Transcript Document

Overview of Tropical Cyclones
AOS 453
April 2004
J. P. Kossin
CIMSS/UW-Madison
HOT

COOLER
Genesis:
Easterly waves  African easterly jet  hot Sahara vs cool temps
along coast of Gulf of Guinea coast  reversal of meridional PV
gradient  combined barotropic-baroclinic instability.
April-October. Period ~ 3-4 days.  ~ 2000-2500 km. N ~ 60/year.
Genesis: may also be instigated by local baroclinic or upper-level
trough forcing; along southermost remnants of fronts. Or perhaps
through barotropic instability of ITCZ (Ferreira and Schubert 1997).
Persistent convection diabatically produces PV and forms Mesoscale
Convective Vortices (MCV) in the mid-levels. Multiple vortices are
formed within tropical cloud clusters.
Mid-level vortex  cold-core system (tangential wind increases
with height).
Tropical cyclone  warm-core. How does the conversion occur?
Modified Rossby-Burger-Prandtl relationship:
Vertical influence  D = (flocal  a)1/2 L / N
Merger (self organization)
Environmental requirements (necessary conditions) for genesis:
1) Warm water [SST > 26.5C (80F)]
2) Low vertical wind shear (~10m/s bottom to top)
3) Ambient rotation ( f ) - off equator.
4) Moist mid-levels.
Surface swirling flow  How does disturbance amplify?
Intensification:
Conditional Instability of the Second Kind (CISK) has fallen out of
favor. Convergence related mechanism. Downdrafts kill moist energy
of boundary layer. Convergence is inefficient at raising air to LFC.
Wind Induced Surface Heat Exchange (WISHE).
Real CISK
•
Scale-dependent feedback from cumulus to system by:
1.
2.
•
momentum forcing
thermal forcing
Response of system to cumulus:
1.
2.
Thermal field (mass) adjusts to momentum forcing (L<LR ,
disturbance is smaller than local Rossby radius)
Wind field (momentum) adjusts to thermal (mass) forcing
(L>LR)
Effects of Heating
(Global)
When Q represents the
diabatic latent heat release
of convection, this is
sometimes called
"up moist down dry"
Where does the warming occur? Not so easy.....
Axisymmetric Dynamics
From Hack and Schubert 1986
Local Response to Local Heating; Linear vs. Nonlinear
Efficiency: There is a nonlinear feedback mechanism at
work. The more intense the local swirling flow is, the more
efficiently the heating can warm locally. More local
warming increases pressure gradients which further
intensifies the local flow.
This can be studied in the context of an axisymmetric
balance model (Schubert and Hack 1982).
Heating efficiency as function of inertial stability:
Transverse
Circulation
Warming
Less inertial
stability
More inertial
stability
Schubert and Hack 1982
Real CISK
(continued)
•
•
•
Since the heating of cumulus projects on to multiple
scales on either side of LR, a multiple of responses to
cumulus occur; some gravity and some rotational.
Because the properties of the rotational response are
so different from the gravity wave response, the
evolving system can be complex.
Normally, the system is defined by a slow mesoscale
response that defines the system organization over
time.
Slant-Wise Convection
• Two competing stabilities present in the
atmosphere:
1. Static Stability (vertical planes)
2. Inertial Stability (horizontal planes)
• Stability in one plane limits instability in the other
• Both stabilities are represented by gradients of a
conservative potential
Slant-Wise Convection
(continued)
• There is free movement relative to a
particular stability along iso-lines of
constant potential.
• There is stability induced oscillation for
movement perpendicular to iso-lines of
constant potential.
Slant-Wise Convection
(continued)
• The potential for dry static stability is
potential temperature (q)
• The potential for moist static stability
(saturated air) is equivalent potential
temperature(qe)
• The potential for inertial stability is angular
momentum given by m  ( f   ) y where
y is the radius from the center of rotation.
Slant-Wise Convection
(continued)
• Lines of constant (q) are usually horizontal but dip
downward (due to thermal wind balance) into the
center of a cyclonic vortex whose strength
decreases with height (warm core) and rise
upward into the center of vortex whose strength
increases with height (cold core).
• Lines of constant inertial stability (m) are usually
vertical, but tilt away from the center of a cyclonic
warm core vortex because of the thermal wind
effect and vice versa in a cold core vortex.
Slant-Wise Convection
(continue)
• Hence if we have a saturated warm core vortex, neutral
inertial upward movement (movement along an “m” surface)
experiences less static stability than pure vertical upward
movement .
• Likewise, neutral horizontal movement along a q surface,
experiences less inertial stability than pure horizontal
movement
• If vortex is strong enough momentum lines and q lines can
cross, creating static instability along m surfaces or inertial
instability along q surfaces (isentropes).
Slant-Wise Convection
(continued)
• Hence convection erupting up the tilted
momentum surface is called slant-wise
convection
• Slant-wise convection is due to “symmetric
instability” or inertial instability relative to
the symmetric vortex that defines the radius
of curvature for the momentum lines.
Conditional Symmetric
Instability
• Conditional Instability along a momentum
“m” surface, ie condition for slantwise
moist convection
• Alternative way of looking at the same
thing: Inertial Instability along a theta_e
surface
Tropical cyclone structure:
Axisymmetric Structure as Deduced from
Rawinsonde Composites (Frank 1977)
Axisymmetric Structure as Deduced from Aircraft
Flight-Level Data
Hawkins and Imbembo 1976
Jorgensen 1984
In an average sense, updrafts in t he eyewall tend to flow along
sloping surfaces of constantangular momentum and equivalent
potential temperat ure (moist neutralit y).
Tropical cyclones are warm core systems. Pressure surfaces
become "flatter" (thickness or hypsometric equation), and
tangential winds consequently decrease, with increasing height.
T he pert urbation (or dynamic) pressure at the vort ex center increa
with increasing height . Any resulting subsidence increases the
upward directed buoyancy force just enough t o reestablish a
hydrostatic balance (Smit h 1980).