AMS Weather Studies

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AMS Weather Studies

Introduction to Atmospheric Science, 5

th

Edition

Chapter 4

Heat, Temperature, &

Atmospheric Circulation

© AMS

Driving Question

What are the causes and consequences of heat transfer within the Earth-atmosphere system?

This chapter covers:

Distinguishing temperature and heat

Heat transfer processes

Thermal response and specific heat

Heat imbalances

How does heat affect atmospheric circulation?

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Case-in-Point

Extreme Heat of Death Valley, CA

Death Valley – Hottest and driest place in North America

134°F in 1913

2nd highest temperature ever recorded on Earth

Summer 1996

40 successive days over 120°F

105 successive days over 110°F

Causes:

Topographic setting

Atmospheric circulation

Intense solar radiation

Cooperative Weather observing station at Furnace Creek Ranch

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Distinguishing Temperature & Heat

All matter is composed of molecules or particles in continual vibrational, rotational, and/or translational motion.

Energy represented by this motion is called kinetic energy.

Temperature

Directly proportional to the average kinetic energy of atoms or molecules composing a substance

Internal energy

Encompasses all the energy in a substance

Includes kinetic energy

Includes potential energy, arising from forces between atoms/molecules

Heat is energy in transit

When two substances are brought together with different kinetic energy, energy is always transferred from warmer object to colder

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Distinguishing Temperature & Heat

5

Temperature Scales

Absolute zero

Temperature at which theoretically all molecular motion ceases

No electromagnetic radiation is emitted

Absolute zero

= -459.67

° F

= 273.15

° C

= 0 K

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Distinguishing Temperature & Heat

Temperature scales measure degree of hotness or coldness

Calorie

Amount of heat required to raise temperature of 1 gram of water 1 Celsius degree

Different from “food” calorie, which is actually 1 kilocalorie

Joule

More common in meteorology today

1 calorie = 4.1868 joules

British Thermal Units (BTU)

Amount of energy required to raise 1 pound of water 1 Fahrenheit degree

1 BTU = 252 cal = 1055 J

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Distinguishing

Temperature & Heat

Liquid-in-glass thermometer

Thermometer

Liquid-in-glass thermometer

Uses mercury or alcohol

Bimetallic thermometer

Two strips of metal with different expansion/contraction rates

Electrical resistance thermometer

Thermograph

Measures and records temperature

The change of temperature during the passage of a cold front as determined by an electronic thermometer.

Bilmetallic thermometer

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Distinguishing Temperature & Heat

Shielding temperature sensors

Important properties

Accuracy

Response time

Location is important

Ventilated

Shielded from weather

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Enclosure for the NWS electronic temperature sensor

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Heat Transfer Processes

Temperature gradient

Change in temperature over distance

Example: the hot equator and cold poles

Heat flows in response to a temperature gradient

This is the 2 nd law of thermodynamics

Heat flows toward lower temperature so as to eliminate the gradient

Heat flows/transfers in the atmosphere

Radiation

Conduction

Convection

Latent heat – phase changes in water

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Heat Transfer Processes

Radiation

Both a form of energy and a means of energy transfer

Occurs even in a vacuum, such as space

Absorption of radiation by an object causes the temperature of object to rise

Converts electromagnetic energy to heat

Radiational heating

Absorption at greater rate than emission

Radiational cooling

Emission at greater rate than absorption

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Heat Transfer Processes

Conduction

Transfer of kinetic energy of atoms or molecules by collision between neighboring atoms or molecules

Heat conductivity

Rate of heat transport across an area to a temperature gradient

Some materials have a higher heat conductivity than others

Solids (metal) are better conductors than liquids

Liquids are better than gases (air)

Conductivity impaired by trapped air

Examples: fiberglass insulation, thick layer of fresh snow

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Heat Transfer Processes

A thick layer of snow is a good insulator because of air trapped between individual snowflakes.

As snow settles, the snow cover’s insulating property diminishes.

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Heat Transfer Processes

Convection

Consequence of differences in air density

Transport of heat within a substance via movement of substance itself

Substance must liquid or gas

Very important process for transferring heat in atmosphere

The convection cycle

Ascending warm air expands, cools and eventually sinks back to ground

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Heat Transfer Processes

Latent heating

Movement of heat from one location to another due to phase changes of water

Example: evaporation of water, movement of vapor by winds, condensation elsewhere

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Thermal Response and Specific Heat

Temperature change caused by input/output of a quantity of heat varies among substances

Specific heat

The amount of heat required to raise 1 gram of a substance

1 Celsius degree

The contrast in specific heat is one reason why the sand is hotter than the water.

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Thermal Response and Specific Heat

Thermal inertia

Resistance to a change in temperature

Large body of water exhibits greater resistance to temperature change than land because of difference in specific heat

Maritime climate

Immediately downwind of the ocean experience much less annual temperature change

Continental climate

Locations well inland experience greater annual temperature change 16

San Francisco, CA, has a maritime climate while

St. Louis, MO, has a continental climate.

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Heat Imbalance:

Atmosphere vs. Earth’s Surface

At Earth’s surface

Absorption of solar radiation is greater than emission of IR

In atmosphere

Emission of IR radiation to space is greater than absorption of solar radiation

Therefore,

Earth’s surface has net radiational heating

Atmosphere has net radiational cooling.

So, Earth’s surface transfers heat to the atmosphere, making up difference

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Heat Imbalance:

Atmosphere vs. Earth’s Surface

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Heat Imbalance:

Atmosphere vs. Earth’s Surface

Latent Heating

Some absorbed solar radiation used to vaporize water at Earth’s surface.

Energy released to the atmosphere when clouds form

Comparatively, large amounts of heat needed for phase changes of water

Sensible Heating

Heat transfer via conduction and convection that can be sensed by temperature change and measured by a thermometer

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Heat Imbalance:

Atmosphere vs. Earth’s Surface

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Heat Imbalance:

Atmosphere vs. Earth’s Surface

Sensible heating, in the form of convectional uplifts, can combine with latent heating, through condensation, to channel heat from Earth’s surface into the troposphere

Produces cumulus clouds

If it continues vertically, cumulonimbus clouds form

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Heat Imbalance:

Atmosphere vs. Earth’s Surface

Bowen Ratio

Describes how energy received at the Earth’s surface is partitioned between sensible heating and latent heating

Bowen ratio =

[(sensible heating)/(latent heating)]

At the global scale, this is

[(7 units)/(23 units)] = 0.3

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Surface energy budget through the course of a year at

Yuma, AZ and Madison, WI.

R = net radiation absorbed

H = sensible heating

LE = latent heating

G = storage

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Heat Imbalance: Tropics vs.

Middle and High Latitudes

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Earth’s surface unevenly heated due to higher solar altitudes in the tropics than higher latitudes

Causes a temperature gradient, resulting in heat transfer

Poleward heat transport

Air mass exchange

Storms

Ocean currents

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Heat Imbalance: Tropics vs.

Middle and High Latitudes

Heat transport by air mass exchange

North-south exchange of air masses transports sensible heat from the tropics into middle and high latitudes

Air mass properties of depend on source region

Modify as they move

Heat transport by storms

Tropical storms and hurricanes are greater contributors to poleward heat transport than middle latitude cyclones

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Heat Imbalance: Tropics vs.

Middle and High Latitudes

The Gulf Stream flows along the East Coast from Florida to the Delaware coast.

Heat transport by ocean circulation

Contributes via wind-driven surface

27 currents and thermohaline circulation

Thermohaline circulation is densitydriven movement of water masses

Transports heat energy, salt, and dissolved gases over great distances and depths

Meridional overturning circulation

(MOC)

At high latitudes, surface waters cool and sink, then flow southward as cold bottom water

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Why Weather?

Imbalances in radiational heating/cooling create temperature gradients

Earth’s surface the troposphere

Low and high latitudes

Heat transported in the Earth-atmosphere system to reduce temperature differences

Cause-and-effect chain starts with the Sun, ends with weather

Some solar radiation is absorbed (converted to heat), some to converted to kinetic energy

Causes winds, convection currents, and north-south exchange of air masses

Rate of heat redistribution varies by season

Causes seasonal weather and air circulation changes

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Variation of Air Temperature

Radiational controls

Factors that affect local radiation budget and air temperature

Time of day and time of the year

Solar altitude and duration of radiation

Cloud cover

Surface characteristics

Annual temperature cycle represents these variations

Annual temperature maximums and minimums do not occur at exact max/min of solar radiation, especially in middle and high latitudes

The atmosphere takes time to heat and cool

Average lag time in US = 27 days

Up to 36 days with the maritime influence

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Variation of Air Temperature

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Variation of Air Temperature

Daily temperature cycle

Lowest temperature usually occurs just after sunrise

Based on radiation alone, minimum temperature would occur after sunrise when incoming radiation becomes dominant

Highest temperature usually occurs in the early to middle afternoon

Even though peak of solar radiation is around noon, imbalance in favor of incoming vs. outgoing radiation continues so the atmosphere also continues to warm

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Variation of Air Temperature

Daily Temperature Cycle

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Variation of Air Temperature

Surface cover

Dry soil heats more rapidly than moist

Less energy used to evaporate water

Especially in drought, energy used only to heat soil, soil becomes hotter

Relative humidity also affects evaporation

Snow

High albedo

Less energy absorbed by the surface or converted to heat

Snow reduces sensible heating of overlying air

Some of the available heat is used to vaporize snow

Snow is an excellent infrared radiation emitter

Nocturnal radiational cooling is extreme

When skies are clear, or light winds or calm conditions

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Variation of Air Temperature

Air mass advection

Horizontal movement of an air mass from one location to another

Cold air advection (A)

Horizontal movement of colder air into a warmer area

Warm air advection (B)

Horizontal movement of warmer air into a colder area

Significance of air mass advection to local temperature

Initial temperature of the air new mass

Degree of modification the air mass as travels over the Earth’s surface

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Variation of Air Temperature

Urban heat island effect

City of warmth surrounded by cooler air

In a city:

Relative lack of moisture

Absorbed heat raises temperature (not for evaporation)

Greater concentration of heat sources (cars, air conditioners, etc)

Multiple reflections and lower albedo

Building materials conduct heat more readily than soil and vegetation

Develops best on nights when air is calm and sky is clear

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Variation of Air Temperature

Providence, RI

Buffalo, NY

Satellite-produced maps of Providence, RI (top) and Buffalo, NY (bott0m) highlighting the role that differences in development patterns/vegetation cover can have on a city’s urban heat island. Providence has a significantly stronger heat island signature.

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