GERB Ground Calibration Overview and Status J. Rufus

Slides:



Advertisements
Similar presentations
AITA 9, MERTIS Team – MERTIS Calibration, Oct 2007 Folie 1 Development of a calibration concept for the MErcury Thermal Infrared Spectrometer Thomas Saeuberlich,
Advertisements

GOME-2 polarisation data and products L.G. Tilstra (1,2), I. Aben (1), P. Stammes (2) (1) SRON; (2) KNMI GSAG #42, EUMETSAT,
GERB SW fluxes: an update (Clear ocean SW radiances and fluxes in the reprocessed V999 June 04 data) Cédric Bertrand GIST th December, Imperial.
Brown Bag Lunch Lecture ABI Calibration
SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS Science Calibration & Instrument Status TIPS 20 Nov 2003 Last COS TIPS Aug 2003.
Clouds and the Earth’s Radiant Energy System NASA Langley Research Center / Atmospheric Sciences Methodology to compare GERB- CERES filtered radiances.
Pre-launch Characterization of the CERES Flight Model 5 (FM5) Instrument on NPP S. Thomas a, K. J. Priestley b, M. Shankar a, N. P. Smith a, M. G. Timcoe.
Calibration commissioning 16/01/2003: Extended ‘Normal mode’ 282 columns 22/01/2003: TOTAL forward and reverse scans ~11:00-12:15 23/01/2003:Earth stare.
ESTEC July 2000 Estimation of Aerosol Properties from CHRIS-PROBA Data Jeff Settle Environmental Systems Science Centre University of Reading.
In-orbit calibration (TOTAL channel) V space -V IBB Raw Earth V (counts) Raw IBB V (counts) =
Sergey Mekhontsev National Institute of Standards and Technology Optical Technology Division, Gaithersburg, MD Infrared Spectral Radiance Scale.
Plans for interim data release J E Russell (Imperial)
Progress in Chamber Simulation Experiments At UCSD Laser Facility Farrokh Najmabadi Kevin Sequoia, Sophia Chen HAPL Meeting September 24-25, 2003 University.
APOGEE: The Apache Point Observatory Galactic Evolution Experiment l M. P. Ruffoni 1, J. C. Pickering 1, E. Den Hartog 2, G. Nave 3, J. Lawler 2, C. Allende-Prieto.
Yimin Ji - Page 1 October 5, 2010 Global Precipitation Measurement (GPM) mission Precipitation Processing System (PPS) Yimin Ji NASA/GSFC,
Z. P. Szewczyk GIST 25, Oct Recent Field Campaigns with CERES Instruments Z. Peter Szewczyk Kory J. Priestley Lou Smith Remote Sensing of Clouds.
Level 1.5 Processing Issues Martin Bates RAL. Level 1.5 Processing Issues Geolocation –Current Status –TSOL Jitter (CSOL-TSOL) correction –Longterm TSOL.
© Imperial College LondonPage 1 Operations Report/ Operational Calibration Strategy GIST 19, RAL 28th August 2003 J A Hanafin.
18 th GIST Meeting 14 th –16 th May 2003 Ground Segment (GGSPS) Report 1 Commissioning update B.C.Stewart RAL.
1 An Observatory for Ocean, Climate and Environment SAC-D/Aquarius HSC - Radiometric Calibration H Raimondo M Marenchino 7th SAC-D Aquarius Science Meeting.
CERES on Terra & Aqua validation and participation in SCALES Z. Peter Szewczyk G. Louis Smith The GIST 19, RAL 08/27-29, 2003.
Overview of the “Geostationary Earth Radiation Budget (GERB)” Experience. Nicolas Clerbaux Royal Meteorological Institute of Belgium (RMIB) In collaboration.
CDE CDR, September 14, 2004 Your Position, Your Name 1 GATS AIM Science Team Meeting January 23-24, 2007 CIPS Calibration Review, Aimee Merkel, Bill McClintock.
NASA Langley Research Center / Science Directorate CERES SW channel spectral darkening: Rev1 adjustments and beyond Contributors: Norman Loeb, Jennifer.
MSG, GERB calibration and data status May ‘07 J E Russell Imperial College, London
1 5-9 October th ICATPP, Como, Italy S. Maltezos NITROGEN MOLECULAR SPECTRA OF AIR FLUORESCENCE EMULATOR USING A LN 2 COOLED CCD S. Maltezos, E.
19th GIST 27 th -29 th August 2003 E Sawyer RAL Status of GERB1,2,3 and 4 Battery issues Operations during eclipse Stray light NOT bearing life test.
© Imperial College LondonPage 1 Calibration Commissioning Report GIST 19 RAL, 27th August 2003 GERB Instrument Team & Operations Team.
RMIB involvement in the Geostationary Earth Radiation Budget (GERB) and Climate Monitoring SAF projects Nicolas Clerbaux Remote sensing from Space Division.
Imperial studies on spectral signatures: Part I CLARREO meeting, 30 th April-2 nd May, 2008 © Imperial College LondonPage 1 Helen Brindley and John Harries.
1 / 22 Deutscher Wetterdienst Lindenberg Meteorological Observatory Richard Assmann Observatory What final GRUAN observations may consist of and look like.
IBB Calibration Update J. Rufus GIST21 Meeting Boulder, CO. 31 st March – 2 nd April 2004 © Imperial College London.
Introduction NICMOS (Near-Infrared Camera and Multi-Object Spectroscopy) was installed on the Hubble Space Telescope during SM2 in 1997 and has been the.
GIST, Boulder, 31/03/2004 RMIB GERB Processing: overview and status S. Dewitte Royal Meteorological Institute of Belgium.
GERB in-flight calibration Monitoring Instrument Gain.
# x pixels Geometry # Detector elements Detector Element Sizes Array Size Detector Element Sizes # Detector elements Pictorial diagram showing detector.
Bias analysis and correction for MetOp/AVHRR IR channel using AVHRR-IASI inter-comparison Tiejun Chang and Xiangqian Wu GSICS Joint Research and data Working.
A. Ealet Berkeley, december Spectrograph calibration Determination of specifications Calibration strategy Note in
1 CLARREO Advances in Reflected Solar Spectra Calibration Accuracy K. Thome 1, N. Fox 2, G. Kopp 3, J. McCorkel 1, P. Pilewskie 3 1 NASA/Goddard Space.
Thomas C. Stone U.S. Geological Survey, Flagstaff, AZ USA GSICS Research Working Group Meeting EUMETSAT 24−28 March 2014 Using the Moon as a Radiometric.
Aqua-MODIS and VIIRS DCC calibration
Pre-launch Characteristics and Calibration
Validation status overivew
Validation status overivew
In-orbit Microwave Reference Records
Lunar observation data set preparation
V2.0 minus V2.5 RSAS Tangent Height Difference Orbit 3761
An Overview of MODIS Reflective Solar Bands Calibration and Performance Jack Xiong NASA / GSFC GRWG Web Meeting on Reference Instruments and Their Traceability.
Aqua MODIS Reflective Solar Bands (RSB)
Calibration Activities of GCOM-W/AMSR2
AIRS (Atmospheric Infrared Sounder) Instrument Characteristics
OMEGA GROUND CALIBRATION
MODIS Lunar Calibration Data Preparation and Results for GIRO Testing
GERB/CERES comparisons
Instrument Characterization: Status
First Assessments of EUVI Performance on STEREO SECCHI
Characterizing DCC as invariant calibration target
Instrument Considerations
VIS/NIR sub-group discussion
MTF Evaluation of Himawari-8/AHI using Lunar Observations
Changchun Institute of Optics Fine Mechanics and Physics
GSICS MW products and a path forward.?
GOES -12 Imager April 4, 2002 GOES-12 Imager - pre-launch info - radiances - products Timothy J. Schmit et al.
TanSat/CAPI Calibration and validation
Early calibration results of FY-4A/GIIRS during in-orbit testing
Na Xu, Xiuqing Hu, Lin Chen, Min Min
Shanghai Institute of Technical Physics , Chinese Academy of Science
goes-16/17 abi lunar calibration
Lunar irradiance measurement and modelling
MERIS Level 1b processing Ludovic Bourg
Presentation transcript:

GERB Ground Calibration Overview and Status J. Rufus CERES-GIST 21 Meeting Boulder, March 29th – April 2rd 2004 © Imperial College London

Vacuum Calibration Chamber GERB Ground Calibration Overview and Status Vacuum Calibration Chamber Cryogenically pumped high vacuum chamber capable of 10-9 Torr. Earth Orbital Calibration Facility Cleanroom (~60m3) maintained to better than class G (equivalent - class ISO6, 1000) and controlled to 2% relative humidity and 1C. © Imperial College London

GERB Ground Calibration Overview and Status © Imperial College London

GERB Ground Calibration Overview and Status © Imperial College London

How is the instrument modeled? GERB Ground Calibration Overview and Status How is the instrument modeled? Designed to be linear with respect to incoming power. where and This is tested during calibration. © Imperial College London

What are the instrument gains? GERB Ground Calibration Overview and Status What are the instrument gains? We need to measure gains in both channels over all pixels, And since LF(off) ~ 0, © Imperial College London

How is the instrument used? GERB Ground Calibration Overview and Status How is the instrument used? Differences measured to avoid external offset and increase instrument flexibility. A full characterization of the IBB source is important for GERB’s accuracy. Where is GERB ‘looking’? Need and accurate picture of the influence of GERBs optics on the field of view. Crucial to Geolocation of observations. © Imperial College London

Summary of Calibration Aims Check Instrument Linearity. GERB Ground Calibration Overview and Status Summary of Calibration Aims Check Instrument Linearity. Produce Gains for TOT and SW channels. Also measure T, filter response and use these three measurements to determine B, Gain Ratio = A, Long Wave Correction Factor = Characterize IBB Source for all pixels. Measure Instrument FOV Response (PSF, cross talk.) Perform Unit Level Spectral Response Spot Checks. Linearity Gsw GTOT IBB FOV R s (%) 0.05 0.53 0.38 0.2 0.1 PP © Imperial College London

GERB Ground Calibration Overview and Status Linearity Assumption of linear response tested for all GERBs. Results shown for 2 & 3. For total channel WBB-IBB output measured for a range of WBB temperatures, 280 – 345K © Imperial College London

GERB Ground Calibration Overview and Status © Imperial College London

GERB Ground Calibration Overview and Status © Imperial College London

GERB Ground Calibration Overview and Status Measurement of Gains Ground calibration sources have limited spatial extent, 6o E-W across the EV (24o) ~ 60 pixels N-S Measurement at 4 angles and 5+ heights. GTOT Measured using the WBB and CBB with QF out GSW Measured using the VISCs source with QF in. © Imperial College London

Gerb-3 Total Gains GERB Ground Calibration Overview and Status © Imperial College London

Gerb-3 Short Wave Gains GERB Ground Calibration Overview and Status © Imperial College London

IBB Characterization - Method GERB Ground Calibration Overview and Status IBB Characterization - Method © Imperial College London

Produce IBB filtered radiance for all pixels at TIBB. GERB Ground Calibration Overview and Status Produce IBB filtered radiance for all pixels at TIBB. Use linear fit to produce lookup table of data for all pixels and at all temperatures. Over Gerb-3 pixels, © Imperial College London

Setup for FOVR Measurement GERB Ground Calibration Overview and Status Setup for FOVR Measurement © Imperial College London

Setup for FOVR Measurement GERB Ground Calibration Overview and Status Setup for FOVR Measurement © Imperial College London

Normalised response profile of a center Pixel GERB Ground Calibration Overview and Status Normalised response profile of a center Pixel © Imperial College London

Contour profile of a typical center Pixel GERB Ground Calibration Overview and Status Contour profile of a typical center Pixel © Imperial College London

Contour Response of an end Pixel GERB Ground Calibration Overview and Status Contour Response of an end Pixel © Imperial College London

Pixel Viewing Angle GERB Ground Calibration Overview and Status GERB2 Pixel Pointing E-W Pixel Pointing E-W Pixel Pointing N-S Pixel Pointing N-S © Imperial College London

Awaiting return of GERB-3 for pre-launch recalibration. GERB Ground Calibration Overview and Status Calibration Status: Awaiting return of GERB-3 for pre-launch recalibration. Expected after Easter. Investigating correction to LIBB processing Conducting refurbishment VISCS Calibration Source. New lamps and stabilization detectors. Employ detectors to ensure greater IR stability. Planning Refit of the EOCF. © Imperial College London

GERB Ground Calibration Overview and Status Calibration Status: Resolved change in detector alpha’s effect on FOVR measurement – negligible. © Imperial College London