Impact of interactive sea surface temperature on convective clustering in radiative convective equilibrium
- 1CNRS(Centre national de la recherche scientifique), LMD(Laboratoire de Meteorologie Dynamique ), Paris, France (addisugezahegn@gmail.com)
- 2Abdus Salam International Centre for Theoretical Physics (ICTP), Trieste, Italy
We present results of radiative convective equilibrium runs using the WRF model coupled to an interactive slab ocean model, for which a relaxation term removes energy to constrain the domain mean sea surface temperature to a target value over a given timescale. By using a short adjustment timescale of one minute, drift in the mean temperature is constrained and the impact of the slab ocean is only through the spatial heterogeneity in sea surface flux. We show how thin slabs slow the onset of organization, and conduct sensitivity experiments to determine the relative contributions of the radiative, sensible and latent surface fluxes, with surface fluxes key. Once clustering starts, the surface feedback acts to aid organization onset due to the drying atmosphere, although the speed of clustering onset is not significantly changed, indicating that it could be determined by a water vapour diffusive timescale as suggested by Windmiller and Craig. An additional set of experiments that permit the mean surface temperature to undergo a diurnal adjustment show how diurnal variations in SST oppose the atmospheric radiative forcing and also act to prevent clustering onset. We show the mechanism for this acts through the reduction of the diurnal variation of convective mass flux and the distance between updraft towers.
How to cite: Semie, A. G. and Tompkins, A. M.: Impact of interactive sea surface temperature on convective clustering in radiative convective equilibrium, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-14171, https://doi.org/10.5194/egusphere-egu2020-14171, 2020