stone RO (1967) A desert glossary. Earth Sci Rev 3:211–268CrossRefGoogle Scholar
  11. Tsoar H (2001) Types of Aeolian sand dunes and their formation. In: Balmforth NJ, Provenzale A (eds) Geomorphological fluid mechanics, Lecture notes in physics 582. Springer, p 403Google Scholar
  12. Zimbelman JR (2010) Transverse Aeolian Ridges on Mars: first results from HiRISE images. Geomorphology 121:22–29. doi:10.1016/j.geomorph.2009.05.012CrossRefGoogle Scholar

Copyright information

© Springer Science+Business Media New York 2015

Authors and Affiliations

  1. 1.Carl Sagan CenterSETI InstituteMountain ViewUSA
  2. 2.Geography DepartmentUmm Al-Qura UniversityMakkah Al-MukkarramahKingdom of Saudi Arabia