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Atmospheric Radiation. ESE_GE 152 April 7, 2009 Yuk Yung yly@gps.caltech.edu Chapter 1. Outline. Blackbody Energy Balance (1) Energy Balance (2) Thermal Structure Composition. Blackbody Radiation. B (T) = 2h 3 /c 2 [exp(h/kT) - 1] -1. Brightness Temperature. Outline.
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Atmospheric Radiation ESE_GE 152 April 7, 2009 Yuk Yung yly@gps.caltech.edu Chapter 1
Outline Blackbody Energy Balance (1) Energy Balance (2) Thermal Structure Composition
Blackbody Radiation B(T) = 2h3/c2[exp(h/kT) - 1]-1
Outline Blackbody Energy Balance (1) Energy Balance (2) Thermal Structure Composition
Outline Blackbody Energy Balance (1) Energy Balance (2) Thermal Structure Composition
George Hadley (1685-1768), English lawyer and scientist. “I think the cause of the general Trade-winds have not been explained by any of those who have wrote on that subject” (1735) The overturning Hadley cells are the main way the atmosphere transports energy polewards in low latitudes
Radiation TOA Quite strong structure due to clouds in ASR and OLR that mostly cancels in the net; some other albedo effects (e.g., Sahara) and land-sea differences, but sun-Earth geometry explains most of pattern. ASR OLR NET Trenberth and Stepaniak, J. Clim. 2003
Surface Top-of-atmosphere Top-of-atmosphere Surface Net Differences Shortwave Kiehl and Trenberth 1997
Radiation TOA Quite strong structure due to clouds in ASR and OLR that mostly cancels in the net; some other albedo effects (e.g., Sahara) and land-sea differences, but sun-Earth geometry explains most of pattern. ASR OLR NET Trenberth and Stepaniak, J. Clim. 2003
Outline Blackbody Energy Balance (1) Energy Balance (2) Thermal Structure Composition
Outline Blackbody Energy Balance (1) Energy Balance (2) Thermal Structure Composition
x: Machida et al. [1995] +: Bernard et al. [2006]
Thanks Elva Kuai, Fai Li, Trenberth, Barnet Goody + Yung Book