The Atmosphere

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The Atmosphere

Chapter 11

11.1

Atmospheric Composition

 About 99% of the atmosphere is composed of nitrogen and oxygen (78% nitrogen, 21% oxygen)

– The remaining 1% consists of small amounts of argon, hydrogen, carbon dioxide, water vapor, & other gases.

Key Atmospheric Gases

 The levels of CO2 and water vapor vary constantly.

– The level of these gases are critical because they play an important role in regulating the amount of energy the atmosphere absorbs.

Ozone

 Ozone (O3) is important because it absorbs

UV radiation from the Sun thus warming the layer.

Structure of the Atmosphere

 The atmosphere is divided into five layers:

– Troposphere

 The lowest layer is where most of the weather occurs.

– Stratosphere

 Contains Ozone layer

– Mesosphere

 Meteors burn up, coldest layer

– Thermosphere

 The aurora caused by

- Exosphere

Outermost layer particles from the Sun i nteracting with Earth’s atm.

– Ionosphere

 Charged particles reflect radio signals

Structure of the Atmosphere

Radiation

 Radiation is the transfer of energy through space by visible light, UV radiation, and other forms of electromagnetic waves

– ~30% of incoming solar radiation is reflected into space by Earth’s surface

– ~20% is absorbed by the atmosphere itself

 Only 50% of incoming solar radiation is absorbed by

Earth’s surface

Radiation

 The rate of absorption for any area varies depending on the physical characteristics of the area and the amount of solar radiation it receives.

– *Land heats and cools faster than water

– Darker objects absorb energy faster than lighter ones

Radiation

Conduction

 Energy is transferred throughout the atmosphere by the process of conduction, convection & radiation.

 Conduction is the transfer of energy that occurs when molecules collide.

– Energy is transferred from the particles of air near Earth’s surface to the particles of air in the lowest layer of the atmosphere.

Convection

 Convection is the transfer of energy by the flow of a heated substance.

– Pockets of air near Earth’s surface are heated, become less dense than the surrounding air & rise.

– As the warm air rises, it expands and starts to cool.

– When it cools below the temperature of the surrounding air, it increases density and sinks.

 Convection Currents

Convection

Conduction, Convection,

Radiation

Chapter 11.1 Quiz

 1. Name the 5 layers of the atmosphere in order from farthest to closest to Earth’s surface.

 2. What is significant about the ionosphere?

 3. What are the 2 main gases in our atmosphere and what is the percent they make up of the atmosphere?

 4. ____________ is the transfer of energy that occurs when molecules collide.

 5. The level of __________ & __________ are critical because they play an important role in regulating the amount of energy the atmosphere absorbs.

11.2

State of the Atmosphere

 Temperature is a measurement of how rapidly or slowly molecules move around.

– fast moving molecules = higher temp.

– Slow moving molecules = lower temp.

 Heat is the transfer of energy that occurs because of a difference in temperature between substances.

– Heat flows from area of high temp. to area of low temp.

Dew Point

 The dew point is the temperature to which air must be cooled at constant pressure to reach saturation.

– Saturation is the point at which the air holds as much water vapor as it possibly can.

 Condensation occurs when matter changes state from a gas to a liquid.

Moisture in the Atmosphere

 When the air is holding as much moisture as it can, the air is saturated .

– The air’s ability to hold water vapor depends upon the temperature.

– The warmer the air, the more moisture the air can hold.

 The dew point is the temperature to which the air must be cooled to become saturated.

– If the temperature falls below the dew point, condensation occurs as water vapor changes to liquid water.

Vertical Temperature Changes

 Dry Adiabatic Lapse Rate: the rate at which unsaturated air (which no heat is added or removed) will cool.

– 10°C for every 1,000m increase in altitude.

 Moist Adiabatic Lapse Rate : the rate at which saturated air cools.

– ~4°C/1,000m in very warm air to ~9°C/1,000m in very cold air.

Vertical Temperature Changes

 Lifted Condensation Level (LCL): the height at which condensation occurs.

– LCL often corresponds to the base of clouds

– Air above the LCL is saturated and cools slower than air below the LCL.

Air Pressure & Density

 Air has mass and exerts pressure on our bodies.

– Atmospheric pressure increases as you near the bottom of the atm because of the greater mass of atm above you.

– Atmospheric pressure decreases with height because there are fewer gas particles exerting pressure.

Air Pressure & Density

 The density of air is proportional to the number of particles of air occupying a particular space.

– The density of air increases as you get closer to the bottom of the atmosphere.

– The density of air decreases as you increase elevation.

Pressure-Temperature-Density

Relationship

 Temperature is directly proportional to pressure.

– As temp increases/decreases, pressure does too

– As pressure increases/decreases, temperature does too

Pressure-Temperature-Density

Relationship

 The relationship between temperature and density is inversely proportional.

– As temperature increases, density decreases

– As temperature decreases, density increases

 **Temperature is proportional to the ratio of pressure to density, which decreases with increasing altitude.

Temperature Inversion

 A temperature inversion is an increase in temperature with height in an atmospheric layer.

– temp-altitude relationship is inverted

Temperature Inversion

Wind

 Cool air = more dense, sinks

 Warm air = less dense, rises

– **Air flows from areas of high pressure to areas of low pressure

 Wind changes with height in the atm

– Near the surface, wind is disrupted by the friction that results from contact with trees, buildings, etc.

– Farther up from Earth’s surface, air encounters less friction & wind speeds increase

Wind

Relative Humidity

 The amount of water vapor in air is referred to as humidity .

 The ratio of water vapor in a volume of air relative to how much water vapor that volume of air is capable of holding is called relative humidity .

– RH is expressed as a percentage %

Relative Humidity

 Compares how much moisture the air is actually holding with how much moisture it could hold if the air were saturated.

– It is expressed as a percent of saturation.

 Air is saturated if it is holding all the moisture it can hold at its present temperature.

 Determined with a psychrometer and a relative humidity table.

Relative Humidity

 Warm air is capable of holding more moisture than cool air.

– If the temp. of a room increased, the air in the room would be capable of holding more moisture.

 If no additional water vapor was added to the air, its relative humidity would decrease.

 If more water vapor was added to the air, its relative humidity would increase.

Relative Humidity

11.3

Moisture in the Atmosphere

Cloud Formation

 Clouds form when rising air is cooled below its dew point.

 Tiny particles called condensation nuclei (small

 particles in the air) allow a cloud to form.

Cloud Formation

 Clouds can also form when wind encounters a mountain and the air has nowhere to go but up.

– As the air rises it cools and condenses.

– This is method of cloud formation is called orographic lifting .

Cloud Formation

 Another method of cloud formation involves the collision of air masses of different temps.

– Cold, more dense air mass will collect near the surface.

– As warm air moves into the area, some of it will warm up the cold air but the bulk will rise over the cold air.

 As the warm air cools, the water vapor in it condenses and forms a cloud.

Stability

 stability = tendency of air to remain in in its original position (resist rising).

– The rate at which an air mass cools depends on the temperature of the surface beneath the air.

 If the air = cooler; it is going to want to sink  stable

 If the air = warmer; it is going to want to rise  unstable

Stability

Latent Heat

 As water vapor in the air condenses, heat is released.

 It takes energy to change liquid water into gaseous state

– That energy is stored in the water vapor and will not be released into the air until condensation occurs.

 The stored energy is called latent heat .

– When condensation occurs, latent heat is released and warms the air.

Types of Clouds

 Clouds are classified by the altitude at which they form and by their shape.

Low Clouds

 Typically form below 2,000m

– Stratocumulus : gray/whitish patch/sheet that is flattened out and spread horizontally

– Cumulus : detached, generally dense clouds with sharp outlines that develop vertically in the form of rising mounds.

– Stratus : layered gray cloud that covers much or all of the sky in a given area

– Cumulonimbus : thunderstorm cloud, dark at the bottom that produces rain and/or hail.

Cumulus

Low Clouds

Stratus

Cumulonimbus

Stratocumulus

Middle Clouds

 Form at heights between 2,000 and 6,000m

– Altocumulus : white/gray patch or sheet layered clouds (resemble fish scales)

– Altostratus : dark but thin veils of clouds that sometimes produce mild precipitation and cover totally or partially the sky. Thin enough to see the sun.

– Nimbostratus : the continuous rain cloud resulting from thickening altostratus. Completely block out the Sun. Dark gray in color; associated with precipitation.

Middle Clouds

Altostratus

Altocumulus

Nimbostratus

High Clouds

 Form at heights of 6,000m

– Temps are below freezing, thus made up of ice crystals.

– Cirrus : wispy, indistinct (detached) appearance

– Cirrostratus : transparent, whitish veil clouds with a smooth appearance. continuous layer that covers the sky

– Cirrocumulus : thin, white patch sheet or layered clouds

Cirrus

High Clouds

Cirrostratus

Cirrocumulus

Types of Clouds

Precipitation

 When cloud droplets collide, they join together to form a larger droplet in a process called coalescence .

 As the process continues the droplet becomes too heavy to be held aloft and falls to earth as precipitation .

– Rain, snow, sleet, and hail

Precipitation

 Rain and snow are the most common forms of precipitation.

 Drizzle is small raindrops that fall slowly

 Sleet is a partially frozen mixture of rain and snow that occurs when the temperature is just above freezing.

 Hail is in the form of ice balls, which usually occurs in violent thunderstorms.

– Hailstones begin as snowflakes that start to melt and gather more moisture as they fall.

The Water Cycle

 Water moves between Earth’s surface and its atmosphere  water cycle

1. Radiation from the Sun causes liquid water to change into a gas  evaporation

2. As water vapor rises, it cools and changes back into a liquid  condensation

3. Water droplets combine to form larger drops that fall to Earth  precipitation

The Water Cycle

Weather

 The short-term (a few hours or days) condition of the atmosphere at a given location.

– Temperature, sky conditions, precipitation, atmospheric pressure, humidity, wind speed, and wind direction.

 Meteorologists are scientists who study and predict the weather.

Air Temperature

 In the daily cycle, temperature is usually lowest in the early morning and warmest at mid-afternoon.

 In the season cycle, winters are generally cold, while summers tend to be hot.

 Short term factors such as cloud cover and regional weather systems affect temperatures.

– Clouds reduce daytime temperature by reflecting sunlight back into space.

– At night, clouds help hold heat energy to Earth.

Air Temperature

 Measured with a thermometer .

– A bulb that contains liquid that expands into a narrow, calibrated neck when it is heated and moves down the neck when the temperature decreases.

 When meteorologists record official air temperature, the thermometer is kept in a special weather shelter to protect the instruments from direct sunlight.

Temperature Scales

 A temperature of zero on the Fahrenheit scale is the temperature of a mixture of equal parts ice, water, and salt.

 The freezing point of water is what sets the zero point on the

Celsius (centigrade) scale.

 The point at which all particle motion stops is defined as zero on the Kelvin scale.

Air Pressure

 Is caused by the weight of the atmosphere.

 Above each square inch of Earth’s surface is a column of air the weighs 14.7 pounds.

Measuring Air Pressure

 A barometer is an instrument used to measure air pressure using the dense liquid metal mercury.

 Meteorologists measure air pressure in millibars .

 Standard sea level pressure is 1013.2 millibars.

 On a weather map, isobars connect places that have the same air pressure.

Air Pressure Factors

 If air is cooled, it contracts and becomes denser.

– This causes pressure to rise.

 If air is heated, it expands and becomes less dense.

– This causes pressure to fall.

 Humid air is lighter than dry air.

– This is because water molecules are lighter than the gasses they displace in the air.

Measuring Moisture in the Atmosphere

 Meteorologists use a sling psychrometer and a dew-point temperature table to determine the dew point.

– The psychrometer consists of two thermometers mounted side by side which can be swung through the air.

– One thermometer measures the air temperature.

– The bulb of the other thermometer is covered by a wet cloth.

– As the thermometers are swung through the air, evaporated cooling causes the wet-bulb thermometer to register a lower temperature.

– When you subtract the wet-bulb temperature from the drybulb temperature, you can use the dew-point table to determine the dew point.

Psychrometer

The Wind

Wind is heat flow by convection within the atmosphere.

Winds are the result of uneven heating of the Earth’s surface.

– This uneven heating causes differences in air pressure to develop.

The Wind

 Winds always blow from areas of high pressure to areas of low pressure.

– Winds blow fastest where the gradient in air pressure is greatest, where the isobars are close together.

Measuring the Wind

 To measure the wind, you need to determine both the wind speed and the wind direction.

 Wind speed is measured with an anemometer .

– The cups catch the wind, causing it to spin.

 Wind direction is indicated by a wind vane, which points into the wind.

The Coriolis Effect

 The Earth’s rotation causes winds to curve.

– to the right in the Northern

Hemisphere .

– to the left in the Southern

Hemisphere.

The Coriolis Effect

 Winds move in a clockwise outward spiral around high-pressure systems.

 Winds move in a counterclockwise inward spiral around low-pressure systems.

The Coriolis Effect

Zones of

Convergence and Divergence

 Rising warm, moist air at the center of the low causes winds and air masses to blow into the low-pressure system.

 The rising air cools, which causes cloud formation and precipitation.

 The descending air turns a high-pressure system into a single mass of cool, dry air that spreads across the surface of Earth.

Precipitation

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