Perhaps you may be interested in downward shortwave flux? It isn't easy to compute or measure, but it should capture what you are after. You can use the equation $$R_{net}=S\downarrow-S\uparrow+L\downarrow-L\uparrow$$
where $S$ represents shortwave, $L$ represents longwave, $R_{net}$ is the net radiation, and the arrows depict upward or downward. If you assume an albedo $\alpha$, you can say that $S\uparrow$ is a fraction of $S\downarrow$: $$R_{net}=S\downarrow(1-\alpha)+L\downarrow-L\uparrow$$
If you use an IR thermometer, you can measure the temperature of the sky ($T_{sky}$) and the ground ($T_{ground}$). If you assume a corresponding emissivity (\epsilon), then you can invoke Stefan-Boltzmann's "law" and get $$R_{net}=S\downarrow(1-\alpha)+\sigma\left(\epsilon_{sky}T_{sky}^4-\epsilon_{surface}T_{surface}^4\right)$$.
If you measure $R_{net}$ using a net radiometer, you can solve for $S\downarrow$. Alternatively, you can also compute $S\downarrow$ empirically, like some of the climate models do. But that is perhaps the most computationally intensive part of climate modeling.