4.7 Article

Calibration Inter-Comparison of MODIS and VIIRS Reflective Solar Bands Using Lunar Observations

期刊

REMOTE SENSING
卷 14, 期 19, 页码 -

出版社

MDPI
DOI: 10.3390/rs14194754

关键词

MODIS; VIIRS; solar calibration; lunar calibration; calibration inter-comparison; moon

资金

  1. NASA
  2. NOAA Mission Operation Team for Terra
  3. NOAA Mission Operation Team for Aqua
  4. NOAA Mission Operation Team for SNPP
  5. NOAA Mission Operation Team for N20
  6. NOAA SDR calibration team

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This paper provides an overview of the solar and lunar calibration methodologies used for the on-orbit calibration of the RSB for MODIS and VIIRS satellites. The calibration inter-comparison results derived from regularly scheduled lunar observations are presented and compared with results obtained using Earth-view targets. The paper also discusses the challenges and ongoing efforts for future improvements in lunar calibration and inter-comparison for Earth-observing sensors.
Multispectral band observations from Terra and Aqua MODIS, launched in December 1999 and May 2002, respectively, and from SNPP and NOAA-20 VIIRS, launched in November 2011 and October 2017, respectively, have continuously enabled a broad range of applications and studies of the Earth system and its changes via a set of geophysical and environmental parameters. The quality of MODIS and VIIRS science and environmental data products relies strongly on the calibration accuracy and stability of individual sensors, as well as their calibration consistency, especially for the data products generated using observations from sensors across different platforms. Both MODIS and VIIRS instruments carry a similar set of on-board calibrators for their on-orbit calibration. Besides, lunar observations are regularly scheduled and implemented in support of their reflective solar bands (RSB) calibration, especially their long-term stability monitoring. In this paper, we provide an overview of MODIS and VIIRS solar and lunar calibration methodologies applied for the RSB on-orbit calibration, and describe the approach developed for their calibration inter-comparisons using lunar observations, including corrections for the effects caused by differences in the relative spectral response and adopted solar spectra between individual sensors. The MODIS and VIIRS calibration inter-comparison results derived from their regularly scheduled lunar observations are presented and discussed, including associated uncertainties and a comparison with those derived using the Earth-view targets. Also discussed are remaining challenges in lunar calibration and inter-comparison for the Earth-observing sensors, as well as on-going efforts for future improvements.

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