2015
DOI: 10.1366/14-07834
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Autocorrelation Analysis Combined with a Wavelet Transform Method to Detect and Remove Cosmic Rays in a Single Raman Spectrum

Abstract: Cosmic rays (CRs) occasionally affect charge-coupled device (CCD) detectors, introducing large spikes with very narrow bandwidth in the spectrum. These CR features can distort the chemical information expressed by the spectra. Consequently, we propose here an algorithm to identify and remove significant spikes in a single Raman spectrum. An autocorrelation analysis is first carried out to accentuate the CRs feature as outliers. Subsequently, with an adequate selection of the threshold, a discrete wavelet trans… Show more

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Cited by 22 publications
(21 citation statements)
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“…combined a kernel PCA with noise estimation to detect spikes and then a best‐fit spectrum replacement to correct the Raman spectra. A different approach was proposed by Maury and co‐workers, who combined an autocorrelation analysis with a discrete wavelet transform filter to identify spikes and interpolate them by making use of a weighted‐average interpolation technique. Their algorithm is limited to spikes with a much narrower bandwidth than the Raman bands.…”
Section: Introductionmentioning
confidence: 99%
“…combined a kernel PCA with noise estimation to detect spikes and then a best‐fit spectrum replacement to correct the Raman spectra. A different approach was proposed by Maury and co‐workers, who combined an autocorrelation analysis with a discrete wavelet transform filter to identify spikes and interpolate them by making use of a weighted‐average interpolation technique. Their algorithm is limited to spikes with a much narrower bandwidth than the Raman bands.…”
Section: Introductionmentioning
confidence: 99%
“…However, some sharp peaks can resemble spikes and might be falsely interpreted as such (i.e., false alarms) in a variety of different despiking methods. 46,[66][67][68] Where a data set contains sharp peaks that repeatedly produce false alarms, the false alarms can, to some extent, be identified when they also occur in other spectra in the same position. This can be detected by examining the number of spike occurrences at every wavenumber and discounting the ''spikes'' if they occur with frequency greater than what would be expected for the detector used at its location.…”
Section: Cosmic Ray-induced Spike Removalmentioning
confidence: 99%
“…In the second category methods such as analyzing the full CCD image 10 , division of the spectrograph slit and image curvature correction 11 . Finally in the third category methods such as moving window filtering 12 , spike fitting , wavelet transforms 14,15,16 and median or polynomial filters 17,18 .…”
Section: Introductionmentioning
confidence: 99%