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. Author manuscript; available in PMC: 2020 Oct 22.
Published in final edited form as: Geophys Res Lett. 2018 Oct 2;45(19):10,456–10,463. doi: 10.1029/2018GL079031

Figure 1.

Figure 1.

An arbitrary orbit (solar zenith angles lower than 70°) is shown to illustrate (a) local solar times, (b) daily correction factors from Eq.1, (c) observational phase angles, and (d) cloud fraction derived from co-located VIIRS-NPP data.