Unformatted text preview: must be peak wavelengths for a blackbody emitter, as well as wavelengths which will make it through the atmosphere without depletion. The IR is related to SST empirically and after processing, the data are plotted on a map like the one here. Difficulties can arise if clouds are present, but several techniques allow us to 'see' through clouds in some cases." Ryan Schuster...
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This note was uploaded on 01/08/2012 for the course MPO 551 taught by Professor Zhang,c during the Summer '08 term at University of Miami.
- Summer '08