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The Stefan-Boltzmann Law is a fundamental law of physics. In this lesson, students will use this law and the near-ground air temperature to compute the hourly irradiance emitted by the surface of Earth. Then comparisons will be made with actual observations of this variable, called upwelling terrestrial radiation.
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Intended for grade levels:
Type of resource:
Subject:
Technical requirements:
No specific technical requirements, just a browser required
Cost / Copyright:
No cost
Copyright 2005 Board of Regents of the University of Oklahoma. All Rights Reserved.
DLESE Catalog ID:
DLESE-000-000-008-759
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Educational standards:
Resource contact / Creator / Publisher:
Publisher:
Oklahoma Climatological Survey EarthStorm Educational Outreach http://earthstorm.ocs.ou.edu/default.php
Contact:
Andrea Melvin EarthStorm Oklahoma Climatological Survey |