1/24 Optical Thermometry Haiqing Guo Dept. of Fire Protection Engineering Lab Methods Day June 25, 2014.

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1/24 Optical Thermometry Haiqing Guo Dept. of Fire Protection Engineering Lab Methods Day June 25, 2014

2/24 Introduction Optical thermometry, i.e. soot pyrometry, provides soot temperature and soot concentration information in flames. Soot radiance in flames was detected and converted to soot temperature (K) and soot volume fraction (ppm). This technique is nonintrusive.

3/24 For hot regions in the visible or near-IR: Choose wavelength Soot Radiance The spectral radiance of hot soot is: Blackbody spectral radiance Speed of light Planck’s constant Boltzmann’s constant Temperature Emissivity Wavelength BλchkTελBλchkTελ Measure radiance (e.g., with filtered digital camera) Determine emissivity wikipedia.org

4/24 Bandpass Filters Choose two or more bandpass filters, e.g., at 450, 650, and 900 nm. Bandwidth choice involves a tradeoff between error and signal strength. A FWHM of 10 nm is most common. Avoid chemiluminescence spectra (e.g., Swan Bands) and should be far separated. newport.com wikipedia.org

5/24 Soot Emissivity Determine emissivity Assume: Refractive index absorption function Soot volume fraction Absorption coefficient Extinction coefficient E(m) f s K abs K ext Notes : The variation of E(m) with soot morphology, soot age, and other conditions is not fully understood. Soot volume fraction f s is unknown. Rayleigh scattering can be assumed because soot primary particles (d p  30 nm) are smaller than the Rayleigh limit.

6/24 Camera Signal Measure soot radiance CCD/CMOS cameras are attractive owing to high bit depth (e.g, 14), higher pixel counts (12M), larger sensor arrays (36 x 24 mm), and decreased noise. Irradiance incident on the CMOS sensor I: aConstant that accounts for pixel size, fill factor, and sensitivity GSGrayscale divided by shutter time  Constant that accounts for magnification and lens light losses  Bandpass filter transmissivity

7/24 Camera Calibration Constant a obtained from blackbody furnace calibration. –Emissivity of ε = 0.99 ± 0.01 –Uniform and stable temperature T range: 900 − 1200 ºC T increment: 25 ºC T accuracy: ± 0.1 ºC

8/24 Line-of-Sight Radiance x y Bandpass Filter x (x,y)dy The exponent term describes the extinction effect from soot. For optically thin cases, it is negligible. Flame cross section

9/24 GS to T Conversion Tomography can convert the line-of-sight integrated irradiance I(x) into the local irradiance I(x,y). For optically thin conditions: From measured grayscale, blackbody calibration, and tomography From filter manufacturer High uncertaintyRequired Objective

10/24 Ratio Pyrometry With multiple bandpass filters, ratio pyrometry allows f s and E(m) to be cancelled: and where C = a τ Δλ / λ 6 is a constant for each filter and camera that does not vary with T or E(m).

11/24 f s from Emissions The pyrometry determined temperature can be used to obtain the soot volume fraction for each filter. A soot refractive index of m = 1.57 – 0.56 i is commonly assumed, which yields E(m) = Any uncertainty in T is amplified in determining f s.

12/24 Camera Tradeoffs Digital cameras require considering: –Response linearity (gamma correction must be avoided) –Parallel light collection (small aperture) –Sufficient depth-of-field (small aperture) –High spatial resolution (big sensor, small object distance) –High temporal resolution (fast shutter) –High signal resolution (high color bit-depth) –Ideal exposures should have high GS but not be saturated in any color plane. This presents tradeoffs with aperture, shutter, and ISO.

13/24 Deconvolution 3D tomographic reconstruction requires multiple imaging at different locations. For axisymmetric flames, tomography from I(x) to I(r) can be simplified and requires only one image. Commonly used deconvolution algorithms: –Abel transform –Onion peeling –Filtered back projection

14/24 Abel Transform Based on an exact solution Requires discretization Line-of-sight integration of the flame property f(r) is: Substituting y with x and r following r 2 = x 2 + y 2 yields: Analytical inverse of the above equation yields: Sensitive to noise Singularity at x = r

15/24 Abel Transform Alternatively, a discretized form is simpler and more commonly used. Lower integration limit region, solved with a open type numeric integration (e.g. Steffensen’s formula). Solved with a regular closed type integration scheme (e.g. Simpson’s rule).

16/24 Onion Peeling Based on numerical approximation. The domain is divided into a series of concentric rings. Within each ring, the value of the spatial function f(r) is assumed to be constant. For the i-th cord and the j-th ring: s ij is a geometric matrix Deconvolve Form:

17/24 Deconvolution Deconvolution results from prescribed projection data. Spatial resolution is 0.05 mm/pixel. Sufficient spatial resolution is required for enough accuracy. Due to the differentiation, deconvolution is very sensitive to noise. Data smoothing can help:  Low-pass filter  Gaussian filter  Savitzky-Golay filter

18/24 Laminar Jet Diffusion Flame A Santoro coflow burner was used. The flame was steady and axisymmetric. Fuel tube: 11.1 mm ID Air tube: 101 mm ID Air Fuel Glass beads

19/24 C 2 H 4 Flame Fuel: ethylene Oxidizer: coflowing air. Flame height: 88 mm  Steady  Optically thin  Axisymmetric

20/24 Soot Temperatures Low soot concentration

21/24 T Contours T range: K. Spatial resolution: 23 µm Longest shutter time: 125 ms Precision: ± 0.1 K Uncertainty: ± 50 K (95% confidence)

22/24 Soot Emission Concentrations

23/24 Results f s results EmissionExtinction f s (ppm) Res. (µm)2334 t (ms) Precision (ppm) ± 4×10 -4 ± 6×10 -4 Uncertainty± 30%± 10%

24/24 Limitations Only applicable for sooting flame. Needs to be optically thin (otherwise complicated corrections are required). Needs to be steady. Needs to be axisymmetric. For detailed information, please refer to “H. Guo, J.A. Castillo, P.B. Sunderland, Digital Camera Measurements of Soot Temperature and Soot Volume Fraction in Axisymmetric Flames, Applied Optics 52 (2013) ”