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Axisymmetric constraints on cross-equatorial Hadley cell extent
We consider the relevance of known constraints from each of Hide's theorem,
the angular momentum conserving (AMC) model, and the equal-area model on the
extent of cross-equatorial Hadley cells. These theories respectively posit that
a Hadley circulation must span: all latitudes where the radiative convective
equilibrium (RCE) absolute angular momentum () satisfies
or or where the RCE absolute
vorticity () satisfies ; all latitudes
where the RCE zonal wind exceeds the AMC zonal wind; and over a range such that
depth-averaged potential temperature is continuous and that energy is
conserved. The AMC model requires knowledge of the ascent latitude
, which need not equal the RCE forcing maximum latitude
. Whatever the value of , we
demonstrate that an AMC cell must extend at least as far into the winter
hemisphere as the summer hemisphere. The equal-area model predicts
, always placing it poleward of . As
is moved poleward (at a given thermal Rossby number), the
equal-area predicted Hadley circulation becomes implausibly large, while both
and become increasingly displaced
poleward of the minimal cell extent based on Hide's theorem (i.e. of
supercritical forcing). In an idealized dry general circulation model,
cross-equatorial Hadley cells are generated, some spanning nearly pole-to-pole.
All homogenize angular momentum imperfectly, are roughly symmetric in extent
about the equator, and appear in extent controlled by the span of supercritical
forcing.Comment: 18 pages, 9 figures, publishe
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Axisymmetric Hadley Cell Theory with a Fixed Tropopause Temperature Rather than Height
Axisymmetric Hadley cell theory has traditionally assumed that the tropopause height (H_t) is uniform and unchanged from its radiative–convective equilibrium (RCE) value by the cells’ emergence. Recent studies suggest that the tropopause temperature (T_t), not height, is nearly invariant in RCE, which would require appreciable meridional variations in H_t. Here, we derive modified expressions of axisymmetric theory by assuming a fixed T_t and compare the results to their fixed-H_t counterparts. If T_t and the depth-averaged lapse rate are meridionally uniform, then at each latitude H_t varies linearly with the local surface temperature, altering the diagnosed gradient-balanced zonal wind at the tropopause appreciably (up to tens of meters per second) but the minimal Hadley cell extent predicted by Hide’s theorem only weakly (≲1°) under standard annual-mean and solsticial forcings. A uniform T_t alters the thermal field required to generate an angular-momentum-conserving Hadley circulation, but these changes and the resulting changes to the equal-area model solutions for the cell edges again are modest (<10%). In numerical simulations of latitude-by-latitude RCE under annual-mean forcing using a single-column model, assuming a uniform T_t is reasonably accurate up to the midlatitudes, and the Hide’s theorem metrics are again qualitatively insensitive to the tropopause definition. However imperfectly axisymmetric theory portrays the Hadley cells in Earth’s macroturbulent atmosphere, evidently its treatment of the tropopause is not an important error source
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