Cavity RingDown Absorption Spectroscopy - PowerPoint PPT Presentation

1 / 24
About This Presentation
Title:

Cavity RingDown Absorption Spectroscopy

Description:

Light intensity decays as a function of time with pulses spaced by ... c speed of light. I ... of cavity and absorbing species, not light amplitude ... – PowerPoint PPT presentation

Number of Views:1013
Avg rating:3.0/5.0
Slides: 25
Provided by: jerryl6
Category:

less

Transcript and Presenter's Notes

Title: Cavity RingDown Absorption Spectroscopy


1
Cavity Ring-Down Absorption Spectroscopy
  • Trisha Blood
  • December 4, 2007

2
Introduction
  • Direct absorption technique governed by Beers
    Law
  • A ? c l
  • Rate of absorption measured as opposed to
    magnitude
  • Sample placed within optical cavity between two
    reflective mirrors
  • Laser pulse coupled into cavity with small
    fraction leaking out upon reflection
  • Decay time dependent upon sample absorbance

Hollas, J.M. Modern Spectroscopy, 4th ed. John
Wiley Sons, Ltd 2004
3
A Brief History
  • 1980 Herbelin proposed use of optical cavity
    for measuring reflectance of mirror
    coatings (CW light beam)
  • 1988 Applications to molecular absorption
    measurements described by OKeefe and
    Deacon (pulsed laser)
  • Sensitivity demonstrated by measuring absorption
    spectrum of weak forbidden b 1?g X
    3?g transition in gaseous oxygen

OKeefe, A. Deacon, D.A.G. Rev. Sci. Instrum.
1988, 59, 2544-2551
4
Principles of CRDS
  • Requirements
  • Light pulse with coherence length shorter than
    mirror spacing
  • Light traverses cavity with small fraction
    exiting upon each pass
  • Light intensity decays as a function of time with
    pulses spaced by round trip time (2L/c)

T ? transmission coefficient L ? cavity mirror
spacing t ? time c ? speed of light
  • I(t) Ioe (-Tt2L/c)

Scherer, J.J. Paul, J.B. Collier, C.P.
Saykally, R.J. J. Chem. Phys. 1995, 102, 5190-5199
5
Spectral Features
  • Ringdown transient, ?, single exponentially
    decaying function of time
  • Allows for direct measurement of total losses
    experienced
  • Dependent only on properties of cavity and
    absorbing species, not light amplitude
  • Absorption spectrum obtained from plot of cavity
    loss (1/c?) versus frequency (?)

?o L / c? lnR?
6
Mirror Reflectivity
  • Higher sensitivity attained with greater mirror
    reflectivity
  • Typical values R 0.99 or better
  • Contributions of broad-band scattering /
    absorption smaller than reflection losses
  • ? ?ln (Reff)? ? 1-
    Reff

Scherer, J.J. Paul, J.B. Collier, C.P.
Saykally, R.J. J. Chem. Phys. 1995, 102,
5190-5199
7
Experimental Set-Up
Berden, G. Peeters, R. Meijer, G. Int. Rev.
Phys. Chem. 2000, 19, 565-607
8
Experimental Design
  • Pulsed dye laser used in visible spectrum
  • Pulse duration of 5-15 ns
  • Moderate pulse energies needed (?1 mJ)
  • Ring-down cavity
  • Two identical plano-concave mirrors
  • Radius of curvature between 25 cm and 1m
  • Separation distance d so as to create
    non-confocal cavity
  • Time-dependent detection
  • Photomultiplier tube (PMT)
  • Analogue-to-digital converter
  • Computer

9
http//www.arp.harvard.edu/atmobs/sciobj/instrumen
t/cr.html
10
Advantages of CRDS
  • High sensitivity due to multipass nature of
    detection cell
  • Effective absorption pathway very long while
    sample volume small
  • Absorption independent of pulse-to-pulse
    fluctuations of laser
  • Absorption measured on absolute time scale
  • Fluorophore unnecessary

11
Applications of CRDS
  • Studies performed on molecules in various
    environments
  • Cells
  • Supersonic jets
  • Transient molecules generated in discharges and
    flames
  • Frequency-dependent absorption strengths given
  • Number density, cross-section and temperature
    determined
  • No intrinsic limitation to spectral region
  • Range from ultraviolet to infrared radiation

http//lot.astro.utoronto.ca/spectrum.html
12
Integrated absorption intensity and Einstein
coefficients for the O2 a 1?g X 3?g (0,0)
transition A comparison of cavity ringdown and
high resolution Fourier transform spectroscopy
with a long-path absorption cell
  • Stuart M. Newman, Ian C. Lane, and Andrew J.
    Orr-Ewing
  • David A. Newnham and John Ballard

13
Ozone photolysis
  • Monitor emission of products formed
  • O3 h? ? O2 (a 1 ? g , b 1?g ) O (1D)
  • O2 electronic configuration
  • ...(2p?g)2(2ppu)4(2ppg)2
  • Hartley system absorption lt 310 nm
  • O2 (a 1 ? g ) and O (1D) formed
  • Short-wavelength side of Hartley system
  • O2 (b 1?g ) directly produced

14
Review of Selection Rules
  • O2 a-X and b-X bands weak
  • Violate electric dipole selection rules
  • ?S 0 D L 0, ? 1
  • g ? g ? ? not allowed
  • Transition induced by magnetic-dipole and
    electric-quadrupole interactions

15
Ozone Concentration
  • Einstein A-coefficient necessary for inference of
    ozone concentration
  • Spontaneous emission from a 1?g X 3?g
  • O2 (a 1?g ) state metastable with lifetime to
    ground state ? 64-113 min.
  • Einstein B-coefficient determined from integrated
    absorption intensity, Sint,B

gl / gr ratio of degeneracies of lower and
upper states (3/2)
nr index of refraction (1.00027)
16
Experimental Apparatus
  • NdYAG laser supplying 450 mJ pulses of 355 nm
    radiation
  • Glass vacuum cell (1.5 m long) bounded by
    ultrahigh reflectivity mirrors
  • Near-IR sensitive InGaAs photodiode
  • Exponential signal decay converted to linear
    function
  • Ringdown rate coefficient, k, obtained by linear
    least-squares analysis

17
Cavity Ring-down Spectra
  • Ringdown rate coefficient, ko obtained in
    absence of absorbing species (baseline region of
    spectrum)
  • Ringdown time (RDT), ?o time required for light
    intensity to fall to 1/e of initial value
  • RDT 7 ?s for empty cavity with R 0.9993
  • Ringdown time reduced with O2 absorption
  • napierian absorption coefficient

Io initial light intensity
18
Cavity Ring-down Spectra
  • Complications in determination of ? when laser
    bandwidth comparable to widths of resolved O2 a-X
    (0,0) rotational features
  • Laser bandwidth 0.25cm-1
  • Pressure- and Doppler-broadened linewidth 0.098
    cm-1

19
Absorption Spectra
  • a 1?g X 3?g (0,0)

20
Absorption Spectra
  • Integrated absorption intensity a function of
    summation of absorption coefficients of all lines
    in (0,0) band
  • Determined by integrating the area under each
    spectrum over the complete wavenumber range of
    the band
  • Value converted to Einstein B- and A-coefficients

21
Results
22
Summary
  • Direct absorption technique following Beers Law
  • Rate of absorption measured rather than magnitude
  • Large effective path length due to highly
    reflective mirrors allows for detection of weak
    absorptions
  • Transitions of low probability or molecules
    present in very low concentrations

23
References
  • Newman, S.M. Lane, I.C. Orr-Ewing, A.J.
    Newnham, D.A. Ballard, J.
  • J. Chem. Phys. 1999, 110, 10749-10757
  • OKeefe, A. Deacon, D.A.G. Rev. Sci. Instrum.
    1988, 59, 2544-2551
  • Scherer, J.J. Paul, J.B. Collier, C.P.
    Saykally, R.J. J. Chem. Phys. 1995, 102,
    5190-5199
  • Berden, G. Peeters, R. Meijer, G. Int. Rev.
    Phys. Chem. 2000, 19, 565-607
  • Hollas, J.M. Modern Spectroscopy, 4th ed. John
    Wiley Sons, Ltd 2004

24
Exam Question
  • What makes CRDS more sensitive than other direct
    absorption techniques?
  • See Slide 10
Write a Comment
User Comments (0)
About PowerShow.com