New multispectrum fitting software used at DLR for analysis of laboratory Fourier-Transform molecular spectra Joep Loos, Manfred Birk, Georg Wagner German.

Slides:



Advertisements
Similar presentations
ECMWF/EUMETSAT NWP-SAF Satellite data assimilation Training Course
Advertisements

D. Chris Benner and V Malathy Devi College of William and Mary Charles E. Miller, Linda R. Brown and Robert A. Toth Jet Propulsion Laboratory Self- and.
Greenhouse gases Observing SATellite Observing SATellite 29 March 2011 Hyper Spectral Workshop The ACOS/GOSAT Experience David Crisp JPL/CALTECH.
Spectral shapes modeling and remote sensing of greenhouse gases. Toward the OCO and GOSAT experiments and future HITRAN issues.
Georg Wagner, Manfred Birk Remote Sensing Technology Institute (IMF) Deutsches Zentrum für Luft- und Raumfahrt (DLR) Shepard A. Clough Clough Radiation.
ACE Linelist Needs for the Atmospheric Chemistry Experiment Chris Boone and Peter Bernath Univ. of Waterloo, Waterloo, Ontario, Canada HITRAN 2006 Conference.
Microwindow Selection for the MIPAS Reduced Resolution Mode INTRODUCTION Microwindows are the small subsets of the complete MIPAS spectrum which are used.
Page 1 ENVISAT Symposium – Salzburg - Austria 6-10 September 2004 GEO-MTR: A 2-Dimensional Multi Target Retrieval System for MIPAS/ENVISAT Observations.
ACE Spectroscopic Issues for the Atmospheric Chemistry Experiment (ACE) Chris Boone, Kaley Walker, and Peter Bernath HITRAN meeting June, 2008.
PRESSURE BROADENING AND SHIFT COEFFICIENTS FOR THE BAND OF 12 C 16 O 2 NEAR 6348 cm -1 D. CHRIS BENNER and V MALATHY DEVI Department of Physics,
A Channel Selection Method for CO 2 Retrieval Using Information Content Analysis Le Kuai 1, Vijay Natraj 1, Run-Lie Shia 1, Charles Miller 2, Yuk Yung.
CAVIAR Meeting September ASSESSMENT OF H 2 O LINE INTENSITIES.
Jet Propulsion Laboratory California Institute of Technology 1 V-1 11 th HITRAN Conference, Cambridge, MA, June 16-18, 2010 The importance of being earnest.
Molecular Databases: Evolution and Revolution Laurence S. Rothman Iouli E. Gordon Harvard-Smithsonian Center for Astrophysics Atomic and Molecular Physics.
“Questions in peak bagging” 1)Two components: leakage matrix & spectral line profile - do we have sufficient accuracy? (simulated data sufficiently real?)
SPECTRA, an Internet Accessible Information System for Spectroscopy of Atmospheric Gases Semen MIKHAILENKO, Yurii BABIKOV, Vladimir.
A new approach to eliminate the broadband absorption in DOAS spectra M. Ródenas 1, E. Soria 2, J.D. Martín 2 1 Fundación CEAM, EUPHORE Labs, Paterna,
11 Collisional effects on spectral shapes and remote sensing H. Tran LISA, CNRS UMR 7583, Université Paris-Est Créteil and Université Paris Diderot
Jet Propulsion Laboratory California Institute of Technology The College of William and MaryUniversity of Lethbridge.
Remote Sensing Technology Institute 1 HITRAN 2006 Conference, Cambridge MA, June 26th-28th 2006 Water Pressure Broadening: A Never-ending Story Georg Wagner,
Solar observation modes: Commissioning and operational C. Vocks and G. Mann 1. Spectrometer and imaging modes 2. Commissioning proposals 3. Operational.
Blue: Histogram of normalised deviation from “true” value; Red: Gaussian fit to histogram Presented at ESA Hyperspectral Workshop 2010, March 16-19, Frascati,
Spectral Line Parameters Including Temperature Dependences of N 2 - and Self-broadened Widths in the Region of the 9 band of C 2 H 6 using a Multispectrum.
Self- and Air-Broadening, Shifts, and Line Mixing in the ν 2 Band of CH 4 M. A. H. Smith 1, D. Chris Benner 2, V. Malathy Devi 2, and A. Predoi-Cross 3.
Self- and air-broadened line shape parameters in the band of 12 CH 4 : cm -1 V. Malathy Devi Department of Physics The College of William.
Laboratory spectroscopy at DLR Manfred Birk, Georg Wagner, Joep Loos German Aerospace Center (DLR) > 2014 GEISA Workshop > J. Loos Laboratory spectroscopy.
ACE Spectroscopy for the Atmospheric Chemistry Experiment (ACE) Chris Boone, Kaley Walker, and Peter Bernath HITRAN Meeting June, 2010.
US Planck Data Analysis Review 1 Christopher CantalupoUS Planck Data Analysis Review 9–10 May 2006 CTP Working Group Presented by Christopher Cantalupo.
Direct Sun measurements of NO 2 column abundances from Table Mountain, California: Retrieval method and intercomparison of low and high resolution spectrometers.
Pressure Broadening and Spectral Overlap in the Millimeter Wave Spectrum of Ozone International Symposium on Molecular Spectroscopy 65 th Meeting — June.
Alex A. TakedaAug. 18, 2010 Mentor Dr. Alexander Kutyrev.
Methyl Bromide : Spectroscopic line parameters in the 10-μm region D. Jacquemart 1, N. Lacome 1, F. Kwabia-Tchana 1, I. Kleiner 2 1 Laboratoire de Dynamique,
© Crown copyright Met Office Radiation scheme for Earth’s atmosphere …and what might not work for exoplanets James Manners 6/12/11.
Measuring Magnetic fields in Ultracool stars & Brown dwarfs Dong-hyun Lee.
Recent Developments in FT Laboratory Spectroscopy at DLR Manfred Birk, Georg Wagner, Joep Loos German Aerospace Center, Remote Sensing Technology Institute.
Hyperspectral remote sensing
MOS Data Reduction Michael Balogh University of Durham.
1 Atmospheric Radiation – Lecture 7 PHY Lecture 7 Thermal Radiation.
CO 2 Lineshapes Near 2060nm Thinh Q. Bui California Institute of Technology ISMS 2014.
H 2 O retrieval from S5 NIR K. Weigel, M. Reuter, S. Noël, H. Bovensmann, and J. P. Burrows University of Bremen, Institute of Environmental Physics
Manfred Birk, Georg Wagner Remote Sensing Technology Institute (IMF) Deutsches Zentrum für Luft- und Raumfahrt (DLR) Lorenzo Lodi, Jonathan Tennyson Department.
69th Meeting - Champaign-Urbana, Illinois, 2014 FE11 1/12 JPL Progress Report Keeyoon Sung, Geoffrey C. Toon, Linda R. Brown Jet Propulsion Laboratory,
SELF- AND CO 2 -BROADENED LINE SHAPE PARAMETERS FOR THE 2 AND 3 BANDS OF HDO V. MALATHY DEVI, D. CHRIS BENNER, Department of Physics, College of William.
TEMPERATURE DEPENDENCES OF AIR-BROADENING AND SHIFT PARAMETERS IN THE ν 3 BAND OF OZONE M. A. H. SMITH NASA Langley Research Center, Hampton, VA
Infrared Spectra of N 2 -broadened 13 CH 4 at Titan Atmospheric Temperatures Mary Ann H. Smith 1, Keeyoon Sung 2, Linda R. Brown 2, Timothy J. Crawford.
MDTERP MarylanD TErrestial Radiation Package A Narrow-Band Longwave Radiation Model with a Graphical User Interface Robert G. Ellingson and Ezra Takara.
FTS Studies Of The Isotopologues Of CO 2 Toward Creating A Complete And Highly Accurate Reference Standard Ben Elliott, Keeyoon Sung, Charles Miller JPL,
HYMN 2nd annual meeting FTIR Introduction/Overview A.K. Petersen, J. Notholt, T. Warneke Hydrogen, Methane and Nitrous oxide: Trend variability, budgets.
EXPERIMENTAL TRANSMISSION SPECTRA OF HOT AMMONIA IN THE INFRARED Monday, June 22 nd 2015 ISMS 70 th Meeting Champaign, Illinois EXPERIMENTAL TRANSMISSION.
Page 1 COST 723 – Opening Workshop - ESTEC March 2004 GEO-MTR: A 2-Dimensional Multi Target Retrieval System for MIPAS/ENVISAT observations Bianca.
Rutherford Appleton Laboratory Requirements Consolidation of the Near-Infrared Channel of the GMES-Sentinel-5 UVNS Instrument: Initial trade-off: Height-resolved.
JWST Spectroscopy of transiting planets Drake Deming University of Maryland at College Park K2 Science Conference, November 5, 2015.
Concentration Dependence of Line Shapes in the Band of Acetylene Matthew Cich, Damien Forthomme, Greg Hall, Chris McRaven, Trevor Sears, Sylvestre.
Digital Imaging and Remote Sensing Laboratory thermal infrared data 1 Processing of TIMS data to emissivity spectra TIMS bands for this analysis 8.407,
ECMWF/EUMETSAT NWP-SAF Satellite data assimilation Training Course
> ISMS 2017 > Joep Loos • P2355: Experimental line list of water vapor > Experimental line list of water vapor absorption lines in the spectral.
A.Zanichelli, B.Garilli, M.Scodeggio, D.Rizzo
A New Technique for Sidelobe Suppression in OFDM Systems
Erin M. Adkins, Zachary D. Reed, and Joseph T. Hodges
Hyperspectral Sensing – Imaging Spectroscopy
Recent progress on Labfit: a robust multispectrum analysis program for fitting lineshapes including the HTP model and temperature dependence Matthew J.
HITRANonline: A New Structure and Interface for HITRAN
Undiscovered errors of Voigt profile beyond tiny W-shaped residuals
Erin M. Adkins, Melanie Ghysels, David A. Long, and Joseph T. Hodges
Photoacoustic Spectroscopy of the Oxygen A-band
Z. Reed,* O. Polyansky,† J. Hodges*
“Brief” update on ACE water vapour
Authors: B.Kerridge, R.Siddans, J.Reburn, B.Latter and V.Jay
Calculations and first quantitative laboratory measurements of O2 A-band electric quadrupole line intensities and positions 16O2 b(1) ← X (1) PQ(11) magnetic.
ATMOSPHERIC TEMPERATURE SOUNDING
Presentation transcript:

New multispectrum fitting software used at DLR for analysis of laboratory Fourier-Transform molecular spectra Joep Loos, Manfred Birk, Georg Wagner German Aerospace Center, Remote Sensing Technology Institute > 13 th International HITRAN Conference > J. Loos New multispectrum fitting software used at DLR > June 24, 2014DLR.de Chart 1

Absorption cross sections or line-by-line data? > 13 th International HITRAN Conference > J. Loos New multispectrum fitting software used at DLR > June 24, 2014DLR.de Chart 2 High measurement effort Higher resolution necessary Low analysis effort Only interpolation  e.g. HFCs, CFCs Baseline less critical Less measurements needed Extrapolation possible (to some extent) Low line density Error parametrization accessible  e.g. CO, NO, H2O

Why multispectral fitting? > 13 th International HITRAN Conference > J. Loos New multispectrum fitting software used at DLR > June 24, 2014DLR.de Chart 3 „Classical“ analysis: single spectrum fitting FitMAS, LINEFIT, tool by MB/GW, … Multispectral analysis Computationally inexpensive Quality assessment accessible:  Chi-Test, filecuts Test of data reduction model possible Error covariances lost Computationally extensive Quality assessment difficult: only spectral residuals Data reduction model has to be known decorrelates various parameters opaque and blended lines can be fitted

Single spectrum fitting + consecutive data reduction = sound method for generation of spectroscopic data Complexity and computation time requirements restrict multispectral fit to small spectral intervals Temperature and number density fit requires large spectral range  restricted to single spectrum fits Multispectrum fit yields higher precision in many cases Multispectrum fit can give higher accuracy in some cases Multispectrum fit enables fitting of parameters not accessible to single spectral analysis e.g. speed-dependence  Fusion of multispectrum and single spectrum fit to combine advantages Multispectrum vs single spectrum fitting > 13 th International HITRAN Conference > J. Loos New multispectrum fitting software used at DLR > June 24, 2014DLR.de Chart 4

Line models Voigt Speed-dependent Voigt (C. Boone) Speed-dependent Galatry + LM (F. Hase) pCqSDHC + LM (Ngo, Tran) Humlicek by Kuntz & Ruyten for Boone and Tran Versatile interactive mode Choice of line model, fitparameters ILS, calibration factors, baseline, channelling, … Automatic mode Microwindow-, spectra-, fitparameter selection (Voigt) Chi-test of spectral residuals Residua analysis similar to MIPAS/ENVISAT REC analsis by Anu Dudhia planned Single spectrum fitting Temperature/number density fit Filecuts (results of single-spectra-fits vs. ms-fit) Identification of systematic spectrum-specific errors Identification/prevention of correlation between fitted parameters Identification of source of information What can the new software do? > 13 th International HITRAN Conference > J. Loos New multispectrum fitting software used at DLR > June 24, 2014DLR.de Chart 5 Filecut

How does it look like? > 13 th International HITRAN Conference > J. Loos New multispectrum fitting software used at DLR > June 24, 2014DLR.de Chart 6

Example: Speed-dependent analysis of H 2 O 2 band > 13 th International HITRAN Conference > J. Loos New multispectrum fitting software used at DLR > June 24, 2014DLR.de Chart 7

Example: Speed-dependent analysis of H 2 O 2 band > 13 th International HITRAN Conference > J. Loos New multispectrum fitting software used at DLR > June 24, 2014DLR.de Chart 8 Voigt: w-shaped residuals for non-opaque lines Voigt: line-wing residuals for opaque lines Fitted broadening parameters systemitically larger when fitted with SDV  Opaque lines are modelled too narrow Influence of narrowing larger when broadening parameter lower (higher J)

Example: Line mixing of N 2 O 3 band > 13 th International HITRAN Conference > J. Loos New multispectrum fitting software used at DLR > June 24, 2014DLR.de Chart 9

Example: Line mixing of N 2 O 3 band > 13 th International HITRAN Conference > J. Loos New multispectrum fitting software used at DLR > June 24, 2014DLR.de Chart 10

Multispectral analysis essential when using line profiles of high complexity and various parameters IDL fitting tool combining advantages of single and multispectrum fit has been developed Several line models Interactive and automatic mode Additional information for quality assessment (parameter correlation matrix, information content, filecuts) H 2 O 2 band reanalyzed Speed-dependence of broadening parameter has to be considered Opaque and non-opaque lines fitted simultaneously Systematically larger broadening parameters than HITRAN N 2 O 3 band High SNR measurements Speed-dependence and line mixing have to be considered Concluding remarks > 13 th International HITRAN Conference > J. Loos New multispectrum fitting software used at DLR > June 24, 2014DLR.de Chart 11