Daylight is present at a particular location, to some degree, whenever the Sun is above the local horizon. This is true for slightly more than 50% of the Earth at any given time, since the Earth's atmosphere refracts some sunlight even when the Sun is below the horizon.
Outdoor illuminance varies from 120,000 lux for direct sunlight at noon, which may cause eye pain, to less than 5 lux for thick storm clouds with the Sun at the horizon (even <1 lux for the most extreme case), which may make shadows from distant street lights visible. It may be darker under unusual circumstances like a solar eclipse or very high levels of atmospheric particulates, which include smoke (see New England's Dark Day), dust,1 and volcanic ash.2
For comparison, nighttime illuminance levels are:
For a table of approximate daylight intensity in the Solar System, see sunlight.
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"Volcanic Ash Impacts & Mitigation". USGS. Retrieved 2017-08-01. https://volcanoes.usgs.gov/ash/ ↩
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Bunning, Erwin; Moser, Ilse (April 1969). "Interference of moonlight with the photoperiodic measurement of time by plants, and their adaptive reaction". Proceedings of the National Academy of Sciences of the United States of America. 62 (4): 1018–22. Bibcode:1969PNAS...62.1018B. doi:10.1073/pnas.62.4.1018. PMC 223607. PMID 16591742. https://www.ncbi.nlm.nih.gov/pmc/articles/PMC223607 ↩
Schlyter, Paul (2006). "Radiometry and photometry in astronomy FAQ". http://stjarnhimlen.se/comp/radfaq.html#10 ↩
"Petzl reference system for lighting performance". Archived from the original on 2008-06-20. Retrieved 2007-04-24. https://web.archive.org/web/20080620123040/http://en.petzl.com/petzl/frontoffice/Lampes/static/referentiel/present_referentiel_en.jsp ↩