Abstract

Although in general the sea breeze can be considered as a mesoscale atmospheric circulation, the sea-breeze front has a much smaller scale. Simulation of the development of a sea-breeze front should therefore be preferably done with a non-hydrostatic model, with high spatial resolution (grid distances of a few hundred meters). Here we describe an attempt to do this. We conducted a few numerical experiments to study in an explicit way the effect of convective cloud formation on the evolution of the sea-breeze front. The model used is a 2-D cloud model, applied to a domain 60 km long and almost 4 km high, with a resolution of 250 m. Integrations were carried out over 4 h of simulated time. We found that even with only a weak offshore background wind (1 m/s), the sea breeze rapidly takes on the form of a gravity current with a well-developed head. A comparison of runs with and without cloud simulation revealed that the formation of clouds tends to strengthen the sea breeze. The reason is that convective clouds form over land or just above the sea-breeze front, and dissipate at the seaward side of the front. The net effect is an additional horizontal gradient in diabatic heating.

Highlights

  • The sea-breeze circulation is a rather pure type of a thermally-driven circulation in the atmosphere, and it has been observed and studied for quite a long time

  • In particular Walsh (1974) showed that a linear model of sufficient spatial resolution is able to recover the essential features of a sea-breeze circulation, even for different background situations

  • The offshore background wind is weak, the simulated sea-breeze circulation rapidly takes on the form of a typical gravity current

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Summary

Introduction

The sea-breeze circulation is a rather pure type of a thermally-driven circulation in the atmosphere, and it has been observed and studied for quite a long time. A well-developed sea-breeze circulation is characterized by two horizontal length scales, namely, the scale of the circulation cell and the scale of the front This has some inplications for the type of models to be used for numerical simulation. It is tempting to assume that in this case the convective clouds help to strengthen the front In view of these considerations, we made an attempt to simulate the sea-breeze front by acloud model', i.e. a high-resolution numerical model of. When the cold air overlying the sea starts to move inland, a situation occurs where organized motion (a gravity current) encounters an essentially turbulent motion field This point should be kept in mind when comparing our flow patterns to the smooth velocity fields obtained in earlier numerical studies of the sea breeze. We carried out integrations over 4 h of simulated time, which appears to be long enough to study the formation and migration of the sea-breeze front

Model description
The numerical experiment
Findings
Conclusions and discussion
Full Text
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