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Megaripple dynamics on a dissipative sandy beach
Author(s) -
Jon Miles,
Antony Thorpe,
Paul Russell,
Gerd Masselink
Publication year - 2014
Publication title -
journal of coastal research
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.247
H-Index - 90
eISSN - 1551-5036
pISSN - 0749-0208
DOI - 10.2112/si70-032.1
Subject(s) - bedform , excursion , wavelength , geology , ripple , wave height , surf zone , geomorphology , dissipative system , orbital speed , oceanography , physics , sediment transport , astrophysics , optics , quantum mechanics , voltage , sediment , political science , law
Miles, J., Thorpe, A., Russell, P., Masselink, G., 2014. Megaripple dynamics on a dissipative sandy beach. In: Green, A.N. and Cooper, J.A.G. (eds.), Proceedings 13th International Coastal Symposium (Durban, South Africa), Journal of Coastal Research, Special Issue No. 70, pp. 187–192, ISSN 0749-0208. Conventional force models of bedform dimensions link bedform wavelength and height to wave orbital excursion and wave orbital velocity. Self-organization models, however, suggest that bedform wavelengths either: grow, remain stable, or are wiped flat, but are unable to reduce in length. This paper presents measurements of megaripple evolution on a macrotidal sandy dissipative beach at Perranporth, England, using measurements from a Sand Ripple Profiler. Measurements were made as the tide flooded and ebbed over the instruments, producing a cross-section of the moving surf zone for 12 separate tides. Water depths varied from 1 to 6 m, and wave heights were up to 2.2 m. The data allowed megaripple dimensions to be observed with heights up to 30 cm and wavelengths up to 1.8 m. Megaripples were observed to grow and decay in both length and height. Megaripple spacing did not increase consistently with age of ripple. Megaripple lengths changed at rates of up to 5 cm/minute, and height changed at rates of up to 0.5 cm/minute. Maximum changes took place in large orbital velocity conditions. At orbital velocities > 0.5 m/s, ripples attempted to stabilize at a wavelength related to the orbital excursion, suggesting a forced mode. The most stable ripples had the greatest height and steepness. At orbital velocities < 0.5 m/s the spacing was greater than the orbital excursion, suggesting self-organized growth may be a more appropriate model for small orbital velocities.

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