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What Cause the Four Seasons? . Review of last lecture. What is energy? 3 methods of energy transfer The names of the 6 wavelength categories in the electromagnetic radiation spectrum Intensity of radiation (Stefan-Boltzman law): I= T 4
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Review of last lecture • What is energy? 3 methods of energy transfer • The names of the 6 wavelength categories in the electromagnetic radiation spectrum • Intensity of radiation (Stefan-Boltzman law): I=T4 • Wavelength of radiation (Wein’s law): max = b/T • The wavelength range of Sun (shortwave) and Earth (longwave) radition • The 11-year solar cycle
Earth’s orbit around the Sun Distance from the sun accounts for only 7% change in radiation receipt, which is not the cause of seasons.
Revolution vs. Rotation • Revolution: about a body (the earth revolves around the sun; i.e., a year) • Rotation: about an axis (The earth rotates about its axis; i.e., a day) • So what causes the seasons?!?!
The 4-seasons is caused by the Earth’s 23.5o tilt from the line perpendicular to its orbit plane (toward the sun during summer)
Video: Mechanism of the seasons • http://www.youtube.com/watch?v=WLRA87TKXLM
How the changing orientation of the Earth directly affects the receipt of insolation: • Length of Daylight period • Angle at which sunlight hits the surface (“Beam Spreading”) • Thickness of atmosphere through which sunlight must travel (“Beam Depletion)
Length of Daylight Period Equinoxes June Solstice • Day length increases from equator to pole in summer hemisphere • opposite in winter • At least one day of 24-hour sunlight/darkness above Arctic/Antarctic circles, depending on season
Beam Spreading • Beam spreading: the increase in surface area over which radiation is distributed in response to a decrease of solar angle • The greater the spreading, the less intense the radiation (and vice versa)
The 4-seasons is caused by the Earth’s 23.5o tilt from the line perpendicular to its orbit plane (toward the sun during summer)
Change of Earh’s orbit at longer time scales - The Milankovitch cycles • Named after Serbian geophysicist and astronomer Milutin Milankovic, who mathematically theorized that variations in eccentricity, axial tilt and precession of the Earth’s orbit affect Earth’s climate Milutin Milankovic (1879-1958)
Eccentricity: shape of orbit varies between a circle and a thin oval on a 100,000 year cycle • Axial tilt with respect to orbit plane: varies between 21.5o and 24.5o on a 41,000 year cycle • Precession: direction of axis varies on a 20,000 year cycle
Summary • The two basic motions of the Earth • What causes the four seasons: the Earth’s tilt and the 3 ways it affects the solar insolation (change of length of the day, beam spreading, beam depletion) • Change of the Earth’s orbit at longer time scales (Milankovitch cycles): eccentricity, axial tilt, and precession