Pressure Broadening and Spectral Overlap in the Millimeter Wave Spectrum of Ozone International Symposium on Molecular Spectroscopy 65 th Meeting — June.

Slides:



Advertisements
Similar presentations
Lecture 6 ATOMIC SPECTROSCOPY
Advertisements

The Amazing Spectral Line Begin. Table of Contents A light review Introduction to spectral lines What spectral lines can tell us.
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.
Yu. I. BARANOV and W. J. LAFFERTY Optical Technology Division Optical Technology Division National Institute of Standards and Technology, Gaithersburg,
Sub-Doppler Resolution Spectroscopy of the fundamental band of HCl with an Optical Frequency Comb ○ K. Iwakuni, M. Abe, and H. Sasada Department of Physics,
Nuclear Magnetic Resonance (NMR)
Analysis of an 18 O and D enhanced lab water spectrum using variational calculations of HD 18 O and D 2 18 O spectra Michael J Down - University College.
17.1 Mass Spectrometry Learning Objectives:
ACE Linelist Needs for the Atmospheric Chemistry Experiment Chris Boone and Peter Bernath Univ. of Waterloo, Waterloo, Ontario, Canada HITRAN 2006 Conference.
Update on the Leicester lab studies (WP2.2 cavity ringdown spectroscopy) Stephen Ball & Simon Neil (Leicester University) CAVIAR science meeting, NPL,
FASSST Cavity Ringdown Spectroscopy of Atmospherically Broadened Lineshapes in the Millimeter Spectral Region Corey Casto Frank C. De Lucia The Ohio State.
Case Western Reserve University
Microwave Spectroscopy I
(8) Absorption – Visible and IR Physics of the Atmosphere II Atmo II 193a.
Hadronic Resonances in Heavy-Ion Collisions at ALICE A.G. Knospe for the ALICE Collaboration The University of Texas at Austin 25 July 2013.
WH04 NUMERICAL AND EXPERIMENTAL ASPECTS OF DATA ACQUISITION AND PROCESSING IN APPLICATION TO TEMPERATURE RESOLVED 3-D SUB-MILLIMETER SPECTROSCOPY FOR ASTROPHYSICS.
LINE PARAMETERS OF WATER VAPOR IN THE NEAR- AND MID-INFRARED REGIONS DETERMINED USING TUNEABLE LASER SPECTROSCOPY Nofal IBRAHIM, Pascale CHELIN, Johannes.
Physical Chemistry 2 nd Edition Thomas Engel, Philip Reid Chapter 28 Nuclear Magnetic Resonance Spectroscopy.
IR/THz Double Resonance Spectroscopy in the Pressure Broadened Regime: A Path Towards Atmospheric Gas Sensing Sree H. Srikantaiah Dane J. Phillips Frank.
Explore. Discover. Understand. AIR-BROADENED LINE WIDTHS AND SHIFTS IN THE ν 3 BAND OF 16 O 3 AT TEMPERATURES BETWEEN 160 AND 300 K M. A. H. SMITH and.
Infrared Spectroscopy
Active control of decoherence of excited resonance states by means of laser pulses A. Garc í a-Vela Instituto de Física Fundamental, Consejo Superior de.
Columbus, 18 June 2013 International Symposium on Molecular Spectroscopy 68 th Meeting - June 17-21, 2013, Ohio State University Determination of the Boltzmann.
65th OSU International Symposium on Molecular Spectroscopy June 21-25, 2010 José Luis Doménech Instituto de Estructura de la Materia 1 TIME-RESOLVED ROTATIONAL.
20 June st International Symposium on Molecular SpectroscopyPetkie – TG03-p1 The Millimeter and Submillimeter-wave Spectrum of the , 6 1.
Broadband Mid-infrared Comb-Resolved Fourier Transform Spectroscopy Kevin F. Lee A. Mills, C. Mohr, Jie Jiang, Martin E. Fermann P. Masłowski.
Substitute Lecturer: Jason Readle Thurs, Sept 17th, 2009
Yu. I. BARANOV, W. J. LAFFERTY, and G. T. Fraser Optical Technology Division Optical Technology Division National Institute of Standards and Technology,
Haifeng Huang and Kevin K. Lehmann
Precision Measurement of CO 2 Hotband Transition at 4.3  m Using a Hot Cell PEI-LING LUO, JYUN-YU TIAN, HSHAN-CHEN CHEN, Institute of Photonics Technologies,
Weeding the Spectra [Preliminary Results with a new ‘Experimental’ Approach] Frank C. De Lucia Department of Physics Ohio State University USA May 5, 2008,
Figure 8.3 gives the basic layout of a continuous wave NMR spectrometer. These intruments were the original type of instrument and have largely.
IMPACT OF ATMOSPHERIC CLUTTER ON DOPPLER-LIMITED GAS SENSORS IN THE SUBMILLIMETER/TERAHERTZ IVAN R. MEDVEDEV, CHRISTOPHER F. NEESE, FRANK C. DE LUCIA,
3-D SUBMILLIMETER SPECTROSCOPY FOR ASTROPHYSICS AND SPECTRAL ASSIGNMENT SARA FORTMAN, CHRISTOPHER NEESE, IVAN R. MEDVEDEV, FRANK C. DE LUCIA, Department.
3-D SUBMILLIMETER SPECTROSCOPY FOR ASTROPHYSICS AND SPECTRAL ASSIGNMENT SARAH M. FORTMAN, IVAN R. MEDVEDEV, FRANK C. DE LUCIA, Department of Physics, The.
Experimental Measurements of Collisional Cross Sections and Rates at Astrophysical and Quantum Collisional Temperatures Frank C. De Lucia Department of.
Ab Initio and Experimental Studies of the E Internal Rotor State of He-CH 3 F Kelly J. Higgins, Zhenhong Yu, and William Klemperer, Department of Chemistry.
Gas cell observations of methanol from 0.6 to 1.9 THz using the Herschel space observatory HIFI instrument Ronan D. Higgins, NUI Maynooth, Co. Kildare,
FE06 : Collisional Cross- Sections at Low Temperatures David L. Graff T. J. Ronningen F. C. De Lucia The Ohio State University.
I. Ventrillard-Courtillot, Th. Desbois, T. Foldes and D. Romanini
The Analysis of Astrophysical ‘Weeds’ Using 3-D Submillimeter Spectroscopy SARAH M. FORTMAN, JAMES P. MCMILLAN, CHRISTOPHER F. NEESE, and FRANK C. DE LUCIA.
The Complete, Temperature Resolved Spectrum Of Methyl Formate Between 214 and 265 GHz JAMES P. MCMILLAN, SARAH M. FORTMAN, CHRISTOPHER F. NEESE, and FRANK.
Cavity Based Medium Resolution Spectroscopy Satyakumar Nagarajan, Frank C. De Lucia, Christopher Neese The 70 th International Symposium on Molecular Spectroscopy.
Line Mixing in Atmospheric Ozone Corey Casto and Frank C. De Lucia The Ohio State University International Symposium on Molecular Spectroscopy 66 th Meeting.
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.
Shui-Ming Hu (胡水明) University of Science & Technology of China (USTC) Hefei, China June 17, 2014, ISMS-UIUC Doppler broadening thermometry based on cavity.
1 Dual Etalon Frequency Comb Spectrometer David W. Chandler and Kevin E. Strecker Sandia National Laboratories – Biological and Energy Sciences Division.
OBSERVATION AND ANALYSIS OF THE A 1 -A 2 SPLITTING OF CH 3 D M. ABE*, H. Sera and H. SASADA Department of Physics, Faculty of Science and Technology, Keio.
Measurement and Analysis of Atmospherically Broadened Linewidths and Lineshapes in the Millimeter Spectral Region Corey Casto Frank C. De Lucia The Ohio.
1 61 st International Symposium on Molecular Spectroscopy, Talk RD10, 22 June 2006, The Ohio State University, Columbus, OH Approved for Public Release;
Frequency-comb referenced spectroscopy of v 4 =1 and v 5 =1 hot bands in the 1. 5 µm spectrum of C 2 H 2 Trevor Sears Greg Hall Talk WF08, ISMS 2015 Matt.
High-resolution mid-infrared spectroscopy of deuterated water clusters using a quantum cascade laser- based cavity ringdown spectrometer Jacob T. Stewart.
FAST SCAN SUBMILLIMETER SPECTROSCOPIC TECHNIQUE (FASSST). IVAN R. MEDVEDEV, BRENDA P. WINNEWISSER, MANFRED WINNEWISSER, FRANK C. DE LUCIA, DOUGLAS T. PETKIE,
An Experimental Approach to the Prediction of Complete Millimeter and Submillimeter Spectra at Astrophysical Temperatures Ivan Medvedev and Frank C. De.
Fast Sweeping Double Resonance Microwave - (sub)Millimeter Spectrometer Based on Chirped Pulse Technology Brian Hays 1, Susanna Widicus Weaver 1, Steve.
SESAPS Terahertz Rotational Spectrum of the v5/2v9 Dyad of Nitric Acid * Paul Helminger, a Douglas T. Petkie, b Ivan Medvedev, b and Frank C. De.
TJ02 3-D SUBMILLIMETER SPECTROSCOPY OF ASTRONOMICAL `WEEDS‘ - EXPERIMENTAL AND THEORETICAL ASPECTS OF DATA PROCESSING AND CATALOGING –> TJ03 Ivan R. Medvedev,
Proposed Laboratory Simulation of Galactic Positron In-Flight Annihilation in Atomic Hydrogen Benjamin Brown, Marquette University, Milwaukee, WI, USA.
MOLECULAR SPECTROSCOPY
Concentration Dependence of Line Shapes in the Band of Acetylene Matthew Cich, Damien Forthomme, Greg Hall, Chris McRaven, Trevor Sears, Sylvestre.
CHAPTER 11 Alkenes; Infrared Spectroscopy and Mass Spectroscopy.
Lineshape analysis of CH3F-(ortho-H2)n absorption spectra in 3000 cm-1 region in solid para-H2 Yuki Miyamoto Graduate School of Natural Science and Technology,
Photoacoustic Spectroscopy of the Oxygen A-band
The Classical Damping Constant
The Near-IR Spectrum of CH3D
Z. Reed,* O. Polyansky,† J. Hodges*
University of Arizona, Dept. of Physics
An Analysis of the Rotation Spectrum of Acetonitrile (CH3CN) in Excited Vibrational States Christopher F. Neese, James McMillian, Sarah Fortman, Frank.
Atomic Absorption Spectroscopy
ANH T. LE, GREGORY HALL, TREVOR SEARSa Department of Chemistry
Presentation transcript:

Pressure Broadening and Spectral Overlap in the Millimeter Wave Spectrum of Ozone International Symposium on Molecular Spectroscopy 65 th Meeting — June 21–25, /22/20101 Corey Casto and Frank C. De Lucia The Ohio State University TE02

Introduction 6/22/20102  Millimeter region:  GHz  Atmospherically broadened lines  Van Vleck-Weisskopf line profile  P = 100 – 760 torr  FWHM = 0.5 – 4.6 GHz  Significant overlap  Isolated lines? TE02

Experiment 6/22/20103  Cavity characteristics  3 second scan  ~6000 resonances in the 172 – 262 GHz range  FSR = 14.5 MHz  Q ~ 7  10 6  Ringdown   = 1/c    ~ 5  s Quasi-Optical Isolator InSb Detector DAQ Pulse Generator BWO HV Power 10.3 m TE02

Low Pressure 6/22/20104  Good agreement between model and experiment  Intensities and linewidths are consistent  Residual is not significantly greater at the peaks  Lines are isolated and less prone to mixing effects TE02

High Pressure 6/22/20105  Similar noise to low pressure  Discrepancies near line peaks  Causes? TE02

Causes of error near line peaks 6/22/20106  Intensity  Frequency  Experiment  Linewidth  Line Mixing TE02

Residuals at various pressures 6/22/20107  Ozone concentration is constant ~ 150 ppm  Narrow features are consistent  Broad features increase by an order of magnitude TE02

Causes of error near line peaks 6/22/20108  Intensity  Frequency  Experiment  Linewidth  Line Mixing TE02

Global linewidth adjustment fit 6/22/20109   a (T 0 /T) n a   a Air-broadened linewidth in MHz/torr  n a Air-broadened coefficient of temperature dependence  Overlap makes measurement of linewidths difficult  Global fit prevents pressure dependent parameters TE02

Global Fit Linewidth Adjustments 6/22/  Disagreement is <5% for most lines  Many lines are known to within 2-5%  How does this affect residuals? TE02

Residuals with global fit parameters 6/22/  Low pressure residuals don’t increase  High pressure residuals improve near line centers  Linewidth error is not sufficient to explain residual  Published parameters accurately describe our data TE02

Causes of error near line peaks 6/22/  Intensity  Frequency  Experiment  Linewidth  Line Mixing TE02

Line mixing characteristics 6/22/  Lines not isolated  Inelastic collisions allow coupling of lines  First order effects can be expressed in a modified line profile  Wing skewing  Small center shift  Linear in pressure Y = Y 0 P TE02

Line mixing 6/22/  Residuals largest at the wings of strong lines  Conditions for line mixing  Lower state energy gap is less than thermal energy  Line separation is less than width E 1 - E 2 < kT <  1,2 E 1 - E 2 < kT <  1,2 TE02

Future Work 6/22/  Model line mixing  Which lines mix?  What are reasonable parameters?  Explore other dense spectra  Formaldehyde (H 2 CO)  Nitric acid (HNO 3 )  Nitrogen dioxide (NO 2 )  Acetonitrile (CH 3 CN)  Methanol (CH 3 OH) TE02