cavity ring down spectroscopy 14 February 2012 CE 540

history: first work in early 1980’s to determine mirror reflectivities in laser applications operated using red laser line 632nm (e.g. laser gyroscopes) mirrors were getting so good (>99.99% efficiency) that measuring them was hard first work Herbelin et al (1980)App. Op. 19, 144 Anderson et al 1984, Appl. Optics 23, 1238  pulsed dye laser (many wavelengths) development of high quality dielectric dichroic mirrors

CRD Optics

CSU thesis

I(t) = I o exp(-t/  o ) [assuming index of refraction n = 1], simple exponential decrease I(t) / I o = exp(-t/  o ) for cavity ring down time of t =  o  time for intensity to drop by 1/e for an empty cavity, the decay constant is dependent on the loss mechanisms within the cavity = mainly mirror reflectivity. If L is the cavity length and c the speed of light, then R = = exp{-L/(c  o )} where (c  o )/L # cell reflections to 1/e intensity  ln (R) = L/(c  o )   o = L/(c ln(R)) but ln(R) = 1 – R for R near 1   o = L / {c(1 – R)} [sec] cavity intensity as a function of time: L = 50cm, decay time  o = 30µs  R = and # round trips ~10,000  total path length 10km

now add a molecular absorption:  = L / {c(1 – R +  L)} [sec] { from I(t) / I o = exp(-t/  o –  ct) and ct = L, total cavity length at time t } where  is the absorption coefficient [/cm] and goes like concentration x cross section Then the relationship between empty cavity decay time (  o ) and the decay time with an absorber present (  ) is: 1/  o + c  since c  is 1/time added for the absorber The  are a function of wavelength and at each wavelength are fitted with an exponential decay curve to get the decay time. Knowing  o allows calculation of  and from that the concentrations can be determined over a full spectral line using Beer’s law using differential spectroscopy.

O’Keefe et al publications/ acs.pdf 750 ppm loss  1 – 750 x = = % best we can do with the NASA system upstairs is about 0.015%, about 2x worse

some specs: mirror reflectivity > % in near UV/vis are available fractional absorbance detectable < /pulse using mirrors at uncertainty in  o of 1% example: L = 50 cm  decay time ~ 30µsec for reflectivity % gives ~ 10,000 round trips during the decay time  a detectable light pulse every 3 nsec = 2 x L/c with laser pulse length < shorter than cavity round trip achievable absorbance example: absorbance. NO 2 example with L = 900m = cm (as in HW problem) I/I o = = exp(-L (2.5 x )N)  N = 4.5x10 6 molecules/cm 3 = 0.2 pptv

Advantages of CRDS: everything is fractional, so not affected by fluctuations in light source intensity – ring down time does not depend on intensity very sensitive due to long path length (km) due to multiple mirror reflections spectral range is usually good since dichroic laser mirrors are somewhat broad Disadvantages: laser is nearly monochromatic  must build up the spectrum need particular laser wavelengths for different molecules high reflectance mirrors (>>99.99% reflectivity) expensive absorbances must be < a few % or don’t get enough bounces source bandwidth must be < absorption bandwidth frequencies within the laser BW must be reflected equally by the mirrors excited state lifetime must be < laser roundtrip time in the cavity – so once a photon is absorbed during a particular laser pass, the excited specie has time to relax before the next laser pass laser scan time limits the time resolution of spectra dirt in system  decreased R. I guess this gets calibrated out when you run the cell w/o the molecule you want to measure in the mixture. But you are sucking outside air into the cell all the time and it is dirty