Spectral Profile
Optical emission and absorption spectra exhibit finite widths rather than infinitely sharp peaks at single wavelengths. This spectral expansion, known as line broadening, arises from physical processes that perturb the energy states of the absorbing or emitting atoms. The resulting peak profile contains information about both the concentration of the target gas and the local conditions within the sample cell.
Thermal Effect
Atomic motion relative to the detector causes frequency shifts through the Doppler effect, which shapes the core of the observed peak. When temperatures rise, line broadening increases as atoms move at higher velocities. This Gaussian distribution is modeled to extract the temperature of the medium under investigation.
Pressure Influence
Collisions between molecules during the transition lifetime shorten the coherence time of the emission or absorption process. This interaction leads to Lorentz-shaped line broadening, which becomes dominant in high-pressure environments like industrial chimneys. Measuring this Lorentzian component allows the analyzer to estimate the pressure of the gas matrix.
Instrumental Contribution
Finite resolution of the spectrometer optics spreads the measured energy across adjacent detector pixels, masking the true physical profile of the peak. This artificial line broadening is governed by the slit width and the grating spacing of the sensor. Engineers must calibrate the instrument with a reference laser of known narrow linewidth to separate the hardware response from the actual gas absorption profile.
Additionally, temperature-induced expansion of the optical bench can shift the alignment, making regular calibration check-ups necessary to maintain the measurement precision of the system over its service life.