Status report of JMA and calibration policy for AHI. Meteorological Satellite Center of JMA Arata OKUYAMA and Toshiyuki KURINO

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Transcription:

Status report of JMA and calibration policy for AHI Meteorological Satellite Center of JMA Arata OKUYAMA and Toshiyuki KURINO

Contents Update of JMA GSICS members Progress of JMA GRWG activities Infrared channel Visible channel inter-calibration/vicarious calibration Progress of JMA GDWG activities Contribution to SCOPE-CM phase2 projects Towards Himawari-8/AHI inter-calibration VIS/NIR vicarious calibration using Metosat-9/SEVIRI as proxy data Observation quality monitoring Summary and future plans 2

2014 JMA GSICS members Executive Panel (EP) (new) Arata OKUYAMA (Mr) GSICS Research Working Group (GRWG) (new) Ryoko YOSHINO (Dr) (new) Arata OKUYAMA(Mr) Masaya TAKAHASHI (Mr)(now staying at EUMETSAT) GSICS Data management Working Group (GDWG) (new) Keita HOSAKA (Dr) Masaya TAKAHASHI (Mr), vice chair GPRC points of contacts for operational matters (new) Arata OKUYAMA (Mr) We acknowledge EUMETSAT for taking in Masaya as a visiting scientist. 3

Contents Update of JMA GSICS members Progress of JMA GRWG activities Infrared channel Visible channel inter-calibration/vicarious calibration Progress of JMA GDWG activities Contribution to SCOPE-CM phase2 projects Towards Himawari-8/AHI inter-calibration VIS/NIR vicarious calibration using Metosat-9/SEVIRI as proxy data Observation quality monitoring Summary and future plans 4

Progress of the MTSAT IR calibration system on GSICS Current status of MTSAT-1R/-2 IR GSICS Correction Demonstration phase, started in July 2010 Reference sensor: Metop-A/IASI and Aqua/AIRS Toward the Pre-Operational phase Additions and modifications to the netcdf conventions, merge of RAC (Re-Analysis Correction) files To meet the requirement of EUMETSAT bias plotting tool,completed in July 2013 Uncertainty evaluation ongoing, will be completed in 2014 5

Preparation for pre-operational phase WG_13.10 : JMA to complete Uncertainty analysis for MTSAT-IASI products by analyzing random errors contribution from spatial and temporal variability at least Method: Hewison (2013), already evaluated for MSG/SEVIRI and GOES/Imager Progress of MTSAT-2/Imager: Systematic errors have been calculated (but not for full error sources) Random error evaluation is underway (will be finished in 2014) Contribution on each source of systematic error to the standard uncertainty of TB Open Uncertainty of TB [K] 3.8 [μm] 6.8 [μm] 10.8 [μm] ch 12.0 [μm] [K] Total systematic uncertainty Temporal mismatch Longitudinal mismatch Latitudinal mismatch in collaboration with Dr. Tim Hewison at EUMETSAT 6

Comparison of TB bias on the EUMETSAT bias plotting tool Requirements for the visualization on the bias plotting tool RAC data are only supported (all information should be contained in one file) We modified MTSAT-2 vs. AIRS/IASI IR RAC format in July 2013 Easy comparison of GSICS Corrections are realized! Time series of 11μm channel TB difference against Metop- A/IASI on http://vgsics.eumetsat.int/plotter/ MTSAT-2 10.8 um Meteosat-10 10.8 um Many thanks for supports and comments of EUMETSAT and NOAA 7

Progress of the MTSAT VIS calibration system on GSICS A) Vicarious calibration using radiative transfer calculation in collaboration with the University of Tokyo Method: Comparison of observed and simulated radiance for particular targets Target: Wide range of radiances Cloud-free ocean/land, Liquid water cloud, Deep Convective Cloud (DCC) Radiative transfer calculation: RSTAR (Nakajima and Tanaka [1986,1988]) Input data: Independent of GEO data JMA Re-Analysis atmos. profiles, MODIS L1B, BRDF, Aura/OMI total column ozone, Aerosol/Cloud optical parameters (e.g., optical thickness) are retrieved from MODIS L1B data Simulated reflectivity Result of MTSAT-2 in Feb. 2011 Observed reflectivity 8

Progress of the MTSAT VIS calibration system on GSICS B) Inter-calibration of NASA s method using DCC JMA compared MTSAT-2 visible sensor gains computed by two vicarious calibration approaches. a. Deep convective cloud (DCC) observation based approach (used by GSICS Processing and Research Centers) b. Radiative transfer model (RTM) based approach In collaboration with Dr. Sebastien Wagner (EUMETSAT) DCC approach RTM approach MTSAT-2 visible sensor gain trends based on DCC and RTM approaches are consistent, whereas large seasonal variation in the RTM based approach. MTSAT-2 VIS Gain (monthly) [(Radiance)/DN] GSICS correction using DCC will enter the demonstration phase 9

Progress of the MTSAT VIS calibration system on GSICS C) Lunar calibration using the ROLO model In collaboration with Dr. Bartolomeo Viticchie at EUMETSAT Applicable to JMA GEO satellites except for MTSAT-1R (due to its scanning pattern) Experience of GMS-5 lunar calibration with the support of Dr. Tom Stone We got started with MTSAT-2 lunar calibration in this March w/ Dr. Viticchie In the near future, this method will be applied to Himawari-8/AHI VIS/NIR bands Preliminary result of MTSAT-2 lunar calibration using the ROLO model (time series of calibration slope against the ROLO model) 10

Contents Update of JMA GSICS members Progress of JMA GRWG activities Infrared channel Visible channel inter-calibration/vicarious calibration Progress of JMA GDWG activities Contribution to SCOPE-CM phase2 projects Towards Himawari-8/AHI inter-calibration VIS/NIR vicarious calibration using Metosat-9/SEVIRI as proxy data Observation quality monitoring Summary and future plans 11

JMA GPRC website updates JMA GDWG activities URL of JMA GPRC will be changed in 2014. We will announce in the near future. New page describing AHI inter-calibration will be created by the summer 2015. Satellite event log Logs opened to the public on the JMA sites (monthly report): http://mscweb.kishou.go.jp/operation/opr_report.htm Logs before 2000 have been archived, but not digitized Ready for providing information to be hyper-linked from the WMO OSCAR 12

Calibration change alerts Calibration change alert discussed in the June 2013 web meeting We have created prototype image using MTSAT-2 vs. IASI NRTC netcdf and reported to gsics-dev. Prototype of calibration change alert derived from MTSAT-2 vs. IASI NRTC Correction ΔTB [K] 5σ 5σ 10.8 [μm] NRTC product Daily Based on Action EP 14.01 GCC, GDWG and GRWG to evaluate the relevance and implications of adding calibration alert system and SNO and GEO-LEO collocation data to the GSICS portfolio, and report to the Executive Panel. 13

Change of GEO-LEO IR Correction (NetCDF) content Requirements for the visualization on the bias plotting tool RAC files are only supported (all information should be contained in one file) We modified MTSAT-2 vs. AIRS/IASI IR RAC format in July 2013 Easy comparison of GSICS Corrections are realized! NetCDF metadata checker created by NOAA was so useful for the work! Time series of 11μm channel TB difference against Metop- A/IASI on http://vgsics.eumetsat.int/plotter/ MTSAT-2 10.8 um Meteosat-10 10.8 um Many thanks for supports and comments of EUMETSAT and NOAA 14

NetCDF metadata checker Current user: NOAA and JMA (but now we do not use because ) Bash script: controls the validation stylesheet: specifically prepared for each GEO-LEO-IR NetCDF We changed the global attributes in Jul 2013. Maintenance is necessary to catch up this modification. Requirements : 1)The tool can only run on a UNIX (Mac OS X, Linux, etc.) computer. 2)Java virtual machine version 1.4 or newer. 3)Saxon-HE, an open source XSLT/XQuery processor for Java. 4)Command-line utililty ncdump that comes with the netcdf library. The ncdump utility must be able to produce XML representation (option -x) of a netcdf file's content. FYI: Other checker available online/offline (CF-Convention compliance checker for netcdf format ) Online: http://cf-pcmdi.llnl.gov/conformance/compliance-checker Offline (python script): http://pypi.python.org/pypi/cfchecker 15

Contents Update of JMA GSICS members Progress of JMA GRWG activities Infrared channel Visible channel inter-calibration/vicarious calibration Progress of JMA GDWG activities Contribution to SCOPE-CM phase2 projects Towards Himawari-8/AHI inter-calibration VIS/NIR vicarious calibration using Metosat-9/SEVIRI as proxy data Observation quality monitoring Summary and future plans 16

Contribution to SCOPE-CM phase2 projects A possible contribution of GSICS to SCOPE-CM phase 2 project with regard to GEO IR and VIS calibration reprocessing 17

Contents Update of JMA GSICS members Progress of JMA GRWG activities Infrared channel Visible channel inter-calibration/vicarious calibration Progress of JMA GDWG activities Contribution to SCOPE-CM phase2 projects Towards Himawari-8/AHI inter-calibration VIS/NIR vicarious calibration using Metosat-9/SEVIRI as proxy data Observation quality monitoring Summary and future plans 18

Himawari-8/9: Next generation JMA s GEO satellites Information can be found on: http://mscweb.kishou.go.jp/ Advanced Himawari Imager (AHI) Band Central Wavelength [μm] Spatial Resolution 1 0.43-0.48 1Km 2 0.50-0.52 1Km 3 0.63-0.66 0.5Km 4 0.85-0.87 1Km 5 1.60-1.62 2Km 6 2.25-2.27 2Km 7 3.74-3.96 2Km 8 6.06-6.43 2Km 9 6.89-7.01 2Km 10 7.26-7.43 2Km 11 8.44-8.76 2Km 12 9.54-9.72 2Km 13 10.3-10.6 2Km 14 11.1-11.3 2Km 15 12.2-12.5 2Km 16 13.2-13.4 2Km : MSG Himawari : a nickname of JMA s GEO satellites, meaning sunflower in Japanese JMA will launch Himawari-8 in summer 2014 and begin its operation in 2015. The launch of Himawari-9 is also planned in 2016. AHI (Advanced Himawari Imager) has 16 bands 10 minutes for full disk observation, 2.5 minutes around Japan Band as of MTSAT-1R/2 Central Wavelength [μm] Spatial Resolution 1 0.55 0.90 1Km 2 3.50 4.00 4Km 3 6.50-7.00 4Km 4 10.3 11.3 4Km 5 11.5 12.5 4Km 19

A Sequence of Himawari-8/9 AHI Observation in 10 minutes Time Frame This super-rapidscan (every 30 seconds) mode will also be used for the lunar observations _ Full Disk Observation in every 10 min. Over Japan (1) every 2.5 min. Over Japan (2) every 2.5 min. Typhoon monitoring every 2.5 min. Land-mark extraction (1) every 30 sec. Land-mark extraction (2) every 30 sec. A combination of one "Full Disk" and "small sectored scans in 10 minutes 20

On-orbit calibration policy of Himawari-8/9 On-board calibrator Infrared(3.9um to 13.3um): Blackbody Visible/NIR(0.46um to 2.3um): Solar diffuser Vicarious calibration Infrared GSICS standard approach (based on hyper-sounder) Collocation with GEO NIR Moon Ray matching with VIIRS RTM (cloud-free bare land) RTM (liquid cloud) Visible GSICS standard approach (based on DCC observation) Moon Ray matching with VIIRS RTM (cloud-free bare land) RTM (liquid cloud) Other approach candidates --> Future work Simulation on ocean, DCC, sun-glint Moon Deep Convective Cloud RTM simulation Ray-matching with VIIRS

On-orbit calibration of Himawari-8/9 roughschedule preparation monitoring 22

Preparation for Himawari-8 AHI calibration JMA examined availability of RTM based vicarious calibration approach using Metosat-9/SEVIRI data as proxy of Himawari-8/AHI data. The approach is applicable for NIR (1.6um). Regression lines overlaid on all groups of targets in NIR channels as well as the visible channel. The availability is not assessed for 0.46, 0.51 and 2.26 um for Himawari-8 simulation 0.635um + ocean + land + liq.cld. + DCC 0.81um 1.64um Band AHI [um] SEVIRI [um] 1 0.46 2 0.51 3 0.64 0.635 4 0.86 0.81 5 1.6 1.64 + ocean + ocean 6 2.3 + land + land 7 3.9 3.92 + liq.cld. + liq.cld. 8 6.2 6.25 + DCC + DCC 9 7.0 10 7.3 7.35 11 8.6 8.70 12 9.6 9.66 13 10.4 10.8 14 11.2 15 12.3 12.0 16 13.3 13.4 23 observation observation observation Metosat-9/SEVIRI observed and simulated reflectivity JMA appreciate EUMETSAT for their providing the Meteosat- 9/SEVIRI data.

MTSAT calibration system on GSICS IR: - Uncertainty evaluation will be finished in 2014 VIS: - GSICS correction using DCC will enter the demonstration phase - Lunar calibration will implement to the JMA calibration system - RTM based vicarious calibration will continue collaboration research with the Univ. of Tokyo SCOPE-CM phase2 projects Join discussions and re-calibrate GEO data for IOGEO, LAGS and ISCCP projects Himawari-8/9(AHI) Summary and future plans We would like to proceed cooperatively with the GSICS colleagues! Preparation for operational inter/vicarious calibration system Information of GSICS correction will be included in NRT distribution 24

Backup Slides 25

Observation quality monitoring in collaboration with Mr. Peter Miu Calibration change alert discussed in the June 2013 web meeting Diurnal variation of TB biases discussed in the paste F2F/web meetings Bias monitoring using global/regional NWP is under development GEO-GEO inter-comparison will also be carried out, if data are available in JMA Prototype of calibration change alert derived from MTSAT-2 vs. IASI NRTC Correction Diurnal variation of TB biases derived from GEO-LEO IR collocation data MTSAT-2 against Metop-A/IASI Aqua/AIRS ΔTB [K] ΔTB [K] 10.8 [μm] Soft limit ΔTB [K] ΔTB [K] 10.8 [μm] MTSAT-2 against Metop-A/IASI Aqua/AIRS 12.0 [μm] 12.0 [μm] 26

Predicted SRFs(Spectral Response Function) of AHI VIS SWIR NIR MWIR LWIR Himawari-8 MTSAT-2 Available on http://mscweb.kishou.go.jp/himawari89/space_segment/srf_201206/ahi_spectralresponsivity.zip 27

NRT (Near Real Time) distribution with GSICS Information Action EP-12.05: Each GPRC to consider implementing the near real time distribution of both the operational calibration information and the corrected calibration information, as part of the L1 data formats For MTSAT: Difficult to include it due to big impacts on users For Himawari-8/-9: Now under consideration (will be announced in a few month) Tentative plan of calibration information included in Himawari-8/-9 NRT data (The information will be valid when GSICS Correction enters Operational-phase) Correction coefficients against one reference sensor Window period to be used in a regression Ancillary information (text block) Calibration method, reference sensor name, 28

Function enhancement of the bias plotting tool This tool is very useful and convenient for both of users and developers! For users: monitoring what they want, easy comparison of all satellite s observation quality For developers: reduction of costs creating lots of figures, easy detection of the product anomaly by changing data period, monitored temperature, Do we support new GSICS products such as GEO-LEO VIS (DCC) and MW FCDR if the GRWG require? Can we link the calibration alerts to the plotting tool? E.g., time series of TB biases are visualized when users clicked the hyperlink in the calibration alert email (or RSS feed) As for current supported products (i.e., GEO-LEO IR), NOAA s products are not to be integrated (reported by Aleksandar in July 2013 EP meeting). How s the progress? Will CMA THREDDS server also integrate to them? 29

Re-calibration of historical satellites: GMS-5 visible channel re-calibration before 2000 GMS-5: operated from June 1995 to May 2003 Developed vicarious calibration technique cannot be directly applied before 2000 due to a lack of MODIS data Solution: Use of constant/climatological value for optical parameters Preliminary results: show similar tendency, but difference of slope magnitude and some spikes can be useful for comparison with other re-calibration methods w/o MODIS, w/ climatological aerosol w/ MODIS Time series of regression coefficient: slope (monthly mean for detector-2) y = 1.0885 x 0.0039 y = 1.241 x 0.0082 Simulated reflectivity Sep. 2000 Detector-2 DCC Sea Sep. 2000 Detector-2 DCC Cloud Land Sea Observed reflectivity Observed reflectivity 1999 2000 30

Towards demonstration-phase GSICS Correction (NetCDF) filename/contents Will be proposed in the Wednesday s GRWG VIS session by Sebastien and will be checked in the GDWG breakout session Product type: E.g., Re-Analysis Correction (RAC) and Near Real Time Correction (NRTC) for GEO-LEO IR product Should we produce the same kinds of products as the IR correction? Time series of MTSAT-2 DCC digital counts statistics (mode/mean) Monthly average 30-day rolling average on a daily basis 31