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Observed and Projected Ocean Wind Speed Trends and Marine Boundary - PowerPoint PPT Presentation

Observed and Projected Ocean Wind Speed Trends and Marine Boundary Layer Clouds Jan Kazil and Graham Feingold Annual mean 10 m wind speed trend 1991 - 2008 +1.5 % +1.0 % +0.5 % 0 % -0.5 % -1.0 % -1.5 % Young et al. (Nature, 2011)


  1. Observed and Projected Ocean Wind Speed Trends and Marine Boundary Layer Clouds Jan Kazil and Graham Feingold

  2. Annual mean 10 m wind speed trend 1991 - 2008 +1.5 % +1.0 % +0.5 % 0 % -0.5 % -1.0 % -1.5 % Young et al. (Nature, 2011)  Satellite radar altimeter  Wave height  10 m wind speed

  3. JJA 10 m wind speed in 2081–2100 relative to 1981–2000 -10% -5% 0% 5% 10% McInnes et al. (Atm. Sci. Lett., 2011)  WCRP CMIP3 model mean  19 coupled climate models  A1B emission scenario

  4. Wind speed Drives Increases Moistens the Warms the non-thermal CCN number boundary boundary turbulence, layer layer shear Horizontal Latent heat Sensible heat Sea spray momentum

  5. Simulations – WRF North-east Pacific  DYCOMS II RF02  Different domain sizes and resolutions South-east Pacific  VOCALS RF14  Different domain sizes and resolutions Geostrophic wind speed:  Fast (average + 25 %) All else equal  Average (observations)  Slow (average – 25 %)

  6. Cloud field VOCALS (after 12 h) DYCOMS II (after 6 h) +18 % Response? -18 %

  7. Net down-welling radiation DYCOMS II RF02 VOCALS RF14 +6.3 W m -2 Faster wind +4.83 W m -2 -0.99 W m -2 Slower wind -5.83 W m -2

  8. Decoupling due to wind shear? More entrainment Shear Water vapor gradient Less latent heat u resolved (m s -1 ) Cloud water (g kg -1 ) Water vapor (g kg -1 ) Θ l (K)

  9. Two different decoupling mechanisms at play? DYCOMS II RF02 VOCALS RF14

  10. Wind speed effects on non-precipitating Sc  Faster wind speed → higher radiative forcing  Slower wind speed → reduced radiative forcing Different decoupling mechanisms depending on boundary layer depth? ● Faster wind speed → Stronger wind shear at inversion → more entrainment → decoupling ● Faster wind speed → Stronger latent heat flux → stronger drizzle → humidification of sub- cloud layer → decoupling

  11. Path forward ● Simulations with higher resolution ● Isolate effect of different mechanisms ● Analyze observations for wind speed effects: MAGIC!

  12. Response to wind speed (VOCALS RF14)

  13. Response to wind speed (DYCOMS II RF02)

  14. Asymmetric response due to solar heating  Faster wind speed → more decoupling  Slower wind speed → less decoupling  Solar heating adds to decoupling in both cases

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