Visible vicarious calibration using RTM

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Presentation transcript:

Visible vicarious calibration using RTM Masaya Takahashi Meteorological Satellite Center/ Japan Meteorological Agency GRWG/GDWG Annual Meeting, Mar. 04-08, 2013, Williamsburg

Contents Methodology of vicarious calibration using RTM Target selection Consideration for DCC Comparison between Terra/MODIS and Aqua/MODIS GMS-5 re-calibration during pre-MODIS era Comparison of RT simulation between w/ and w/o MODIS Summary and future plan GRWG/GDWG Annual Meeting, Mar. 04-08, 2013, Williamsburg

Methodology Method: Comparison of observed and simulated radiance for four targets Target: Wide range of TBB in order to obtain reliable regression line Cloud-free ocean, Cloud-free land, Liquid water cloud, DCC Radiative transfer calculation: RSTAR (Nakajima and Tanaka [1986,1988]) Input data: Independent from GEO data JMA Re-Analysis atmos. profiles, MODIS L1B, BRDF, Aura/OMI total column ozone, … Result of MTSAT-2 in Feb. 2011 Simulated reflectivity Observed reflectivity This work have been done as part of a research program conducted in collaboration with the University of Tokyo, the visible channel calibrations of GMS and MTSAT satellites. GRWG/GDWG Annual Meeting, Mar. 04-08, 2013, Williamsburg

Target selection Spatially uniform scene Geometrical condition Small standard deviation of DN in a target area Geometrical condition Sun zenith angle, satellite zenith angle are < 60 deg. Exclude near sunglint area Thresholds used in a target selection for MTSAT Cloud-free Sea Cloud-free Land Liquid cloud DCC STDV of DN (5x5km mean) < 6 < 3 < 12 < 15 Optical depth Aerosol for sea, land Cloud for cloud, DCC < 0.3 > 10 & < 40 > 150 TBB of 10.8um ch. >273K > 273K < 205K GRWG/GDWG Annual Meeting, Mar. 04-08, 2013, Williamsburg

Example of crystal shape (Heymsfield, 2002) Consideration for DCC In order to minimize an influence of ice crystal shape uncertainty, hexagonal column for ice crystal shape based on Yang et al. (2000) is adopted. Example of crystal shape (Heymsfield, 2002) Height Particle size Large uncertainty in RT radiance calculation is caused by the difference of hexagonal and spherical shape particle phase function. We introduce the geometrical condition in a target selection: Difference between phase function of hexagonal shape and that of spherical shape is small. GRWG/GDWG Annual Meeting, Mar. 04-08, 2013, Williamsburg

Time series of regression coefficient: slope Result (MTSAT-2) Terra/MODIS Compatible results between Terra and Aqua Some spikes in a time series Due to a small number of target selection? Feb. 2012 Simulated reflectivity DCC Cloud Land Sea Time series of regression coefficient: slope Aqua/MODIS Feb. 2012 Simulated reflectivity DCC Cloud Land Sea 2010 2011 2012 Observed reflectivity GRWG/GDWG Annual Meeting, Mar. 04-08, 2013, Williamsburg

GMS-5 re-calibration during pre-MODIS era Background Calibration of past satellites data is required for climatological use GMS-5: JMA’s geostationary satellite which had been operated from June 1995 to May 2003 Problem Developed calibration technique can’t be applied before 2000 due to a lack of MODIS data Solution Find conditions that optical parameter uncertainty on the RT simulation is small Target: cloud-free ocean, DCC GRWG/GDWG Annual Meeting, Mar. 04-08, 2013, Williamsburg

Target selection and input parameters into RTM w/o MODIS Cloud-free ocean target Radiance sensitivity test using RSTAR ”climatological AOD < 0.1 & sunglint angle > 30 deg." meets the reflectivity error < 0.01 Check whether RT simulation w/ retrieved AOD from MODIS under the conditions satisfies a small reflectivity error 70% of simulated reflectivity: reflectivity error < 0.1 (from 6-months test) DCC Comparison of simulated radiance Cases using cloud ice parameters retrieved from MODIS Cases using constant values: “Cloud ice optical depth: 150, effective radius: log-normal distribution (center: 20um)” Mean TOA radiance difference ≈ 2 W/m^2/sr/um Thresholds of DCC selection TBB of IR 10.8um < 200K, small STDV of DN (for VIS and IR channel) GRWG/GDWG Annual Meeting, Mar. 04-08, 2013, Williamsburg

Preliminary results: w/ MODIS vs. w/o MODIS w/ climatological aerosol Tendency looks like Difference of slope magnitude, some spikes Need of further investigation y = 1.0885 x – 0.0039 Sep. 2000 Detector-2 Simulated reflectivity Time series of regression coefficient: slope (monthly mean for detector-2) DCC Sea w/ MODIS y = 1.241 x – 0.0082 Sep. 2000 Detector-2 Simulated reflectivity DCC Cloud Land Sea 1999 2000 Observed reflectivity GRWG/GDWG Annual Meeting, Mar. 04-08, 2013, Williamsburg

Summary and future plan JMA has been developing visible channel vicarious calibration technique using RTM in collaboration with the University of Tokyo. Re-calibration during pre-MODIS period is underway. Future plan Comparison of other calibration methods Expansion of vicarious calibration technique to NIR channel of AHI (Advanced Himawari Imager) on Himawari-8/-9. use SEVIRI, MODIS, VIIRS as proxy data GRWG/GDWG Annual Meeting, Mar. 04-08, 2013, Williamsburg

Backup slides GRWG/GDWG Annual Meeting, Mar. 04-08, 2013, Williamsburg

"RSTAR" - Radiative Transfer Code Developed by Dr. NAKAJIMA’s Lab. (AORI, Univ. of Tokyo) Algorithm is based on Nakajima and Tanaka [1986,1988] http://www.ccsr.u-tokyo.ac.jp/~clastr/ General package for simulating radiation fields k - distribution method HITRAN2004 database Wavelengths between 0.2m to 200m Absorption and scattering schemes Parallel atmosphere divided into sub-layers Input Sun and view angles Sensor's response function Atmosphere profile Surface condition Output Radiance, irradiance GRWG/GDWG Annual Meeting, Mar. 04-08, 2013, Williamsburg