2017
DOI: 10.1080/01431161.2017.1342050
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VIIRS night-time lights

Abstract: The Visible Infrared Imaging Radiometer Suite (VIIRS) Day/Night Band (DNB) collects global low-light imaging data that have significant improvements over comparable data collected for 40 years by the DMSP Operational Linescan System. One of the prominent features of DNB data is the detection of electric lighting present on the Earth's surface. Most of these lights are from human settlements. VIIRS collects source data that could be used to generate monthly and annual science grade global radiance maps of human… Show more

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Cited by 721 publications
(474 citation statements)
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“…These data are radiance calibrated, and consist only of observations that were taken under clear sky conditions (as determined by infrared channels of the VIIRS sensor), and without twilight illumination or stray light [8]. The fall months were chosen based on our experience using the DNB data.…”
Section: Methodsmentioning
confidence: 99%
See 1 more Smart Citation
“…These data are radiance calibrated, and consist only of observations that were taken under clear sky conditions (as determined by infrared channels of the VIIRS sensor), and without twilight illumination or stray light [8]. The fall months were chosen based on our experience using the DNB data.…”
Section: Methodsmentioning
confidence: 99%
“…The US National Oceanic and Atmospheric Administration is currently developing annual based composites, which should be less affected by such errors [8]. To reduce the impact of such events, pixels were therefore only considered lit in a given year if they were above a 3 nW/cm 2 sr threshold in both the October and November composites.…”
Section: Methodsmentioning
confidence: 99%
“…There are several pixels of negative radiance values on the images from monthly composites. These negative radiance values result from the system noise in the dark current correction process [20]. The average northern hemisphere dark night ocean data was utilized in the dark current correction process, but some system noise remained that made some pixels slightly negative in no-light areas [20].…”
Section: Correction Of the Npp-viirs Ntl Datamentioning
confidence: 99%
“…In the past, the façade lighting was sometimes reduced due to a lamp burning out but not being immediately noticed, and there is no record of when lamps were replaced. The isolation of the church makes it possible to directly identify the light coming from the church using data from the Visible Infrared Imaging Radiometer Suite Day-Night Band (VIIRS DNB) instrument on the Suomi NPP satellite [24]. The pixel size of a DNB observation is around 750 m, so to uniquely identify a single lighting installation, it must be well separated from other lights.…”
Section: Prior Lightingmentioning
confidence: 99%