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Chapter 2 The Energy Cycle

Chapter 2 The Energy Cycle. ATMO 1300 FALL 2009. Why Study Solar Radiation?. The sun is the ultimate source of energy for atmospheric processes. Important concepts: the energy balance (what goes in/out?) satellite imagery atmospheric motion. Basics: Law of Motion.

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1.37k views • 79 slides

Seasons and Sun

Seasons and Sun. Sun Angle and Solar Heating Investigation 3, Part 3. Lesson Objective: I can explain how beam spreading affects the temperature of the Earth in different locations. The tilt of Earth’s axis produces changes in day length over the course of a year. Review.

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594 views • 28 slides

The incoming solar energy

The incoming solar energy . Review of last lecture. The standard units of measurements (SI) Earth ’ s three atmospheres: 1st: 4.6 billion years ago, H, He, magnetic field, volcano 2nd: 4 billion years ago, CO 2 , H 2 O, N 2 , life, ocean 3rd: 400 million years ago, O 2 , land

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455 views • 21 slides

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