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IF YOU EQUATE THE INCOMING RADIATION TO OUTGOING RADIATION, YOU CAN SOLVE FOR THE TEMPERATURE TO GET EQUATION Te ï½ 4 ( So / 4)(1 ï ï¡ p ) ï³ ï¢ This is the emission temperature which is the temperature that the earth needs to maintain energy balance. ï¢ 1. It depends on the solar constant and albedo of earth. ï¢ 2. Emission temperiture for earth ~ 255K (ï18 ï°C)
