ess 111 – climate & global change lecture 1 structure of the atmosphere global wind belts

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ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

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Page 1: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

ESS 111 – Climate & Global Change

Lecture 1

Structure of the Atmosphere

Global Wind Belts

Page 2: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Where is the atmosphere?

Everywhere!Completely surrounds EarthHeld to Earth by gravitational attraction

Page 3: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

What makes up the atmosphere?

Page 4: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Water Vapor

Location of this in the atmosphere is highly variable Significantly influences climate & weather

How?

Page 5: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Atmospheric Thickness

No defined top to the atmosphereThe atmosphere is very shallow—and is less than 2% of the Earth’s thickness

Over 90% ofatmosphere inthe lowest 16km& is where nearlyall weather occurs

Page 6: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Temperature Basics Temperature – measure of average kinetic energy (motion) of individual molecules in matterThree temperature scales (units): Kelvin (K), Celsius (C), Fahrenheit (F)

All scales are relative

degrees F = 9⁄5 degrees C + 32degrees K = degrees C + 273.15

Page 7: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Temperature Layers

Due to surface heating (Longwave, Latent heat, Sensible heat)

Due to ozone absorption of sunlight

Due to Solar winds, Cosmic rays

Temperature decreases with height in the Troposphere

Page 8: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Density & Pressure

Page 9: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Density & Pressure

Lower layers of atmosphere are compressed by air above it

This compression increases pressure & density of the lower layers of the atmosphere

Page 10: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

What is atmospheric pressure?

Weight of the overlying airTaller the column of air above an object, the greater the air pressure exerted on that object

Page 11: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Standard Atmospheric Pressure

1013.25 mb1013.25 hPa29.92 inches of Hg

Page 12: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

The Layers of the Atmosphere

Thermosphere

Page 13: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Troposphere

Lowest region of the atmosphereContains ½ of the Earth’s atmosphere

density density

Page 14: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Troposphere

Page 15: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Depth of tropopauseBetween the Troposphere & Stratosphere is the tropopauseHeight is variable – Thermal expansion & contraction

Page 16: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

How do we determine where the tropopause is located?

Page 17: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts
Page 18: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Stratosphere

Temperature increases with an increase in altitude

What is this called?

Page 19: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Why is there a temperature inversion in the stratosphere?

Temp Inversion – temperature warms with height instead of cooling w/ heightOzone

Gas that absorbs ultraviolet (UV) solar energyIncreases the temperature of the air surrounds ozone

Page 20: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Mesosphere

Temperature decreases with an increase in altitudeWhere meteors burn up while entering the Earth’s atmosphere

Page 21: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Thermosphere

First exposed to the Sun's radiation and so is first heated by the Sun

Air is so thin that a small increase in energy can cause a large increase in temperature

Page 22: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Vertical Structure of the Atmosphere

Page 23: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Space shuttle Endeavour straddles mesosphere & stratosphere

Page 24: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Planetary WindsWell-defined pressure patterns exist across the Earth that induce the global wind patterns on the planet

Page 25: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Idealized Single-Cell Convection Model for a Planet

Features of the circulation pattern:

•horse latitude•trade winds•doldrums•prevailing westerlies•polar easterlies•polar front

Page 26: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

The Three-Cell Model

Intertropical convergence zone (ITCZ) -- surface low pressure with clouds and rain

Subtropical high -- Air subsides (dry climate)

Hadley cell -- tropical convection cell

Ferrel cell -- southwesterly winds at surface

Polar cell -- northeasterly winds at surface

Page 27: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Observed Distribution of Pressure and Winds

(a) An imaginary uniform Earth with idealized zonal (continuous) pressure belts

(b) Actual planetary winds belts on Earth taking into account continents and ocean currents

Page 28: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Equatorial Low- warm air rising creates cell of low pressure.

Intertropical Convergence Zone (ITCZ)- referred to as the convergence zone because this region is where the trade winds converge. Ascending air leads to cloud formation which makes thisregion clearly visible on satellite imagery.

Subtropical Highs- These zones are caused primarily by Coriolis deflection which restricts upper-level winds from moving poleward.Subsiding air and divergent winds at the surface cause warm, cloud-free weather (many large desert areas are located along this latitudinal belt). Subtropical Highs tend to persist throughout the year, with the center of the high migrating, and are regarded as semi-permanent pressure systems.

Idealized Pressure Belts

Page 29: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Idealized Pressure Belts (cont.)

Subpolar Low – located around 50 to 60 latitude. Associated with the polar front. The belt of low pressure is formed by theinteraction (convergence) of the polar easterlies and the westerlies

Polar Highs – located over the poles! The process which producesthe polar highs is different than the process which produces thesubtropical highs. Surface cooling is the principle reason the polar high.

Page 30: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

The ITCZ is a band of clouds across the tropics

ITCZ

Page 31: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

The three-celled model vs. reality:

• Hadley cells are close approximations of real world equatorial winds

• Ferrel and polar cells do not approximate the real world winds very well at all

• Model is unrepresentative of westerly flow aloft

• Continents and topographic irregularities cause significant variations in real world wind patterns compared to the model

Page 32: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Semi-Permanent Pressure Cells are large areas of higher or lower atmospheric pressure than the surface average

They may be thermally induced (rising warm air or subsiding cold air) or they may be caused dynamically by converging or diverging wind patterns)

They fluctuate seasonally

Northern hemisphere semi-permanent cellsThe Aleutian, Icelandic, and Tibetan lows

Siberian, Hawaiian, and Bermuda-Azores highs

ITCZ (low)

Page 33: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Vertical structure and mechanisms

Hadley Cell (thermal): Heating in tropics forms surface low and upper level high air converges equatorward at surface, rises, and diverges poleward aloft descends in the subtropics

Ferrel Cell (dynamical): Dynamical response to Hadley and polar cells

Polar Cell (thermal): Driven by heating at 50 degree latitude and cooling at the poles

Page 34: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Average atmospheric air pressure and wind patterns in January

Page 35: ESS 111 – Climate & Global Change Lecture 1 Structure of the Atmosphere Global Wind Belts

Average atmospheric air pressure and wind patterns in July