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The Energy Balance in Short Gravity Waves

  • G. J. Komen

Abstract

Earlier results on the energy balance in gravity waves (Komen, Hasselmann and Hasselmann, 1985) are discussed. It is shown that these can be used to describe the evolution of short gravity waves, provided wind speeds are low enough. For higher wind speeds equilibrium range ideas are considered.

Keywords

Source Term Gravity Wave Significant Wave Height Wave Spectrum Wind Wave 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Kitaigorodskii, S.A., V.P. Krasitskii and M.M. Zaslavskii (1975) ‘On Phillips’ theory of equilibrium range in the spectra of wind-generated gravity waves.’ J. Phys. Oceanogr. 5, 410.CrossRefGoogle Scholar
  2. Komen G.J., S. Hasselmann and K. Hasselmann (1984) ‘On the existence of a fully developed wind-sea spectrum.’ J. Phys. Oceanogr. 14, 1271.CrossRefGoogle Scholar
  3. Phillips, O.M. (1958) ‘The equilibrium range in the spectrum of windgenerated gravity waves.’ J. Fluid Mech. 66, 625.CrossRefGoogle Scholar
  4. Phillips, O.M. (1985) ‘Spectral and statistical properties of the equilibrium range in wind-generated gravity waves.’ J. Fluid Mech. 156, 505–531.CrossRefGoogle Scholar
  5. Toba, Y (1973) ‘Local balance in the air-sea boundary process III On the spectrum of wind waves.’ J. Oceanogr. Soc. Japan 29, 209.CrossRefGoogle Scholar

Copyright information

© Kluwer Academic Publishers 1989

Authors and Affiliations

  • G. J. Komen
    • 1
  1. 1.KNMIDe BiltThe Netherlands

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