2018
DOI: 10.5194/amt-11-939-2018
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Intercalibration between HIRS/2 and HIRS/3 channel 12 based on physical considerations

Abstract: Abstract. High-resolution Infrared Radiation Sounder (HIRS) brightness temperatures at channel 12 (T 12 ) can be used to assess the water vapour content of the upper troposphere. The transition from HIRS/2 to HIRS/3 in 1999 involved a shift in the central wavelength of channel 12 from 6.7 to 6.5 µm, causing a discontinuity in the time series of T 12 . To understand the impact of this change in the measured brightness temperatures, we have performed radiative transfer calculations for channel 12 of HIRS/2 and H… Show more

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Cited by 4 publications
(15 citation statements)
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References 16 publications
(30 reference statements)
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“…The filters for channels 1-12 are located close to the central axis of the filter wheel, whereas the filters for the remaining channels are located close to the outer edge. The order in which the channels are measured is: 1,17,2,3,13,4,18,11,19,7,8,20,10,14,6,5,15,12,16, and 9. HIRS detects radiation using three different detectors: a Mercury Cadmium Telluride (HgCdTe) detector receives radiation for longwave (wavelength λ > 6 µm) channels 1 to 12, an Indium Antimonide (InSb) detector for shortwave (λ < 5 µm) channels 13 to 19, and a silicon photodiode for the visible channel 20.…”
Section: Hirs Channels and Calibrationmentioning
confidence: 99%
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“…The filters for channels 1-12 are located close to the central axis of the filter wheel, whereas the filters for the remaining channels are located close to the outer edge. The order in which the channels are measured is: 1,17,2,3,13,4,18,11,19,7,8,20,10,14,6,5,15,12,16, and 9. HIRS detects radiation using three different detectors: a Mercury Cadmium Telluride (HgCdTe) detector receives radiation for longwave (wavelength λ > 6 µm) channels 1 to 12, an Indium Antimonide (InSb) detector for shortwave (λ < 5 µm) channels 13 to 19, and a silicon photodiode for the visible channel 20.…”
Section: Hirs Channels and Calibrationmentioning
confidence: 99%
“…Other sensors with a clear temporal evolution are NOAA-6 and -7 (inter-detector and InSb), NOAA-8 (inter-detector), NOAA-9 (HgCdTe), and NOAA-12 (inter-detector). The behaviour in recent sensors (NOAA-18 onward) appears more stable, although the error correlation in Metop-A and -B increases somewhat for the InSb detector (channels [13][14][15][16][17][18][19], and in MetOp-B decreases somewhat for the HgCdTe detector (channels 1-12). Pearson product-moment correlation between the error in different channels for all HIRS satellites.…”
Section: Correlated Errormentioning
confidence: 99%
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“…The authors came up with a second statistical correction procedure that brings HIRS 3 levels down to HIRS 2 levels, which takes effect at cold temperatures when T 12 < 235 K. The method appeared to correct satisfactorily the low T 12 values, such that jumps in the time series from HIRS 2 to HIRS 3 where no longer apparent at the low T 12 temperature range. Very recently, Gierens et al (2018) tested the physics behind the statistical inter-calibration of Shi and Bates (2011), wondering whether it is right from a physical point of view to combine measurements by two instruments which sense different layers of the upper atmosphere. They compared T 12 data calculated by radiative transfer modelling of large sets of temperature and relative humidity profiles, using the HIRS 2 and HIRS 3 spectral response functions.…”
Section: Introductionmentioning
confidence: 99%