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Table of Contents > Section A > Section B > Section C > Section D > Section E > Section F >

User Guide to the Jb95 Spectral Fitting Program

G. Calibration, normalization and linearization procedures
Most spectroscopic data will need to be normalized and calibrated (linearized) prior to any detailed analysis. The calibration is usually based on a relative frequency reference and performed by simultaneously recording the marker fringes from, for instance, a Fabry-Perot cavity. A procedure is described to generate a normalized and linearized data file under these conditions. In this procedure, it is assumed that the signal file is named PmtF, that of the reference cavity marker file is MarkersF, and that of the laser power is PwdF.


1. Calibration
  • Select the MANIPULATION/CALNORMLINEAR dialog.
  • Run the peak-finding (PEAK FIND) procedure on the MarkersF file.
  • Display the MarkersF channel and depress the t key from the MAIN WINDOW to display the file positions found. The file positions are only shown in the MED and RAW data views.
  • Correct problems using P to erase or add marker positions.
2. Normalization
  • Toggle the display status off for the MarkersF channel and the display status on for thePwdF channel. Make sure PwdF is the active channel.
  • Shrink the view and position the cursor cross hair over a region representative of the average power across the scan.
  • Depress the h key to determine average voltage value. This factor is used as the normalizing factor.
  • Reposition the cursor in a region where laser was blocked to determine the voltage for power zero. Depress the l key to determine the average voltage value for zero power. Note that depressing the W key will zero both the h and l values. Display the PmtF channel to make sure it is zero when the laser is blocked. If not, use the OFFSET option in the MANIPULATION/CONVERSION dialog to manually offset this file.
  • Select the MANIPULATION/CALNORMLINEAR dialog. If the h and l values are not displayed in the REFER (h) and OFFSET (l) fields, enter 0 in either field and they should be updated.
  • Edit the filenames fields in the NORMALIZATION section to read
IN FLNM PmtF

OUT FLNM PmtFn

NORM FLNM PwdF
  • Normalization of the PmtF file will be done using the following formula:
PmtFn[n] = PmtFn * Vh / [PwdF[n] - Vl]. Depress the NORM button.
  • Note that the %CUT is defined on the power channel as a percentage of the voltage range between the h and l values. Regions of the spectrum where powers fall below this value will not be normalized and are set to zero.
  • Also, in some cases, you may want to smooth the power channel file prior to normalization. Use the FFT SMOOTH option in the MANIPULATION/CONVERSION dialog prior to normalization.
3. Linearization
  • Edit the filenames fields in the LINEARIZATION section to read,
IN FLNM PmtFn

OUT FLNM PmtFnl
  • Check that the value for PTS/FSR is the same as that for AVE PTS/FSR shown in the CALIBRATION section.
  • Check that the FINAL MARKER number is the same as the # MKS in the CALIBRATION section.
  • Check the FSR value.
  • Depress LINEARIZE.
  • Select the ANALYSIS OPTIONS dialog and enter PmtFnl in a channel filename. Check the DSP STAT box and set the page values and TYPE fields for each view.
< Section F Top Appendix A >

For technical information or questions, contact:
David F. Plusquellic
Phone: (301)-975-3896
Fax: (301)-975-2950
Email: david.plusquellic@nist.gov

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Online: April 2001   -   Updated: December 2002