Noise Performance Optimization of a Fast Wavelength Calibration Algorithm for OSAs

A new fast correlation algorithm for calibrating the wavelength of Optical Spectrum Analyzers (OSAs) was introduced in [1]. The minima of acetylene gas spectra were measured and correlated with saved theoretical data [2]. So it is possible to find the correct wavelength calibration data using a noisy reference spectrum. First tests showed good algorithmic performance for gas line spectra with high noise. In this article extensive performance tests were made to validate the noise resistance of this algorithm. The filter and correlation parameters of the algorithm were optimized for improved noise performance. With these parameters the performance of this wavelength calibration was simulated to predict the resulting wavelength error in real OSA systems. Long term simulations were made to evaluate the performance of the algorithm over the lifetime of a real OSA.

Authors:



References:
[1] Fuhrmann, T. "Fast Wavelength Calibration Algorithm for Optical
Spectrum Analyzers". International Journal of Information and
Communication Engineering 6:1 2010, pp. 1-6.
[2] S. L. Gilbert, W. C. Swann "Acetylene 12C2H2 Absorption Reference
for 1510 nm to 1540 nm Wavelength Calibration - SRM 2517a". NIST
Special Publication 260-133, 2001.
[3] ITU-T "Spectral Grids for WDM applications: DWDM frequency grid".
ITU-T, G694.1, 06/2002.
[4] K. Benzel, A. Conzelmann, T. Fuhrmann, E. Löcklin "Device for
simultaneous analysis of multiple optical channels". European Patent EP
1106979, 1999.
[5] JDSU "ONT Platforms, Optical Spectrum Analyzer Modules". JDSU
Product Overview.
[6] A. Savitzky, M. J. E. Golay "Smoothing and Differentiation of Data
by Simplified Least Square Procedure". Analytical Chemistry, Vol. 36,
No. 8, pp. 1627-1639, 1964.