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Section3_Slides_v1

Section3_Slides_v1 - Equations governing TOA solar...

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Equations governing TOA solar radiative flux: [governed solely by geometry] δ declination angle (radians) = 23.45 π 180 cos 2 π 365 (172 DOY ) DOY Day of year φ latitude (radians) τ hour angle (radians) = 2 π T h 12 24 ; T h hour of day [0, ..., 23] r ratio of actual to mean Earth-Sun distance = 1 + 0.017cos 2 π 365 (186 DOY ) cos θ = sin δ sin φ
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