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Chapter 4 Convective Dynamics Photographs © Todd Lindley

Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

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Page 1: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Chapter 4 Convective Dynamics

Photographs ©  Todd Lindley

Page 2: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Textbook materials for reading

• Bluestein Vol II p 445-462• Holton p.287 – 303• Houze 268 – 295• (more later when we get into squall lines

and supercells)

Page 3: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

4.1. Introduction

• Issues with Thunderstorms / Convection Types of storms Necessary conditions for them Large-scale organization of Feedback to environment Dynamics of Factors that control movement and rotation Prediction of

Page 4: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Thunderstorms• Definition: A thunderstorm is a local storm, invariably

produced by a cumulonimbus cloud, that always is accompanied by lightning and thunder.  It usually contains strong gusts of wind, heavy rain, and sometimes hail. 

• We often use the word "convection" to describe such storms in a general manner, though the term convection specifically refers to the motion of a fluid resulting in the transport and mixing of properties of the fluid.  To be more precise, a convective cloud is one which owes its vertical development, and possibly its origin, to convection (upward air currents).

Page 5: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Modes of Convection / Storm Classification

• Although a continuous spectrum of storms exists, meteorologists find it convenient to classify storms into specific categories according to their structure, intensity, environments in which they form, and weather produced. 

Page 6: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley
Page 7: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley
Page 8: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

The most basic classification includes: • Single-cell or air-mass storm Typically last 20-30 minutes. Pulse storms can

produce severe weather elements such as downbursts, hail, some heavy rainfall and occasionally weak tornadoes.

• Multicell cluster storm A group of cells moving as a single unit, with each cell in a different stage of the thunderstorm life cycle. Multicell storms can produce moderate size hail, flash floods and weak tornadoes.

• Multicell Line (squall line) Storms - consist of a line of storms with a continuous, well developed gust front at the leading edge of the line. Also known as squall lines, these storms can produce small to moderate size hail, occasional flash floods and weak tornadoes.

• Supercells Defined as a thunderstorm with a rotating updraft, these storms can produce strong downbursts, large hail, occasional flash floods and weak to violent tornadoes.

Page 9: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

4.2 Ordinary or "air-mass“ storm • 4.2.1. Main Characteristics

Consists of a single cell (updraft/downdraft pair)

Forms in environment characterized by large conditional instability and weak vertical shear

Vertically erect built-in self-destruction mechanism

Can produce strong straight-line winds or microburst

Life cycle is generally < 1 hour, usually 30-45 min

These storms form in weakly-forced environments, and are driven primary by convective instability rather than the ambient winds

They are some times called "air-mass" storm because they form within air-masses with more-or-less horizontal homogeneity

Page 10: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

This is a single cell storm, looking east from about 15 miles. The storm was moving east (into the photo). Some of the anvil cloud has been left behind the storm, but the greater portion of the anvil is blowing off in advance of the storm and is not observable from this perspective. (May storm in the Texas Panhandle near Amarillo.)

Photograph by: NSSL

Page 11: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

• This late May storm in Oklahoma, looking northeast from about 20 miles, occurred with weak to moderate vertical wind shear. It did not produce any severe weather.

Page 12: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Life cycle of a non-severe single cell storm in weak wind shear

Radar history of the severe pulse storm – often with larger instability

Page 13: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Example of Single-cell Life Cycle

(a) – developing stage

(b) – maturing

(c) Mature stage

(d) – dissipating stage

Page 14: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

4.2.2. Basic Dynamics (forces acting on an air parcel in the vertical)

Perturbation Vertical Momentum Equation (base-state hydrostatic equations has been

subtracted off on the RHS)

where L = liquid+ice water content. Note that the water vapor contributes to the buoyancy of air parcel and the combined effect can be expressed in terms of virtual potential temperature

Page 15: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Three stages of single-cell storm development

Towering stage Mature Stage Dissipating Stage

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LCL – Lifting condensation level

LFC – Level of freeconvection – level atwhich the parcel is warmer than theEnvironment

EL – Equilibrium Level – level at which the parcel’s T becomesthe same as the environment again

Page 17: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Development of Single Cell Storm

Step 1 In the absence of frontal or other forcing, daytime heating of

the PBL causes the convective temperature to be reached. Thus, there is no ‘negative area’ on the skew-T diagram for an air parcel rising from the surface – the lid is broken

Page 18: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Development of Single Cell Storm

Step 2

Updraft forms – once the air reaches the LCL, latent heat is released due to condensation:

- L dqv = Cp dT

For every 1g/kg of water condensed, the atmosphere warms about 3 degrees. This feeds into the buoyancy term through an increase in ’ (remember earlier vertical momentum equation?). The saturated air parcel ascends following the moist adiabat, along which the equivalent potential temperature e is conserved.

Until the ‘Equilibrium level’ is reached, the air parcel is warmer than the environment, which keeps the buoyancy positive (without the effect of water loading – see later)

Page 19: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Development of Single Cell Storm

Step 2 – continued … When cloud forms, part of it is carried upward by the draft and the

other part falls off the updraft. The ‘weight’ of this liquid water makes the air parcel heavier, this ‘water loading’ effect acts to reduce the positive buoyancy.

B = g(’g L

10 x 3/300 ~ - 10 x 0.01 kg/kg

Therefore 10 g/kg of cloud or rain water will offset 3 K temperature surplus.

Page 20: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Development and decay of Single Cell Storm

• When the cloud grows to a stage that the updraft becomes too ‘heavy’ because of water loading, it will collapse, updraft then turns into downdraft.

• Another important process that contributes to the collapse is the evaporative cooling. When cloud grows, cloud droplets turn into larger rain drops that fall out of the updraft, reaching the lower level where the air is sub-saturated. The rain drops will partially evaporate in this sub-saturated air, producing evaporative cooling. This cooling enhances the downdraft.

• In the absence of vertical wind shear, the cell is upright, this downdraft would then disrupt the low-level updraft, causing the cell to dissipate. This is the built-in self-destruction mechanism mentioned earlier

• The cold downdraft sometimes form a cold pool that propagates away from the cell above, further removing the lifting underneath the cell

Page 21: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

The effect of pressure gradient force• In addition to buoyancy force and water loading, another force that is also

acting on the rising parcel is the vertical pressure gradient force (PGF)

• When an air parcel rises (due to buoyancy), it has to push off air above it, creating higher pressure (positive p’) above (imagine pushing yourself through a crowd)

• Below the rising parcel, a void is created (imagine a vacuum cleaner), leading to lower pressure at the cloud base

H

L

PGF

Page 22: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Effect of Pressure Gradient Force

• The higher pressure above will push air to the side, making room for the rising parcel, while the lower pressure below attracts surrounding air to compensate for the displaced parcel

• Such a positive-negative pattern of p perturbation creates a downward pressure gradient. The PGF force therefore opposes the buoyancy force, therefore acts to reduce the net upward forcing.

Page 23: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Effect of Pressure Gradient Force

• The degree of opposition to the buoyancy force depends on the aspect ratio of the cloud (L/H), or more accurately of the updraft

• The effect is larger for wider/large aspect-ratio cloud, and weaker for narrower/small aspect ratio cloud, because

For narrow cloud, a small amount of air has to be displaced/attracted by the rising parcel, therefore the p perturbation needed to achieve this is smaller, so that the opposing pressure gradient is smaller (often <<buoyancy) so a narrow cloud can grow faster

PGF is stronger for wider clouds, as a results, the net upward force (buoyancy – PGF) is significantly reduced, the cloud can only grow slowly. When B and PGF has similar magnitude, the vertical motion becomes quasi-hydrostatic – this is typical of large scale broad ascent.

• Dynamic stability analysis of inviscid flow shows that the infinitely narrow clouds grow the fastest, but in reality, the presence of turbulent mixing prevents the cloud from becoming too narrow, hence the typical aspect ratio of clouds is 1.

Page 24: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Skew-T analysis and Parcel Theory

• Skew-T analysis and Parcel Theory typically neglect the effect of PGF induced by vertical motion, essentially they assume that the environment is unchanged by the parcel motion. They also neglect the effect of mixing/friction

• Therefore, parcel theory tends to overestimate the intensity of updraft. Sill, it provides a useful upper-limit for the convection intensity

Page 25: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Convective Available Potential Energy (CAPE)

• CAPE measures the amount of convective instability, or more accurately the potential energy of an environmental sounding – the energy that can be converted into kinetic energy when an air parcel rises from LFC to EL

• It is based on the simple parcel theory which neglects the effect of mixing/friction, PGF and sometimes water loading.

• From CAPE, we can estimate the maximum vertical velocity that can be reached by a parcel

Page 26: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

CAPE dt

Page 27: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

Skew-T• The ‘negative’ area is equal

to CIN(Convective Inhibition)

• The positive area (where air parcel is warmer than environment) is equal to CAPE

• Lifted Index – temperature excess in 500mb environment over that of a parcel lifted from the low ‘moist’ layer (negative value indicates instability)

Page 28: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

ARPS Simulation of a Single Cell Storm

• May 20, 1977 Del City Supercell Storm Sounding – used without environmental wind

Page 29: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

ARPS Simulation of a Single Cell Storm

T-equivalent buoyancy+qw+ref Eq. Pot. Temp.+qw+Ref+wind t=0

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ARPS Simulation of a Single Cell Storm

T-equivalent buoyancy+qw+ref Eq. Pot. Temp.+qw+Ref+wind t=15min

Page 31: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

ARPS Simulation of a Single Cell Storm

T-equivalent buoyancy+qw+ref Eq. Pot. Temp.+qw+Ref+wind t=20min

Page 32: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

ARPS Simulation of a Single Cell Storm

T-equivalent buoyancy+qw+ref Eq. Pot. Temp.+qw+Ref+wind t=25min

Page 33: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

ARPS Simulation of a Single Cell Storm

T-equivalent buoyancy+qw+ref Eq. Pot. Temp.+qw+Ref+wind t=30min

Page 34: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

ARPS Simulation of a Single Cell Storm

T-equivalent buoyancy+qw+ref Eq. Pot. Temp.+qw+Ref+wind t=45min

Page 35: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

ARPS Simulation of a Single Cell Storm

Perturbation Pressure +qw+ref +wind t=0, 15min

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ARPS Simulation of a Single Cell Storm

Perturbation Pressure +qw+ref +wind t=20, 25min

Page 37: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

ARPS Simulation of a Single Cell Storm

Perturbation Pressure +qw+ref +wind t=30, 45min

Page 38: Chapter 4 Convective Dynamics Photographs © Todd LindleyTodd Lindley

ARPS Simulation of a Single Cell Storm

Perturbation Pressure +qw+ref +wind t=45min

High pressure is seen undernearth the cold pool. Gust front circulation produces strong lifting.