This preview shows page 1. Sign up to view the full content.
Unformatted text preview: Stefan-Boltzmann Law E BB = T 4 (Eq. 2.5) 2.4: Emission Temperature of a planet, Albedo 2.5: Greenhouse Effect (1-layer model) S 4 (1 " # p ) = T e 4 T s 4 = 2 T e 4 (Eq. 2.11-12) 2.6: Global radiative flux balance 2.7: Distribution of Insolation Q = S d d " # $ % & 2 cos ( s (Eq. 2.14 ) Solar zenith angle cos s = sin sin + cos cos cos h (Eq. 2.16 ) 2.8: Energy balance at the Top of the Atmosphere: Incoming SWR Reflected SWR = Absorbed SWR (ASR) = Outgoing LWR (OLR)...
View Full Document
This test prep was uploaded on 04/02/2008 for the course ATMO 324-501/50 taught by Professor Saravanan during the Fall '08 term at Texas A&M.
- Fall '08