Air-Sea Interaction in Hurricanes Kerry Emanuel Massachusetts Institute of Technology.

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Presentation transcript:

Air-Sea Interaction in Hurricanes Kerry Emanuel Massachusetts Institute of Technology

Topics Hurricanes are flux-driven phenomena Hurricane intensity is sensitive to rates of transfer of enthalpy and momentum between the atmosphere and ocean Interface tends toward an emulsion at hurricane wind speeds Theory, modeling, lab experiments, and field experiments have led to progress in understanding air-sea interaction at very high wind speeds

Distribution of Entropy in Hurricane Inez, 1966 Source: Hawkins and Imbembo, 1976

Theoretical Upper Bound on Hurricane Maximum Wind Speed: Air-sea enthalpy disequilibrium Surface temperature Outflow temperature Ratio of exchange coefficients of enthalpy and momentum, pertaining to gradient wind

Numerical Experiments Using Reduced Model of Emanuel (1995) but with Dissipative Heating (see talk by Carl Friehe) Note: Coefficients Pertain to Gradient Wind

Hindcast of Katrina Assuming C k =C D

Break in Cumulative Intensity Distribution at wind speeds near 35 m/s potentially explainable by shift in C k and/or C D at that wind speed Wind speed normalized by potential intensity calculated assuming that C k =C D

Sea Spray

Nondimensional Control Parameters:

Similarity Hypothesis: All quantities become independent of molecular properties in limit of large R u Sea surface becomes self-similar, with all length scales scaling as u* 2 /g Nondimensional coefficients become constant

Mechanistic argument from Emanuel (2003):

Note that the previous development pertains to coefficients that operate on the gradient wind. The similarity theory predicts that the wind u at a fixed altitude z should scale as where G is some function. Depending on the form of G, u * can be a multi-valued function of u for some range of altitude z. See talk by Ed Andreas this afternoon!!

Results from 2003 CBLAST Experiment FabianIsabel Work of Michael Bell, PhD Dissertation, Naval Postgraduate School, 2010

Absolute Angular Momentum and Total Energy Structure IsabelFabian (Color)(Contour)

Budget Control Volumes Bottom 0 & 100 m; Top 400 – 1000 m; Width 10 – 22 km Aspect Ratio 20 – 30Inner Radius 0.8 +/- 2 km = 72 retrievals * 6 missions = 432 total samples

Tangential Reynolds Stress and Enthalpy Flux

Prev Coefficients CDCD CKCK CKCDCKCD Large and Pond 1982 DeCosmo et al Black et al Drennan et al French et al Zhang et al Haus et al Bell 2010 Large and Pond 1981 Donelan et al Black et al French et al Powell et al Vickery et al Bell 2010

Summary Hurricanes are driven by surface enthalpy fluxes and retarded by surface drag Sea surface becomes emulsion-like at hurricane wind speeds Fluxes through such an emulsion constitute a challenging problem for theory, numerical experiments, lab experiments, and field programs

Formulating fluxes in terms of 10-m winds may be ill-posed (see talk by Ed Andreas) Results of field and laboratory experiments suggest little change in flux coefficients through whole range of wind speeds, but error bars still large