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Original Articles

Inversion of spectroscopic data, application on CO2 radiation of flame combustion

, , &
Pages 219-240 | Received 24 Jun 2003, Accepted 14 Sep 2004, Published online: 31 Aug 2006

Figures & data

Figure 1. The observation of radiation intensity.

Figure 1. The observation of radiation intensity.

Figure 2. Radiative intensity for Gaussian distributions, and some subsets of wave numbers.

Figure 2. Radiative intensity for Gaussian distributions, and some subsets of wave numbers.

Figure 3. The first six right singular vectors and their images by the sensitivity matrix.

Figure 3. The first six right singular vectors and their images by the sensitivity matrix.

Figure 4. Evaluation of Nr(1% ) corresponding to adimensionalized parameters for four subsets of wave numbers.

Figure 4. Evaluation of Nr(1% ) corresponding to adimensionalized parameters for four subsets of wave numbers.

Figure 5. Inversion result of retrieving all discretization values of profiles.

Figure 5. Inversion result of retrieving all discretization values of profiles.

Figure 6. The four right singular vectors and their images by the sensitivity matrix.

Figure 6. The four right singular vectors and their images by the sensitivity matrix.

Figure 7. Evaluation of Nr(1% ) corresponding to the subparameterization Φ for four subsets of wave numbers.

Figure 7. Evaluation of Nr(1% ) corresponding to the subparameterization Φ for four subsets of wave numbers.

Table 1. Averaged values and averaged relative errors for different noise levels.

Figure 8. Temperature and concentration profiles for real case inversion.

Figure 8. Temperature and concentration profiles for real case inversion.

Figure 9. Inversion CO2 spectrum of the exhaust of a motor.

Figure 9. Inversion CO2 spectrum of the exhaust of a motor.

Figure 10. Convexity over the segment between (t0,c0) and (0.3,0) of radiative intensities for all wave numbers σ ∈ Σ.

Figure 10. Convexity over the segment between (t0,c0) and (0.3,0) of radiative intensities for all wave numbers σ ∈ Σ.

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