Unit 4: Sun-Earth Relationships
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Revolution Rotation Declination (Tilt of Earth’s Axis) Seasons Time Zones Insolation and its variation - PowerPoint PPT Presentation


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Unit 4: Sun-Earth Relationships. Revolution Rotation Declination (Tilt of Earth’s Axis) Seasons Time Zones Insolation and its variation. Sunrise over the Earth. Source: http://ajorbahman.blogspot.com/2011/02/third-of-russians-think-sun-spins-round.html. OBJECTIVES

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Unit 4: Sun-Earth Relationships

  • Revolution

  • Rotation

  • Declination (Tilt of Earth’s Axis)

  • Seasons

  • Time Zones

  • Insolation and its variation

Sunrise over the Earth. Source: http://ajorbahman.blogspot.com/2011/02/third-of-russians-think-sun-spins-round.html


  • OBJECTIVES

  • Examine the Earth’s motions relative to the Sun

  • Demonstrate the consequences of the Earth’s axis tilt for the annual march of the seasons

  • Introduce the time and spatial variations in solar radiation received at surface locations


  • Revolution of the Earth around the Sun

  • Perihelion-closest to Sun Jan. 3rd

  • Aphelion-farthest from Sun July 4th

  • Distance differences from Sun do not influence amount of solar energy received significantly

Earth revolves around the Sun in an elliptical path. Earth and Sun are not drawn to scale, and the orbit’s elongation is highly exaggerated for clarity.



Video shows misconceptions about the cause of the seasons. http://www.youtube.com/watch?v=iMEfYLvxioc


Midnight Sun: Within the Arctic and Antarctic Circle the Sun does not set at Summer Solstice




World’s Time Zones

Source: http://www.colourbox.com/vector/clocks-in-people-head-vector-invitation-card-vector-3095601

Why are the boundaries not straight lines?

Why are the Prime Meridian, International Dateline significant?



Intensity of Sunlight

Source: http://nsidc.org/cryosphere/frozenground/what_affects_fg.html

Reception of solar radiation at different latitudes showing direct, indirect rays


Relationship between solar noon altitude and daylight hours

Daylength (left axis) and noon solar altitude (right axis) at 45° north latitude. These factors work together in producing pronounced seasonality at middle and high latitudes. Notice also how the pace of change in both is much greater near the equinoxes than near the depths of summer and winter.



Spatial distribution of insolation at top of the atmosphere as percentage of global average

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Seasonal and spatial variation in solar radiation reaching the top of the atmosphere as a percentage of the global average. The latitude axis is scaled to acount for shrinking area at higher latitudes. Compare with patterns of the previous figures to see how solar position modulates the effect of daylength.


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