chapter 11 atmosphere

Upload: ncl12142

Post on 06-Apr-2018

231 views

Category:

Documents


0 download

TRANSCRIPT

  • 8/3/2019 Chapter 11 Atmosphere

    1/55

    Prentice Hall

    EARTH SCIENCEEARTH SCIENCE

    Tarbuck Lutgens

  • 8/3/2019 Chapter 11 Atmosphere

    2/55

    Chapter

    1111The Atmosphere

  • 8/3/2019 Chapter 11 Atmosphere

    3/55

    Composition of the Atmosphere

    11.1 Atmosphere Characteristics

    Weather: constantly changing, and it refers

    to the state of the atmosphere at any given

    time and place

    Climate: based on observations of weather

    that have been collected over many years. -

    - helps describe a place or region

  • 8/3/2019 Chapter 11 Atmosphere

    4/55

    Composition of the Atmosphere

    11.1 Atmosphere Characteristics

    Air is a mixture of different gases and particles,

    each with its own physical properties.

    Permanent atmospheric gases:

    -do not change: nitrogen and oxygen:99%

    -others that have changed through time:

    helium, methane, and ammonia

  • 8/3/2019 Chapter 11 Atmosphere

    5/55

    Volume of Clean, Dry Air

  • 8/3/2019 Chapter 11 Atmosphere

    6/55

    Composition of the Atmosphere

    17.1 Atmosphere Characteristics

    Variable Components: not as constant,

    varies1. Water vapor: gaseous form of water, source of

    all clouds and precipitation. Like carbon dioxide,

    water vapor absorbs heat given off by Earth and

    some solar energy.

    2. Ozone is a form of oxygen that combines three

    oxygen atoms into each molecule (O3). If ozone did not filter most UV radiation and all of

    the suns UV rays reached the surface of Earth,

    our planet would be uninhabitable for many

    living organisms.

  • 8/3/2019 Chapter 11 Atmosphere

    7/55

    Variable Gases, cont.

    3. Carbon Dioxide:-concentration has risen from 0.028% to 0.039% due

    to greenhouse gas

    -cycled between the atmosphere, oceans, organisms,

    and rocks

    -global warming due to absorption of heat

  • 8/3/2019 Chapter 11 Atmosphere

    8/55

    Composition of the Atmosphere

    11.1 Atmosphere Characteristics

    Human Influence

    Emissions from transportation vehicles account

    for nearly half the primary pollutants by weight.

  • 8/3/2019 Chapter 11 Atmosphere

    9/55

    Primary Pollutants

  • 8/3/2019 Chapter 11 Atmosphere

    10/55

    Height and Structure of the

    Atmosphere

    11.1 Atmosphere Characteristics

    The atmosphere rapidly thins as you travelaway from Earth until there are too few gas

    molecules to detect. Air pressure

    decreases

    Atmospheric pressure is simply the weight of the

    air above.

    Pressure Changes

  • 8/3/2019 Chapter 11 Atmosphere

    11/55

    Atmospheric Layers(p. 284-285)

    Draw the atmospheric layers in your notes.

    -describe the key features of each layer

  • 8/3/2019 Chapter 11 Atmosphere

    12/55

    Atmospheric Pressure vs. Altitude

    In the Troposphere

  • 8/3/2019 Chapter 11 Atmosphere

    13/55

    Height and Structure of the

    Atmosphere

    11.1 Atmosphere Characteristics

    Temperature Changes The atmosphere can be divided vertically into

    layers based on temperature.

    The troposphere is the bottom layer of the

    atmosphere where temperature decreases with an

    increase in altitude. The stratosphere is the layer of the atmosphere

    where temperature remains constant to a height

    of about 20 kilometers. It then begins a gradual

    increase until the stratopause.

  • 8/3/2019 Chapter 11 Atmosphere

    14/55

    Snowy Mountaintops Contrast with

    Warmer Snow-Free Lowlands

    (troposphere)

  • 8/3/2019 Chapter 11 Atmosphere

    15/55

  • 8/3/2019 Chapter 11 Atmosphere

    16/55

    Exosphere

    -the uppermost (or outermost) layer

    -gas molecules can be exchanged betweenEarths atmosphere and space

    -satellites orbit in the exosphere

  • 8/3/2019 Chapter 11 Atmosphere

    17/55

    Thermal Structure of the Atmosphere

  • 8/3/2019 Chapter 11 Atmosphere

    18/55

    Earth-Sun Relationships

    11.1 Atmosphere Characteristics

    Earths Motions Earth has two principal motionsrotation and

    revolution.

    Earths Orientation Seasonal changes occur because Earths

    position relative to the sun continually changes

    as it travels along its orbit.

  • 8/3/2019 Chapter 11 Atmosphere

    19/55

    Tilt of Earths Axis

  • 8/3/2019 Chapter 11 Atmosphere

    20/55

    Earth-Sun Relationships

    11.1 Atmosphere Characteristics

    Solstices

    summer solstice: occurs on June 21 or 22 in

    the Northern Hemisphere and is the official first

    day of summer. Longest day of year.

    winter solstice: occurs on December 21 or 22

    in the Northern Hemisphere and is the official

    first day of winter. Shortest day of year.

  • 8/3/2019 Chapter 11 Atmosphere

    21/55

    Earth-Sun Relationships

    11.1 Atmosphere Characteristics

    Equinoxes: 12 hours day, 12 hours night

    autumnal equinox :occurs on September 22 or

    23 in the Northern Hemisphere.

    spring equinox: occurs on March 21 or 22 in

    the Northern Hemisphere.

  • 8/3/2019 Chapter 11 Atmosphere

    22/55

    Solstices and Equinoxes

  • 8/3/2019 Chapter 11 Atmosphere

    23/55

    Energy Transfer as Heat

    11.2 Heating the Atmosphere

    Heat :energy transferred from one object to

    another because of a difference in the

    objects temperature.

    Temperature :measure of the average

    kinetic energy of the individual atoms or

    molecules in a substance.

  • 8/3/2019 Chapter 11 Atmosphere

    24/55

    Energy Transfer as Heat

    11.1 Heating the Atmosphere

    Three mechanisms of energy transfer as

    heat are conduction, convection, and

    radiation.

    Conduction is the transfer of heat through

    matter by molecular activity.

    1. Conduction

    Convection is the transfer of heat by mass

    movement or circulation within a substance.

    2. Convection

  • 8/3/2019 Chapter 11 Atmosphere

    25/55

    Energy Transfer as Heat

  • 8/3/2019 Chapter 11 Atmosphere

    26/55

    Energy Transfer as Heat

    11.2 Heating the Atmosphere

    3. Radiation: Electromagnetic Waves

    The sun emits light and heat as well as the

    ultraviolet rays that cause a suntan. These formsof energy are only part of a large array of energy

    emitted by the sun, called the electromagnetic

    spectrum.

  • 8/3/2019 Chapter 11 Atmosphere

    27/55

    Electromagnetic Spectrum

  • 8/3/2019 Chapter 11 Atmosphere

    28/55

    Visible Light Consists

    of an Array of Colors

  • 8/3/2019 Chapter 11 Atmosphere

    29/55

    Energy Transfer as Heat

    11.2 Heating the Atmosphere

    Radiation Radiation :transfer of energy (heat) through

    space by electromagnetic waves that travel outin all directions.

    Unlike conduction and convection, which need

    material to travel through, radiant energy can

    travel through the vacuum of space.

  • 8/3/2019 Chapter 11 Atmosphere

    30/55

    Energy Transfer as Heat

    11.2 Heating the Atmosphere

    Radiation

    All objects, at any temperature, emit radiant

    energy.

    Hotter objects radiate more total energy per unit

    area than colder objects do.

    The hottest radiating bodies produce the shortest

    wavelengths of maximum radiation. Objects that are good absorbers of radiation are

    good emitters as well.

  • 8/3/2019 Chapter 11 Atmosphere

    31/55

    Pressure, Temperature, and

    Density Relationship Open to page 291 Summarize the relationships between

    these 3 variables using a skit.

  • 8/3/2019 Chapter 11 Atmosphere

    32/55

    Temperature Inversion (p. 292)

    Define temperature inversion and give

    examples

  • 8/3/2019 Chapter 11 Atmosphere

    33/55

    Wind (p. 292)

    Describe how wind is created.

  • 8/3/2019 Chapter 11 Atmosphere

    34/55

    Humidity (p. 294)

    Humidity: amount of water vapor in the

    atmosphere

    Saturation: when the amount of watervapor in the air is at its maximum

    Relative humidity: amount of water vapor

    in air relative to the amount of water

    needed to reach saturation (in %)

    If the air is saturated, the relative humidity is

    100%

  • 8/3/2019 Chapter 11 Atmosphere

    35/55

    Humidity, cont.

    Dew point: temperature that air must be

    cooled to in order to reach saturation

    If the dew point is near the actual

    temperature, the relative humidity is high

    Latent heat: extra thermal energy stored in

    water vapor compared to liquid water

    Adiabatic process: temperature changeswithout the addition or subtraction of

    thermal energy (pressure is changing-bike

    tire example)

  • 8/3/2019 Chapter 11 Atmosphere

    36/55

    What Happens to Solar Radiation?

    17.2 Heating the Atmosphere

    When radiation strikes an object, there

    usually are three different results.

    1. Some energy is absorbed by the object.

    2. Substances such as water and air are

    transparent to certain wavelengths of radiation.

    3. Some radiation may bounce off the object

    without being absorbed or transmitted.

  • 8/3/2019 Chapter 11 Atmosphere

    37/55

    Solar Radiation

  • 8/3/2019 Chapter 11 Atmosphere

    38/55

    What Happens to Solar Radiation?

    11.2 Heating the Atmosphere

    Reflection and Scattering Reflection occurs when light bounces off an

    object. Reflection radiation has the sameintensity as incident radiation.

    Scattering produces a larger number of weaker

    rays that travel in different directions.

  • 8/3/2019 Chapter 11 Atmosphere

    39/55

    What Happens to Solar Radiation?

    11.2 Heating the Atmosphere

    Absorption

    About 50 percent of the solar energy that strikes

    the top of the atmosphere reaches Earthssurface and is absorbed.

    The greenhouse effect is the heating of Earths

    surface and atmosphere from solar radiation

    being absorbed and emitted by the atmosphere,mainly by water vapor and carbon dioxide.

  • 8/3/2019 Chapter 11 Atmosphere

    40/55

    Why Temperatures Vary

    11.3 Temperature Controls

    Factors other than latitude that exert a

    strong influence on temperature include

    heating of land and water, altitude,geographic position, cloud cover, and

    ocean currents.

  • 8/3/2019 Chapter 11 Atmosphere

    41/55

    Why Temperatures Vary

    11.3 Temperature Controls

    Land and Water Land heats more rapidly and to higher

    temperatures than water. Land also cools morerapidly and to lower temperatures than water.

  • 8/3/2019 Chapter 11 Atmosphere

    42/55

    Mean Monthly Temperatures

    forVancouver and Winnipeg

  • 8/3/2019 Chapter 11 Atmosphere

    43/55

    Why Temperatures Vary

    11.3 Temperature Controls

    Geographic Position

    The geographic setting can greatly influence

    temperatures experienced at a specific location.

  • 8/3/2019 Chapter 11 Atmosphere

    44/55

    Mean Monthly Temperatures for

    Eureka and New York City

  • 8/3/2019 Chapter 11 Atmosphere

    45/55

    Mean Monthly Temperatures

    for Seattle and Spokane

  • 8/3/2019 Chapter 11 Atmosphere

    46/55

    Why Temperatures Vary

    11.3 Temperature Controls

    Altitude

    The altitude can greatly influence temperatures

    experienced at a specific location.

  • 8/3/2019 Chapter 11 Atmosphere

    47/55

    Mean Monthly Temperatures for

    Guayaquil and Quito

  • 8/3/2019 Chapter 11 Atmosphere

    48/55

    Clouds Reflect and Absorb Radiation

  • 8/3/2019 Chapter 11 Atmosphere

    49/55

    World Distribution of Temperature

    11.3 Temperature Controls

    Isotherms are lines on a weather map that

    connect points where the temperature is

    the same. Isotherms generally trend east and west and

    show a decrease in temperatures from the

    tropics toward the poles.

  • 8/3/2019 Chapter 11 Atmosphere

    50/55

    11.3 Clouds and Precipitation

    (p. 297) Describe how clouds form using the termsrising, cooling, air mass, warming, denser,

    condensation nucleus

  • 8/3/2019 Chapter 11 Atmosphere

    51/55

    Atmospheric Stability (p. 298)

    Rising air masses become colder similar

    to the air as you increase altitude, but air

    masses cool off more quickly

    It will become cooler than the surrounding

    air and more dense, so it will sink down

    When the air mass stops rising and

    sinking, it is stable

    If the air mass is moving, it is unstable

  • 8/3/2019 Chapter 11 Atmosphere

    52/55

    Atmospheric Lifting (p. 299)

    Mechanical processes can create clouds

    1. Orographic lifting: air mass if forced to

    rise over a topographic barrier like amountain (thus it cools due to an increase

    in altitude, creating clouds due to

    condensation)

    2. Convergence: two air masses collide, thewarmer air mass rises over the cooler air

    mass because it is less dense

  • 8/3/2019 Chapter 11 Atmosphere

    53/55

    Types of Clouds (p. 300)

    Summarize the types of clouds and their

    associated weather in a data table.

    Low

    Clouds

    Middle

    Clouds

    High

    Clouds

    Vertical

    Development

    Clouds

    Description

    Weather

    TypeOther Info

  • 8/3/2019 Chapter 11 Atmosphere

    54/55

    Precipitation (p. 302)

    Precipitation: all forms of water that fall

    from clouds to the ground

    examples:

    Coalescence: cloud droplets join together

    to make larger droplets

    Eventually, get too big to stay in cloud and fall

    When does snow, sleet, and hail form?

  • 8/3/2019 Chapter 11 Atmosphere

    55/55

    Water Cycle (p. 303)

    Complete the water cycle activity