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Solar radiation (light) strikes Earth's surface throughout the daylight hours. Radiation (heat or infrared) also leaves the Earth during daylight and at night. Averaged over time and space, these downward and upward energy fluxes are equal. If they were not, our planet would gradually heat up or gradually cool down. But the surface of our planet is not simply a mirror for radiation. Some of the incoming radiation goes through a process of change before it is radiated back into space. In this lesson, students will analyze plots of temperature and radiation data to determine change over time.
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Intended for grade levels:
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Technical requirements:
No specific technical requirements, just a browser required
Cost / Copyright:
No cost
This product is free and clear for general use.
DLESE Catalog ID:
MYND-000-000-000-058
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Educational standards:
Resource contact / Creator / Publisher:
Contact:
Dr Lin Chambers NASA |