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This presentation describes the processes affecting the movement of insolation of energy through the atmosphere and how energy from the Sun is absorbed by the Earth.
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What Happens to Insolation?
Intro to Physical Geography
Energy Basics Energy Pathways and Principles
Shortwave energy in from the Sun (ultraviolet, visible light, and near-infrared)
Longwave energy out from Earth (thermal infrared)
Transmission The passage of energy through atmosphere
or water
Insolation input All radiation received at Earth’s surface –
direct and indirect
What happens to insolation?
Scattering (diffuse radiation) Changing direction of light’s
movement, without altering its wavelengths
Rayleigh scattering makes our skies lookblue
Wavelengths
Wavelength image from Universe by Freedman and Kaufmann.
Because blue light has a shorter wavelength it scatters more easily.
Image from http://missionscience.nasa.gov/ems/09_visiblelight.html
What Happens to Insolation?
Refraction Change in speed and direction of light as
insolation travels from space through the atmosphere
Examples: Rainbows and mirages
What happens to insolation?
Some energy is reflected without being absorbed So we need to think about albedo (how
reflective a surface is) Clouds and aerosols have unpredictable
albedos
What types of surfaces are most reflective? What types of surfaces absorb more energy?
Albedo Values
Clouds and Albedo
Bottom images from http://earthobservatory.nasa.gov/Features/Clouds/clouds4.php
Changes in albedo
What happens to energy that reaches the surface?
Absorption – the assimilation of radiation by molecules of matter and conversion to different kinds of energy.
• Heat is energy produced by the motion of atoms and molecules.
• Heat flows from a region of higher temperature to a region of colder temperature, but not the other way around.
• Four types of heat transfer: • conduction, convection, advection, and
radiation.
Methods of Heat Transfer