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Title: "INSOLATION AND THE SEASONS TOPIC 6 page 85106


1
"INSOLATION AND THE SEASONSTOPIC 6(page
85-106)
2
6-1) SOLAR RADIATION AND INSOLATION
  • insolation - (incoming solar radiation)
  • the sun's energy that is received by Earth.
  • maximum intensity occurs as visible light.

3
Effects of Earth's Atmosphere on Insolation
  • insolation may be
  • absorbed,
  • reflected, or
  • scattered
  • before it reaches the Earth's surface.

4
1 - ABSORPTION
  • SHORT WAVE ENERGY
  • Most of the short wave radiation is
  • absorbed by the atmosphere.
  • Ultraviolet (UV) radiation is
  • absorbed by the ozone layer.
  • ozone
  • form of oxygen gas. (03)
  • destroyed by (CFCs) chlorine and fluorine gases.
  • less ozone more UV radiation striking the
    Earth's surface.
  • UV radiation causes skin cancer.

5
  • LONG WAVE ENERGY.
  • Is absorbed by greenhouse gases.
  • Greenhouse gases
  • carbon dioxide
  • water vapor
  • methane gas

6
2 - REFLECTION SCATTERING
  • clouds reflect insolation back into space.
  • aerosols reflect, scatter, and absorb insolation.

7
aerosol
  • finely dispersed solids and liquids in the air.
  • examples ice crystals, water droplets, dust,
    volcanic ash, pollution.
  • As the amount of aerosols increases
  • more insolation is scattered
  • the amount of insolation reaching the ground is
    less
  • the temperature will decrease.

8
Balance of Energy
  • the amount of energy from insolation is equal to,
    the amount of energy radiated from the Earth.
  • therefore, Earth's temperature and heat are
    balanced.

9
Factors Affecting Absorption and Reflection at
Earths Surface.
10
1 - Angle of Insolation
  • Angle of Insolation (angle of incidence)
  • the angle at which the insolation strikes Earth's
    surface.

11
The greater the angle of insolationmore energy
is absorbed and less energy is reflected.
  • the higher the sun is in the sky, the greater the
    angle of insolation.
  • noon sun almost overhead large angle of
    insolation.
  • early morning or late evening low in sky low
    angle of insolation.

12
diagram
high angle
energy focused on small area
intense heating
low angle
energy spread over a large area
less heating
13
2 - Surface Characteristics.
  • Texture and color
  • rough surfaces and dark colors absorb more
    insolation.

14
3 - Change of State and Transpiration
  • When energy is involved in change of state or
    transpiration.
  • it is not available to raise the temperature of
    Earth's surface.

15
4 - Land vs Water
  • Liquid water will heat up and cool off more
    slowly than an equal area of land.

16
4 Reasons why Water heats more slowly than land.
  • water has a higher specific heat.
  • insolation can penetrate water (it only heats the
    surface of the land).
  • water can flow, so energy can be distributed by
    convection currents.
  • energy is used to evaporate water.

17
THE GREENHOUSE EFFECT
  • infrared energy, from the Earth, is absorbed by
    gases in the atmosphere.
  • greenhouse gases carbon dioxide, water vapor
    and methane.
  • Greenhouse gases reduce the amount of energy that
    is lost to space.
  • If less energy is lost, Earth's atmosphere
    becomes warmer.
  • As more of these gases are added to the
    atmosphere, more energy is absorbed (global
    warming).

18
Greenhouse Effect Diagram
  • Short-wave radiation (insolation) passes through
    the atmosphere,
  • Long-wave radiation from the Earth (terrestrial
    radiation) is absorbed by the atmosphere.
  • diagram

19
  • Global Warming
  • an increase in average Earth temperatures.
  • Caused by
  • the burning of wood and fossil fuels.
  • Results..
  • Rising sea level.
  • Shifting of climatic zones.

20
Review Book Complete Review Questions page
88, 1-10.
21
6-2) VARIATION IN INSOLATION
22
Insolation can vary in 2 ways
  • intensity (strength).
  • duration (length of time)

23
Five factors that affect Intensity
  • intensity
  • the rate at which solar energy is received.

24
  • Angle of Insolation
  • At 90 o (perpendicular)
  • maximum intensity (energy is concentrated).
  • At angles close to 0 o
  • minimum intensity (energy is spread out).

25
  • 2) Earth's Shape
  • At any given time, there is only one location
    where the angle of insolation is 90o. (maximum
    intensity)
  • For every degree of latitude (N or S of that
    location) the angle of insolation is one degree
    less. (intensity is less)
  • Examples

26
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27
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28
  • 3) Latitude.
  • The maximum intensity of insolation occurs near
    the equator.
  • The noon sun is always close to overhead.

29
  • 4) Time of year (Seasons)

30
SPRING
March 21
Equinox
SUMMER
WINTER
SUN
Dec 21
June 21
Solstice
Solstice
FALL
Sept 23
Equinox
31
Equinox (March 21 Sept 23)
  • Maximum intensity of insolation is at
  • 0 o Latitude (the equator).
  • Duration
  • 12 hours light and 12 hours of darkness,
    everywhere.
  • diagram

32
day
night
Suns rays
equator
0o
33
Summer Solstice (June 21) "first day of summer"
  • Maximum intensity of insolation is at
  • 23 1/2 o N Latitude (Tropic of Cancer).
  • Duration
  • North Pole, 24 hours of daylight.
  • South Pole, 24 hours of darkness.
  • diagram

34
day
night
90.0o -23.5o
66 ½ oN
23 ½ o N
0o
Suns rays
equator
35
Winter Solstice (December 21) "first day of
winter"
  • Maximum intensity of insolation is at
  • 23 1/2 o S Latitude (Tropic of Capricorn).
  • Duration
  • South Pole, 24 hours of daylight.
  • North Pole, 24 hours of darkness.
  • diagram

36
day
night
66 ½ oN
equator
Suns rays
0o
23 ½ o S
66 ½ oS
37
5) Time of Day
  • Maximum angle and intensity of insolation occurs
  • at solar noon.

38
Variation in Duration of Insolation
  • duration amount of time.
  • time between sunrise and sunset.

39
  • Duration is determined by.
  • Latitude and Season.
  • In the Northern Hemisphere
  • Longest day of the year..
  • Summer Solstice (June 21)
  • Shortest day of the year
  • Winter Solstice (December 21)
  • 12 hours daylight 12 hours dark
  • Spring Fall Equinox (March 21 Sept 23)

40
Relationship of Surface Temperature to Insolation
  • When energy is being gained at a greater rate
    than it is being lost, Earth's surface
    temperature
  • rises.
  • Greater intensity and/or greater duration usually
    means greater temperature.

41
Times of Maximum Minimum Yearly Temperature.
  • The date for maximum and minimum temperatures
    occurs
  • after the date for maximum and minimum
    insolation.

42
In the Continental United States
  • Greatest intensity of insolation occurs on June
    21 but ..
  • the highest temperature occurs late July or early
    August.
  • reason after June 21 the surface still receives
    more energy than it loses.
  • Minimum insolation occurs on Dec. 21
  • lowest temperature occurs in late January or
    early February

43
Times of Maximum and Minimum Daily Temperature.
  • Maximum intensity of insolation occurs at..
  • solar noon.
  • The hottest part of day occurs in
  • mid-afternoon.
  • Minimum intensity of insolation occurs
  • after the sun sets.
  • Coolest temp occurs
  • just after sunrise.

44
Answer Review Questions 11 - 31 on page 93.
45
6.3) HEAT BUDGET AND CLIMATE CHANGE.
46
Earth's heat budget is the result balance between
  • the radiation from the sun (insolation)
  • the radiation Earth gives off to space.

47
Examples of Climate Change.
48
1) Ice Ages and Long, Warm Periods on Earth.
  • ice ages - periods when glaciers advanced into
    the middle latitudes.
  • interglacial periods - warmer periods that
    occurred between the times of glacial advance.

49
2) El Nino and La Nina.
50
El Nino -
  • occurs every two to ten years.
  • the normally cold waters of the eastern Pacific
    Ocean (off western South America) are replaced
    with warmer waters.

51
La Nina
  • periods of time when there is exceptionally cold
    water.

52
El Nino and La Nina cause major climatic
repercussions around the world.
53
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54
3) Global Warming.
  • from the early 1980's there has been a trend of
    rising temperatures known as global warming.

55
E) CAUSES OF HEAT BUDGET SHIFTS.
56
1 - Changes in Solar Energy.
  • the sun's energy output and related sunspot
    activity follow an 11 year cycle.
  • sunspot - a darker region of the sun's surface.
  • when there are more sunspots, the sun emits 0.1
    to 1.0 percent more energy.

57
2 - Changes in Earth's Orbit and Axis Tilt.
  • over thousands of years the tilt of Earth's axis
    changes a few degrees.

58
  • minor changes in the eccentricity of Earth's
    orbit.
  • if these two things occur at the same
    timesummers may be cooler and winters warmer.
  • these changes seem to correlate with the advances
    of glaciers during the Pleistocene Ice Age.

59
3 - Volcanic Eruptions
  • 1990 eruption of Mount Pinatubo, causes cooling
    of Earth's atmosphere.
  • addition of aerosols makes Earth's atmosphere
    less transparent to insolation.

60
4 - Human Causes.
61
a) desertification
  • overgrazing causes grasslands to become deserts.
  • deserts heat up faster than grasslands, so the
    temperature of these areas increases.

Sahara Desert encroach on Nouakchott, the capital
of Mauritania.
62
b) deforestation -
  • insolation once absorbed by trees goes into
    heating Earth's surface.
  • without trees, there is less transpiration which
    decreases the humidity of the atmosphere and
    therefore there is less precipitation.
  • these areas become hotter and drier.

Loggers prepare to fell an 800-year-old red cedar
in the state of Washington.
63
A burned clearing stands in grim contrast to
surrounding rain forest in Brazil.
Brazilian cattle graze in a pasture where rain
forest once stood.
64
c) Addition of greenhouse gases to the
atmosphere.
65
d) urbanization -
  • clearing the land of plants and trees to
    construct buildings.

66
Read pages 95 99Answer Review Questions p 99,
32-38.
67
F) SEASONS.
  • Seasonal changes result from variation in the
  • angle of insolation.
  • intensity of insolation.
  • duration of insolation.
  • There is little seasonal change near..
  • the equator.
  • Season changes are more extreme near .
  • the poles.

68
Causes of the Seasons.
69
a) Tilt of Earth's Axis.
  • Earth's axis is tilted 23.5o with respect to the
    plane of its orbit.
  • perpendicular insolation from the sun shifts
    between 23.5o N (on June 21) and 23.5o S
    latitude (on Dec 21).
  • a greater tilt would produce warmer summers and
    colder winters.
  • no tilt would result in no seasons.

70
b) Parallelism of Earth's Axis.
  • the position of Earth's axis at any time is
    always parallel to its position at any other time
    (parallelism).
  • the Northern end of Earth's axis always points
    towards the North Star (Polaris).

71
c) Revolution Around the Sun.
  • As Earth revolves around the sun, the direction
    of Earth's axis with respect to the sun
    varies..
  • on June 21..the North Pole is inclined toward
    the sun.
  • on Dec 21.. the South Pole is inclined toward
    the sun
  • on March 21 Sept. 23 neither is inclined
    toward the sun.

72
Effect of Earth's Elliptical Orbit.
  • because the Earth's orbit is an ellipse, the
    distance between the Earth and the sun varies.
  • these changes are too small to have any
    significant affect on the seasons.
  • during Winter in the Northern Hemisphere the
    Earth is closest to the sun.

73
Read pages 99 101.Answer Review Questions p
101, 39-48.Complete Questions for Regents
Practice p. 102.1-19
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