2013
DOI: 10.1117/12.2029432
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The sea and land surface temperature radiometer (SLSTR) detection assembly design and performance

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Cited by 8 publications
(9 citation statements)
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“…Isoradiance lines for the noise (SWIR bands S5 and S6 and MIR bands S7 and F1) and saturation levels (MIR bands S7 and F1) for SLSTR and noise and saturation for the SWIR and MIR bands (M10, M12 and M13) of VIIRS used in the Nightfire algorithm. The SLSTR noise levels were computed using the End-of-Life noise-equivalent differential reflectance (S5 and S6) and noise-equivalent differential temperature levels (S7 and F1) [47] and were 1.5 × 10 −2 , 8.4 × 10 −3 , 2.6 × 10 −4 and 2.1 × 10 −1 W m −2 µm −1 sr −1 for S5, S6, S7 and F1 respectively. A reflectance of 30% as given in the original works [47] was considered, together with irradiance data from SCIAMACHY http://www.iup.uni-bremen.de/UVSAT/Datasets/solar-reference-data [51], to compute the noise levels.…”
Section: Detectionmentioning
confidence: 99%
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“…Isoradiance lines for the noise (SWIR bands S5 and S6 and MIR bands S7 and F1) and saturation levels (MIR bands S7 and F1) for SLSTR and noise and saturation for the SWIR and MIR bands (M10, M12 and M13) of VIIRS used in the Nightfire algorithm. The SLSTR noise levels were computed using the End-of-Life noise-equivalent differential reflectance (S5 and S6) and noise-equivalent differential temperature levels (S7 and F1) [47] and were 1.5 × 10 −2 , 8.4 × 10 −3 , 2.6 × 10 −4 and 2.1 × 10 −1 W m −2 µm −1 sr −1 for S5, S6, S7 and F1 respectively. A reflectance of 30% as given in the original works [47] was considered, together with irradiance data from SCIAMACHY http://www.iup.uni-bremen.de/UVSAT/Datasets/solar-reference-data [51], to compute the noise levels.…”
Section: Detectionmentioning
confidence: 99%
“…The distribution of the SLSTR spectral channels with SWIR, MIR and 2 channels in TIR should allow for the detection and characterisation of GF and other hot spots via the SWIR detection and dual Planck curve fitting methodology. Compared to VIIRS, SLSTR is observing in one additional SWIR channel at night-time and it has better signal-to-noise requirements [47,48]. SLSTR can therefore be expected to detect even smaller and cooler hot targets than VIIRS.…”
Section: Introductionmentioning
confidence: 99%
“…no. cept of uncertainty validation is presented in detail by Corlett et al (2014). Briefly, the standard deviation of the satellite/drifter differences is comprised of contributions from the satellite and drifter measurements, as well as terms to represent the spatial and temporal differences between the two measurements.…”
Section: Evaluation Of Hrsst-1 and Hrsst-2 Driftersmentioning
confidence: 99%
“…These can be used directly to monitor the evolution of the surface ocean on decadal timescales and help quantify the intensity of events such as El Niño/La Niña, as well as being useful to constrain climate reanalyses (e.g., Dee et al, 2014). For these reasons, the importance of monitoring SST was recognized as a priority by the Copernicus program, and a sensor aimed at observing SST was included on Sentinel-3 satellites, the Sea and Land Surface Temperature Radiometer (SLSTR; Coppo et al, 2013). To deliver the SST data product service (Bonekamp et al, 2016), the dual-view capability and onboard calibration of SLSTR give it comparable accuracy to similar sensors, such as the Advanced Along-Track Scanning Radiometer (AATSR;Llewellyn-Jones et al, 2001).…”
Section: Introductionmentioning
confidence: 99%
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