Meteorology

35
“Atmosphere”

Transcript of Meteorology

Page 1: Meteorology

“Atmosphere”

Page 2: Meteorology

VocabularyOzoneTroposphereStratosphereMesosphereThermosphere

ExosphereRadiationConductionConvection

Page 3: Meteorology

Atmospheric BasicsClimate and weather relies in how solar

energy interacts with the atmosphere, and how the interactions combine to produce weather and climate

Page 4: Meteorology

Atmospheric CompositionAir is a combination of many gases, each with

its own unique characteristicsThese gases form Earth’s atmosphere, which

extends from Earth’s surface to outer space

Page 5: Meteorology

About 99% of the atmosphere is composed of nitrogen and oxygen

These main components are critical for life on Earth

If either were to change significantly, life as we know it could not exist.

Page 6: Meteorology

Key Atmospheric GasesThe amount of water vapor in the atmosphere

at any given time or place changes constantly, from 4% to 0%

Percentage varies with seasons, altitude, and with the surface features beneath the air

Page 7: Meteorology

Water vapor, the gaseous form of water, is the source of clouds, rain, and snow.

Water is the only substance in the atmosphere that exists in all three states

When water changes state to another, heat is either absorbed or released, this heat greatly affects motions that create weather and climate.

Page 8: Meteorology

Atmosphere also contains solids such as dust and salt from the wind and oceans

Dust and salt play a role in cloud formationIce is the third solid found the atmosphere as

hail and snow

Page 9: Meteorology

OzoneOzone is a gas formed by the addition of a

third oxygen atom to an oxygen molecule.Absorbs ultraviolet radiation It is thinning

Page 10: Meteorology

Structure of the AtmosphereMade up of several different layersEach layer differs in composition and

temperatureThere are lower atmospheric layers and

upper atmospheric layers

Page 11: Meteorology

Lower Atmosphere LayersLayer closest to the Earth’s surface, the

troposphere, contains most of the mass of the atmosphere, including water vapor

Most weather takes place here Most pollution is collectedGeneral temp decrease from bottom to topUpper limit is called the tropopause, 9km

Page 12: Meteorology

The next layer up is the stratosphere, made up primarily of concentrated ozone

Ozone absorbs more radiation than the troposphere.

Stratosphere is heatedGradual increase in temp Top layer called a stratopause, 50km up

Page 13: Meteorology

Upper AtmosphereAbove the stratopause is the mesosphereNo concentrated ozoneTemp decreasesMesopause is the top layer

Page 14: Meteorology

Above the mesopause is the thermosphere.Only minute portion of atmosphere’s massThis layer increases in temperature, more

than 1000°C

Page 15: Meteorology

Ionosphere is part of the thermosphereMade up of electrically charged particles

of progressively lighter gasesExosphere is the outermost layer of

Earth’s atmosphereLight gases such as helium and hydrogen

are found in this layerThere is no clear line between the

exosphere and space

Page 16: Meteorology

Solar FundamentalsThe sun is the source of all energy in the

atmosphere.This energy is transferred to Earth and

throughout the atmosphere in three ways

Page 17: Meteorology

RadiationRadiation is the transfer of energy

through space by visible light, ultraviolet radiation, and other forms of electromagnetic waves.

While Earth is absorbing solar radiation, it is also continuously sending energy back into space.

35% of incoming radiation is deflected15% is absorbed be the atmosphere

Page 18: Meteorology

Rate of absorption for any particular area varies depending on the physical characteristics of the area and the amount of solar radiation it absorbs

Water heats up and cools down more slowly than land.

Darker objects absorb energy faster than lighter ones

Page 19: Meteorology

Solar radiation does not heat air directlyMost radiation travels as short wavelengths

and the atmosphere does not easily absorb short wavelengths and so is absorbed by the Earth’s surface.

Page 20: Meteorology

The energy then released in the heat of the Earth’s surface gives off long wavelengths

It is absorbed by the atmosphere and warms the air through the processes of conduction and convection

Page 21: Meteorology

ConductionConduction which is the transfer of energy

that occurs when molecules collideLike a pot of boiling waterFor conduction to occur, substances must be

in contact with one anotherConduction affects only a very thin

atmospheric layer

Page 22: Meteorology

ConvectionConvection - transfer of energy by the

flow of a heated substancePockets of air near the Earth’s surface are

heated, become less dense than the surrounding air, and rise

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

When it cools below the temp of the surrounding air, it increases in density and sinks

Page 23: Meteorology

It heats again and the cycle continuesConvection currents are among the main

mechanisms responsible for the vertical motions of air, which in turn cause the different types of weather

Page 24: Meteorology

“State of the Atmosphere”

Page 25: Meteorology

VocabularyTemperatureHeatDew pointCondensationLifted condensation levelTemperature inversionHumidityRelative humidity

Page 26: Meteorology

Temperature Versus HeatHeat and temperature are two different

concepts.Temperature is a measurement of how

rapidly or slowly molecules move around.Heat, on the other hand, is the transfer of

energy that occurs because of a difference in temperature between substances.

Page 27: Meteorology

Direction of heat flow depends on temperature

Heat flows from an object of higher temperature to an object of lower temperature

Heat is the transfer of energy that fuels atmospheric processes, while temperature is used to measure and interpret that energy

Page 28: Meteorology

Measuring TemperatureThree units of measuring temp

Fahrenheit (F) Celsius (C) Kelvin (K)

Is based on absolute zero which corresponds to about -273 C

More direct measure of molecular activity, because at absolute zero, molecular motion theoretically stops (no negative numbers)

Page 29: Meteorology

Dew PointThe dew point is the temperature to which air

must be cooled at constant pressure to reach saturation.

Dew point is important because until air is saturated, condensation can not occur

Page 30: Meteorology

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

Dew point is often called the condensation temperature.

Page 31: Meteorology

Vertical Temperature ChangesThe temperature on a mountaintop is cooler

than at lower elevations because the temperature of the lower atmosphere decreases with increasing distance from its heat source

The height at which condensation occurs is called the lifted condensation level (LCL).

Page 32: Meteorology

Height of the LCL often corresponds to the base of clouds.

Above the LCL air becomes saturated and cools slowly

The rate at which saturated air cools is called the moist adiabatic lapse rate.

Page 33: Meteorology

Air Pressure and DensityThe gravitational attraction between Earth

and atmospheric gases causes particles of gas to be pulled toward the center of the Earth.

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

Page 34: Meteorology

Pressure-Temperature-DensityTemperature is directly proportional to

pressureAs temperature increases or decreases

pressure does the sameTemperature and density are inversely

proportionalAs temperature decreases, density increases.

Page 35: Meteorology

Pressure-Temperature-DensityAs temp increases, pressure increasesAs temperature decreases, pressure

decreasesAs temperature decreases, density increasesAs temperature increases, density decreases