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(BRAVO) Study: Final Report. - Desert Research Institute

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<strong>Final</strong> <strong>Report</strong> — September 2004<br />

Table 6-6. Multiple regression fits of factor scores and CM to BBEP daily average b ext .<br />

Season<br />

No. of<br />

Days<br />

Adj. R 2<br />

Std. Dev.<br />

of Error<br />

Resulting Equation<br />

Summer 46 0.74 7.6 b ext = 42.6 + 2.6(fRH*F1) + 13.9(F2)<br />

Fall 55 0.88 7.0 b ext = 34.5 + 12.5(fRH*F2) + 4.5(F3) + 2.6(F5)<br />

Despite differences between BIBE1 and BBEP, the factor analysis approach did<br />

demonstrate that PM-fine sources explained most of the variance in optical b ext during<br />

<strong>BRAVO</strong>, and that these sources were associated with many of the components in the<br />

reconstruction equation. In both periods of the study, sulfate-related F 2 (possibly partially<br />

attributed to coal combustion) explained most of the variance in b ext in the regression<br />

formulas in Tables 6-4 and 6-6.<br />

6-14

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