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Observations and Modelling of Fronts and Frontogenesis

Observations and Modelling of Fronts and Frontogenesis

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constant pressure c = 4.1x103 J K1- kg1-, <strong>and</strong> thermal<br />

expansibility a = l.7xl04 K-) are,<br />

x Ax'<br />

= (g(p*/p0)h*)l/2/f = 2m0u*/f [100 m], (26b)<br />

t = t*tl, t* = [3300 s = 55 mm], (26c)<br />

(h1,h2,h3,H) =h*(h11,h2',h3',H'),<br />

h* = 2m0u*3/(agQ*/cp) [33 m], (26d)<br />

(ul,u2,u3)=U*(ui',u2',u3'),<br />

(v1,v2,v3) =<br />

(P3 Pl,P3 P2P2 P1) =<br />

= fA* [1 cm s'-], (26e)<br />

u*2/th* [3 cm 1.j,<br />

(26f)<br />

*(aQ*/c)(f/u*2) [3x104 kg m3]. (26g)<br />

The vertical scale h is the Monin-Obukhov length. The<br />

ageostrophic velocity scale V* results from the balance <strong>of</strong><br />

Coriolis force <strong>and</strong> vertical stress divergence, <strong>and</strong> the<br />

geostrophic velocity scale U* from the inertial balance <strong>of</strong><br />

Coriolis force <strong>and</strong> acceleration. The time scale t,i- is chosen<br />

to balance temporal <strong>and</strong> advective rates <strong>of</strong> change. The<br />

density scale p* is suggested by the balance <strong>of</strong> local or<br />

advective heating <strong>and</strong> surface heat flux. The horizontal<br />

length scale * is the internal deformation radius formed<br />

from h* <strong>and</strong> p*. Note that the density <strong>and</strong> horizontal length<br />

scales are small. Much larger density differences <strong>and</strong><br />

horizontal scales 0(1 kg m3, 50 kin) characterize the initial<br />

61

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