Figure 2.3 Same as Figure 2.1 but for the diffuse solar flux

Figure 2.2 Same as Figure 2.1 but for the direct component of the solar flux

Table 2.6.1 Equation of fit (forced through the origin) and correlation coefficient for Grayling I

SR04-1
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T i m e iS ee iSeroestofetheifDu s e tM e a s u red & CCla lulutedeSoSao lFlr x l u x

T m r e s i f h D f irec M easur e d & a c c a la t d l r a uF

Measured Total Solar

Calculated Total Solar

M e a s u re d D iffus e S o la r

C a lc u la te d D iffu s e S o la r

Fractional DOY

Figure 2.3 Same as Figure 2.1 but for the diffuse solar flux.

Most surface energy budget models, including FASST, utilize only the total solar flux.

Figure 2.4 is a scatter diagram of the total measured and calculated solar flux. A least

square fit to the data and its correlation coefficient, R2, is presented in the figure. The

least square fit has been forced through the origin (0,0).

Grayling I Total Solar Flux

Messured Solar Flux(W/m )

Figure 2.4 Scatter diagram of the total solar measured and calculated flux and the least

square fit to the data.

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