2014
DOI: 10.1002/2013ms000278
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Balanced dynamics of deep and shallow Hadley circulations in the tropics

Abstract: This paper examines the dynamics of large-scale overturning circulations in the tropical atmosphere using an idealized zonally symmetric model on the equatorial b-plane. Under certain simplifications of its coefficients, the elliptic partial differential equation for the transverse circulation can be solved by first performing a vertical transform to obtain a horizontal structure equation, and then using Green's function to solve the horizontal structure equation. When deep diabatic heating is present in the I… Show more

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Cited by 9 publications
(27 citation statements)
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References 46 publications
(69 reference statements)
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“…More specifically, the inertia‐gravity wave amplitude peaks when (y1+y2)/21150 km and 950 km in the southern and northern cell, respectively. These ITCZ locations nearly coincide with the ITCZ location where there is the maximum asymmetry between the southern and northern Hadley cells [ Hack et al ., ; Gonzalez and Mora Rojas , ]. Also, the inertia‐gravity waves in the southern cell are about twice as large in amplitude as those in the northern cell, similar to the time average asymmetry between the two cells.…”
Section: Examples Using Single Vertical Mode Diabatic Heatingmentioning
confidence: 93%
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“…More specifically, the inertia‐gravity wave amplitude peaks when (y1+y2)/21150 km and 950 km in the southern and northern cell, respectively. These ITCZ locations nearly coincide with the ITCZ location where there is the maximum asymmetry between the southern and northern Hadley cells [ Hack et al ., ; Gonzalez and Mora Rojas , ]. Also, the inertia‐gravity waves in the southern cell are about twice as large in amplitude as those in the northern cell, similar to the time average asymmetry between the two cells.…”
Section: Examples Using Single Vertical Mode Diabatic Heatingmentioning
confidence: 93%
“…Values of the γ1 parameter in the switch‐on function T(t), presented in the next section, are plotted in the four horizontal dashed lines, γ1=3, 6, 12, 24 h. Notice how γ1=24 h does not intersect with any of the m=0,1,2,3,4 inertia‐gravity wave frequencies. As will be seen later, when diabatic heating is switched on at this slow rate, inertia‐gravity wave activity is minimal and the transient solutions are approximately equal to the balanced solutions derived in Gonzalez and Mora Rojas []. In the next section, we solve (40) and (41) for a particular forcing.…”
Section: Solution Via Hermite Transformsmentioning
confidence: 99%
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