Top-down height tendency reasoning is explained and examined. This app
roach uses the assumption of a stratospheric level of insignificant dy
namics (LID)-where height and pressure tendencies are considered negli
gible-to simplify the understanding of cyclone-scale hydrostatic heigh
t (pressure) tendency in the troposphere. Quasigeostrophic analytic mo
del results confirm the existence of such a LID for scales less than a
pproximately 5000 km. An examination of a height tendency equation wit
h the LID assumption shows that there must be net integrated local war
ming (cooling) between the LID and any level below the LID where heigh
ts are falling (rising). The local temperature tendency, which from th
e thermodynamic equation results from advection, diabatic heating, and
the product of vertical motion and static stability, reflects the com
bined actions of all thermodynamic and dynamic processes that together
promote hydrostatic height change in isobaric coordinates. In particu
lar, the important dynamic effects of mass-diverging secondary circula
tions are implicitly contained in the local temperature tendency. New
observational evidence and analytic model simulations supporting the t
op-down approach for understanding height tendency are also provided.
The analytic model simulations show that isolated layers of equivalent
diabatic heating and temperature advection do not produce equivalent
dynamic responses in the vertical-motion field and height tendency fie
lds. This result is used to explain observations that temperature adve
ctions in the upper troposphere/lower stratosphere are associated with
larger lower-tropospheric height tendencies than equivalent temperatu
re advections in the lower troposphere.