Observations and Modelling of Fronts and Frontogenesis
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 />
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