THE SUN AND THE SEASONS 1. Introduction 2. Solar energy 4 ...

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THE SUN AND THE SEASONS 1. Introduction 2. Solar energy 3. Variation and the solar constant 4. Seasons

Transcript of THE SUN AND THE SEASONS 1. Introduction 2. Solar energy 4 ...

Page 1: THE SUN AND THE SEASONS 1. Introduction 2. Solar energy 4 ...

THE SUN AND THE SEASONS

1. Introduction

2. Solar energy

3. Variation and the solar constant

4. Seasons

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LITHOSPHERE

BIOSPHERE

Source: After

Christopherson,

2012, p. 13

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The Solar System. Source: Christopherson, 2012, p. 41.

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Earth-Sun size comparison. Source: Christopherson, 2009, p. 44.

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The Sun imaged by SOHO. Source: Christopherson, 2009, p. 44.

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The Sun imaged by SOHO. Source: Christopherson, 2012, p. 42.

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Energy production in the Sun: hydrogen fusion.

Hydrogen atoms

Helium atom

Energy

Squeezed together by

Sun’s immense gravity

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PROCESSES OF ENERGY TRANSFER:

HOW DOES IT GET FROM (A) TO (B)?

1. Convection: vertical mixing currents

2. Conduction: two surfaces touching

3. Advection: warm or cold air moves

horizontally

4. Radiation: via electromagnetic waves,

making no use of intervening medium

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Wavelength and frequency. Source: Christopherson, 2012, p. 44.

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0.4 µm 0.5 µm 0.6 µm 0.7 µm

Visible light 0.4 to 0.7 µm

The electromagnetic spectrum

Wavelength (λ)

gamma

rays x-rays

ultraviolet

visible light

infrared

microwaves

radio waves

COLOURS OF THE

RAINBOW:

ROY G. BIV

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Solar output by

wavelength.

Source: Christopherson, 2012,

p. 45.

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CAUSES OF VARIABILITY IN SOLAR

ENERGY RECEIVED BY EARTH

1. Solar output

2. Distance from the Sun

3. Atmospheric absorption and reflection

4. Where on Earth? (Sun angle)

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Earth-Sun size comparison. Source: Christopherson, 2009, p. 44.

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Changes in solar output: the effect of sunspots

Sunspots

Emitted solar radiation

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Sunspot numbers and

solar irradiance. Source: Lean, 2010.

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The 11-year

sunspot cycle

and the Maunder

Minimum.

Source: Barry and Chorley, 1992.

Maunder Minimum

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The Little Ice Age, c. 1450-1850.

Caused by the Maunder Minimum??

Figures on a Frozen Canal, Gerrit van Battem, 1670-1680. Source: J. Paul Getty Museum.

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Perihelion

January 3rd Aphelion

July 4th

7% difference in insolation

Distance from the sun also influences solar radiation

received, because the Earth has an elliptical orbit:

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Valley fog and inversion in Salt Lake Valley,

December 2004.

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Valley fog and inversion in Salt Lake Valley,

December 2004.

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Global dimming:

reduced surface

insolation due to

air pollution.

Source: Romanou et al., 2006.

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Estimated global temperature change since 1860.

Source: The heat is on, The Economist, 2011.

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Effects of Earth’s curvature. Source: Christopherson, 2012, p. 46.

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Effects of Earth’s curvature. Source: Mann and Kump, 2009, p. 10.

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DEFINING THE SOLAR CONSTANT:

What variations need to be accounted for?

1. Average INSOLATION

2. Average DISTANCE FROM THE SUN

3. At the SUBSOLAR POINT

4. At the top of the atmosphere

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Taking into account all of these

sources of variation, the solar

constant has been most accurately

measured as

1372 W/m2

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What causes seasons?

Can your explanation account for the

temperature data in the handout?

Is there a better

explanation? How?

YES NO

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Earth’s surface experiences variations in:

•DAY LENGTH

•HEIGHT OF THE SUN IN THE SKY

These variations result from

SEASONAL CHANGES

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Earth’s revolution and rotation. Source: Christopherson, 2012, p. 49.

1 complete revolution

every 365 ¼ days.

1 complete rotation every 24 hours.

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Axial tilt and the plane of the ecliptic.

Source: Christopherson, 2009, p. 53;

see Christopherson, 2012, p. 50.

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Arctic circle

Sun’s rays

EQUINOX:

September 22

EQUINOX:

March 21

SOLSTICE:

June 21

SOLSTICE:

December 21

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Solstices and equinoxes. Source: Christopherson, 2012, p. 51.

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Antarctic circle

66.5° south

Arctic circle

66.5° north

Equator (0°)

Tropic of Cancer

23.5° north

Tropic of Capricorn

23.5° south

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Sun angle changes with seasons. Source: Christopherson, 2012, p. 53.