lecture 1: introduction to urban atmospheric flows by h.j.s. fernando

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Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

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Page 1: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Lecture 1:

Introduction to Urban Atmospheric Flows

By

H.J.S. Fernando

Page 2: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

The Planet Earth• One of the 1011 planets and stars in our

galaxy (Milky Way), and there are 1011

galaxies in the universe, 4.6 billion years old

• Unique in the sense that it is the only planet so far known to sustain life

• Quite vulnerable as it maintains conditions in narrow bands of properties.

– e.g., water is maintained as a liquid, has a sufficient amount of oxygen, temperature is conducive for life.

– The mass (6 x 1024 kg) and its radius (6400 km) are such that it can keep an atmosphere via gravitation.

• Climate (average atmospheric state over at least a score of years, modulated by seasonal cycles) is fragile

Earth as seen from the TOPEX-POSEIDON satellite (orbits Earth 4700 times/yr and has continuously surveyed ocean currents with radar altimeters since 1992).

World population ~ 6 billion- expanding at a rate ~ 1.5%

Page 3: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Figure 1: Urban and rural population prospects (from the population division of the department of Economic and Social Affairs of the United Nations Secretariat, World Population Prospectus: The 2003 Revision of the World Urbanization Prospects)

Page 4: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Urban Share of World’s Population

Page 5: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Brown Revolution

•Megacities ( >10 M people)

Page 6: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Figure 3: The emergence of Supercities (Source: United Nations, World

Urbanization Prospects, The 1999 Revision)

Supercities ( >5 M people)

Page 7: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Urban Airflow (Meteorology) Studies

Why?• human comfort• energy usage• air quality• security

Governing Factors:

• city’s meteorology

• pollutant emissions and where

• topography

• landuse

Page 8: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

A Rapidly Urbanizing Region: Phoenix

Urban (Latin meaning – City)Definition for Urban - vary

- Sweden and Denmark > 2000- Japan > 2000- USA and Mexico > 2500

Page 9: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Los Angeles, California

Page 10: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Climate System

Page 11: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Urban Ecosystems (Environment)

• Ecosystem - Community of living things interacting with non-living things.

Page 12: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Prediction of Environmental Motions

Mouse Moral: Seeing a part makes a fine tale. Wisdom comes, however, from seeing the whole.(From Nature, Nov. 2000).

(5/5)

Page 13: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Atmospheric Motions

• Thermally driven motions are dominant

Idealized global atmospheric circulation

Page 14: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Global ScaleL ~ 103 - 104 kmT ~ 50 - 100 yrs

Synoptic (Regional Scale)L ~ 1000 km

T ~ days, weeks

Urban ScaleL ~ 10 - 100 km

T ~ 5 - 10 yr; matured~ 1 - 3 yr; rapidly expanding

Rural

NeighborhoodL ~ 0.3 - 10 km

Global ↔ Local• Climate variability• Land cover change• Economic development• Technology & diffusion• Population dynamics

Long range flow

& transport

Regional B.C.

Solutions• Command & control• Market-driven

Air Quality (CO, O3, PM)• Sources (bio & anthro.)• Meteorology (T, v, q)• Solar insolation• B.C.

MesoscaleL ~ 100 km

T ~ hours - day

Urbansecurity

Street CanyonL ~ 10 - 100 m

CBDL ~ 1 - 2 km

PersonalL ~ 1 m

Page 15: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

System Horizontal Scale (km)

Vertical Scale (km)

Time Scale

Global Synoptic

>1000 3 - 10 1-6 months

Regional Macro

500-1000 1-10 1-6 months

Local Climate

1-10 1/100 – 1/10

1 to 24 hrs

Micro-climate

<1/10 <1/100 <24 hrs

Page 16: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Prediction of Environmental Motions

• Schematic diagram of global climate system, to illustrate the way in which the Earth’s atmosphere - ocean system, and land surface area - is divided into thousands of boxes with sides typically extending several hundred kilometers in latitude and longitude, and with heights of a few kilometers in altitude.

• In a general circulation model (GCM), the computer treats each box as a single element as it calculates the evolving global climate.

– The GCM imposes seasonal and latitudinal changes of incoming solar radiation, the height and shape of the continents, and other external conditions which affect the behavior of the atmosphere.

– In GCMs, for example, the equations may be solved in hourly increments over at least 20 years of simulated time to generate an output which is statistically ‘accurate’.

– Such large and time-consuming calculations require the use of best super-computers.

(1/5)

Page 17: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

From Synoptic-scale to Personal-scale

WRF, MM5

(i) Interpolation(ii) CFD

- Full scale (TKE, dissipation…)- Diagnostic way (sparse

observations + conservations laws)

Page 18: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Phoenix Terrain

Diffusion Coefficients

ihi

i

j

j

imji

x

bKbu

x

U

x

UKuu

Page 19: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Horizontal Wind & Topography of Domain 2: 0500 LST Jan 30 – 0500 LST Feb 1

Every hour

Page 20: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

48-hour Urban Simulation

Page 21: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando
Page 22: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Simulation for Oklahoma City

Page 23: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Urban Meteorological Issues

• Terrain (70% are in complex terrain)

• Landuse changes (rapidly growing!)

• Urban heat island

• Transport and Dispersion of Pollutants (Air Quality)

Page 24: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Atmospheric Boundary Layer

ABL - The layer near the ground affected by the presence of the ground

• Drag is important

• Stratification is important

(Stable, Unstable and Neutral)

• Rotation – depending on the view

• Terrain (complex or flat)

Page 25: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Flat Terrain BL

Page 26: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Phoenix ABL

287 288 289 290 291 292 293 294Virtual potential temperature (K)

0

20

40

60

80

100

120

140

160

180

200

220

1641-1644

1657-1701

1721-1724

1738-1741

1756-1800

1814-1817

1835-1838

1856-1900

z(m

)

287 288 289 290 291 292 293 294Virtual potential temperature (K)

0

20

40

60

80

100

120

140

160

180

200

220

1641-1644

1657-1701

1721-1724

1738-1741

1756-1800

1814-1817

1835-1838

1856-1900

287 288 289 290 291 292 293 294Virtual potential temperature (K)

287 288 289 290 291 292 293 294Virtual potential temperature (K)

0

20

40

60

80

100

120

140

160

180

200

220

1641-1644

1657-1701

1721-1724

1738-1741

1756-1800

1814-1817

1835-1838

1856-1900

0

20

40

60

80

100

120

140

160

180

200

220

1641-1644

1657-1701

1721-1724

1738-1741

1756-1800

1814-1817

1835-1838

1856-1900

z(m

)

Page 27: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Mexico City, MexicoComplex Terrain ABL

Image source: NASA Goddard Space Flight Center Scientific Visualization Studio

Page 28: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

An Ideal Complex Terrain

(katabatic)

(anabatic)

Ufp ~1

(synoptic)

Page 29: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Slope Flows

Whiteman 2000

Page 30: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Flows in CT Urban AirshedsSynoptic Flow

Thermal circulation

Page 31: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33

0

2

4

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Win

d s

pee

d,

m/s

14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33

0

90

180

270

360

Win

d d

irec

tio

n,

deg

14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33Julian Days, 1998

5

10

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Air

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(b)

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14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33

0

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Win

d s

pee

d,

m/s

14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33

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Win

d d

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14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33Julian Days, 1998

5

10

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tem

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Winds in Phoenix – Little synoptic, sloshing

Page 32: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Pollution in Complex Terrain

Phoenix

Los Angeles

Salt Lake City

Hong Kong

Page 33: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Chemical Spills

From the Arizona Republic

Page 34: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Experimental Modeling of the Cold Pool Destruction

Page 35: Lecture 1: Introduction to Urban Atmospheric Flows By H.J.S. Fernando

Cold Pool BreakupLow B

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