Abstract

The Visible and Infrared Imaging Radiometer Suite (VIIRS) onboard the Joint Polar Satellite System (JPSS)/Suomi National Polar-Orbiting Partnership (SNPP) satellite provide sensor data records for the retrievals of many environment data records. It is critical to monitor the VIIRS long-term calibration stability to ensure quality EDR retrieval. This study investigates the radiometric calibration stability of the NOAA operational SNPP VIIRS Reflective Solar Bands (RSB) and Day-Night-Band (DNB) using Deep Convective Clouds (DCC). Monthly and semi-monthly DCC time series for 10 moderate resolution bands (M-bands, M1–M5 and M7–M11, March 2013–September 2015), DNB (March 2013–September 2015, low gain stage), and three imagery resolution bands (I-bands, I1–I3, January 2014–September 2015) were developed and analyzed for long-term radiometric calibration stability monitoring. Monthly DCC time series show that M5 and M7 are generally stable, with a stability of 0.4%. DNB has also been stable since May 2013, after its relative response function update, with a stability of 0.5%. The stabilities of M1–M4 are 0.6%–0.8%. Large fluctuations in M1–M4 DCC reflectance were observed since early 2014, correlated with F-factor (calibration coefficients) trend changes during the same period. The stabilities of M8-M11 are from 1.0% to 3.1%, comparable to the natural DCC variability at the shortwave infrared spectrum. DCC mean band ratio time series show that the calibration stabilities of I1–I3 follow closely with M5, M7, and M10. Relative calibration changes were observed in M1/M4 and M5/M7 DCC mean band ratio time series. The DCC time series are generally consistent with results from the VIIRS validation sites and VIIRS/MODIS (the Moderate-resolution Imaging Spectroradiometer) simultaneous nadir overpass time series. Semi-monthly DCC time series for RSB M-bands and DNB were compared with monthly DCC time series. The results indicate that semi-monthly DCC time series are useful for stability monitoring at higher temporal resolution.

Highlights

  • The Visible and Infrared Imaging Radiometer Suite (VIIRS) onboard the Joint Polar SatelliteSystem (JPSS)/Suomi National Polar-Orbiting Partnership (SNPP) satellite has 22 spectral bands, with14 Reflective Solar Bands (RSB), 7 Thermal Emissive Bands (TEB) and 1 Day-Night-Band (DNB) [1,2].VIIRS RSBs are calibrated using a full-aperture Solar Diffuser (SD) and the degradation of SD is Remote Sens. 2016, 8, 32; doi:10.3390/rs8010032 www.mdpi.com/journal/remotesensingRemote Sens. 2016, 8, 32 monitored by a Solar Diffuser Stability Monitor (SDSM)

  • [14] Deep Convective Clouds (DCC) radiometric sensitivity studies based on VIIRS bands M5, M7, and I2 DCCs indicated that the mode of DCC reflectance is more stable in terms of spatial resolution, TB11 threshold and calibration bias, and DCC cluster size

  • We investigated the feasibility of splitting monthly DCC datasets to monitor the VIIRS calibration stability at a higher temporal resolution from April to November, while monthly DCCs are continued to be used for the remaining months

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Summary

Introduction

The Visible and Infrared Imaging Radiometer Suite (VIIRS) onboard the Joint Polar SatelliteSystem (JPSS)/Suomi National Polar-Orbiting Partnership (SNPP) satellite has 22 spectral bands, with14 Reflective Solar Bands (RSB), 7 Thermal Emissive Bands (TEB) and 1 Day-Night-Band (DNB) [1,2].VIIRS RSBs are calibrated using a full-aperture Solar Diffuser (SD) and the degradation of SD is Remote Sens. 2016, 8, 32; doi:10.3390/rs8010032 www.mdpi.com/journal/remotesensingRemote Sens. 2016, 8, 32 monitored by a Solar Diffuser Stability Monitor (SDSM). The Visible and Infrared Imaging Radiometer Suite (VIIRS) onboard the Joint Polar Satellite. VIIRS RSBs are calibrated using a full-aperture Solar Diffuser (SD) and the degradation of SD is Remote Sens. 2016, 8, 32 monitored by a Solar Diffuser Stability Monitor (SDSM). Telescope Assembly (RTA) mirror degradations were observed, especially early after launch. The rate of RTA mirror and SD degradations has decreased since mid-2013 and early 2014, respectively. Their impacts on the instrument performance are negligible (at 0.1% level) due to weekly updates of RSB calibration coefficients (F-factor) Look-Up Table (LUT) [3,4]. Larger F-factor fluctuations have been observed since early 2014 in some shorter wavelength bands, with band M1 fluctuating the most (~3%).

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