Extraterrestrial Radiation

The radiant energy from the sun is practically the only source of energy that impacts climatic processes on earth. The solar constant, ISC, is the rate of total solar energy at all wavelengths incident on a unit area exposed normally to rays of the sun at a distance of 1 AU from the sun. Quantifying this value has been the object of numerous studies through the years. The value officially adopted by the Commission for Instruments and Methods of Observation in October 1981 is

ISC=1367Wm2=4.921MJm2h1I_{SC} = 1367 W m^{-2} = 4.921 MJm^{-2} h^{-1}

On any given day, the extraterrestrial irradiance (rate of energy) on a surface normal to the rays of the sun, I0nI_{0n}, is:

I0n=ISCE0I_{0n} = I_{SC}E_0 1:1.2.1

whereE0E_0 is the eccentricity correction factor of the earth's orbit, and I0nI_{0n}has the same units as the solar constant,ISCI_{SC}. To calculate the irradiance on a horizontal surface,ISCI_{SC},

To calculate the irradiance on a horizontal surface,I0I_0,

I0=I0ncosθz=ISCE0cosθzI_0 = I_{0n} \cos\theta_z = I_{SC}E_0\cos\theta_z 1:1.2.2

wherecosθzcos\theta_z, is defined in equation 1:1.1.3.

The amount of energy falling on a horizontal surface during a day is given by

H0=SRSSI0dt=20SSI0dtH_0 = \int_{SR}^{SS} I_0dt = 2 \int_0^{SS} I_0dt 1:1.2.3

whereH0H_0 is the extraterrestrial daily irradiation(MJm2d1)(MJ m^{-2} d^{-1}), SR is sunrise, and SS is sunset. Assuming that E0E_0remains constant during the one day time step and converting the time dtdt to the hour angle, the equation can be written

H0=24πISCE00ω.TSR(sinδsinϕ+cosδcosϕcosω.t)dω.t H_0 = \frac{24}{\pi} I_{SC}E_0\int_0^{\omega.T_{SR} }(\sin\delta \sin\phi+\cos\delta\cos\phi\cos\omega.t)d\omega.t 1:1.2.4

or

H0=24πISCE0[ω.TSR(sinδsinϕ+cosδcosϕsin(ω.TSR))] H_0 = \frac{24}{\pi} I_{SC}E_0[{\omega.T_{SR} }(\sin\delta \sin\phi+\cos\delta\cos\phi\sin(\omega.T_{SR}))] 1:1.2.5

where ISCI_{SC} is the solar constant (4.921 MJm2h1MJ m^{-2} h^{-1}), E0_0is the eccentricity correction factor of the earth's orbit, is the angular velocity of the earth's rotation (0.2618radh10.2618 rad h^{-1}), the hour of sunrise, TSRT_{SR}, is defined by equation 1:1.1.4, δ is the solar declination in radians, and is the geographic latitude in radians. Multiplying all the constants together gives

H0=37.59E0[ω.TSRsinδsinϕ+cosδcosϕsin(ω.TSR)] H_0 = 37.59E_0[{\omega.T_{SR} }\sin\delta \sin\phi+\cos\delta\cos\phi\sin(\omega.T_{SR})] 1:1.2.6

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