ese_ge 152 april 7, 2009 yuk yung yly@gpsltech chapter 1
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Atmospheric Radiation. ESE_GE 152 April 7, 2009 Yuk Yung [email protected] 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. - PowerPoint PPT PresentationTRANSCRIPT
ESE_GE 152 April 7, 2009
Yuk Yung
Chapter 1
Atmospheric Radiation
OutlineOutline
Blackbody Energy Balance (1) Energy Balance (2) Thermal Structure Composition
Blackbody Radiation
B(T) = 2h3/c2[exp(h/kT) - 1]-1
Brightness Temperature
OutlineOutline
Blackbody Energy Balance (1) Energy Balance (2) Thermal Structure Composition
Unit = Watts
OutlineOutline
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
68 100
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
Kiehl and Trenberth 1997
Top-of-atmosphere
Surface
Top-of-atmosphere
Surface
Net DifferencesShortwave
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
OutlineOutline
Blackbody Energy Balance (1) Energy Balance (2) Thermal Structure Composition
OutlineOutline
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