STANDARDIZING AND CALIBRATING A SPECTROMETRIC INSTRUMENT

    公开(公告)号:CA2087360C

    公开(公告)日:2005-04-12

    申请号:CA2087360

    申请日:1993-01-15

    Abstract: A spectrometric instrument which exhibits an intrinsic profile for a sharp spectral line produces profile data for narrow spectral lines. The spectral lines are effected with a high finesse etalon of gold coated polymer. A transformation filter is computed for transforming the profile data to a gaussian profile. A wavelength calibration is combined with the filter to effect a correction matrix which is applied to sample data to generate calibrated standardized data. Iteratively a correction matrix is applied to calibration data to generate standardized calibration data which is utilized for the wavelength calibration. Calibration is effected with an optical standard, an interference etalon and a fringe formula. Etalon effective thickness is first estimated and then precisely determined so that fringe peaks calibrate wavelength.

    PHOTODETECTOR AMPLITUDE LINEARITY
    12.
    发明专利

    公开(公告)号:CA2087821C

    公开(公告)日:2002-11-26

    申请号:CA2087821

    申请日:1993-01-21

    Abstract: To calibrate a photodetector, a rotating disk with a slot is disposed in a light beam with decreasing speed from a defined maximum rotational speed to a defined minimum speed, while magnitudes and times of signals are read out and stored. Vernier pairs of signals occur in adjacent readout intervals, and non- vernier signals exclude the verniers. Readout times for verniers are used to estimate a preliminary function of rotations versus time. From the function are estimated an occurrence time for each pair and period of disk rotation at the time. Vernier fraction is the ratio of one signal in the pair to the sum of the pair. A time offset is the product of vernier fraction, slot fraction of the disk and the estimated period. Occurrence times corrected with the time offset are utilized to fit a corrected function of disk rotations versus time. Points of time for the non-vernier signals are determined from the corrected function, each point corresponding to disk rotations to a corresponding non-vernier signal. These points of time are employed with corresponding signals for linearly calibrating the photodetector.

    14.
    发明专利
    未知

    公开(公告)号:DE69309504T2

    公开(公告)日:1997-11-06

    申请号:DE69309504

    申请日:1993-01-07

    Abstract: To calibrate a photodetector, a rotating disk with a slot is disposed in a light beam with decreasing speed from a defined maximum rotational speed to a defined minimum speed, while magnitudes and times of signals are read out and stored. Vernier pairs of signals occur in adjacent readout intervals, and non-vernier signals exclude the verniers. Readout times for verniers are used to estimate a preliminary function of rotations versus time. From the function are estimated an occurrence time for each pair and period of disk rotation at the time. Vernier fraction is the ratio of one signal in the pair to the sum of the pair. A time offset is the product of vernier fraction, slot fraction of the disk and the estimated period. Occurrence times corrected with the time offset are utilized to fit a corrected function of disk rotations versus time. Points of time for the non-vernier signals are determined from the corrected function, each point corresponding to disk rotations to a corresponding non-vernier signal. These points of time are employed with corresponding signals for linearly calibrating the photodetector.

    15.
    发明专利
    未知

    公开(公告)号:DE69309504D1

    公开(公告)日:1997-05-15

    申请号:DE69309504

    申请日:1993-01-07

    Abstract: To calibrate a photodetector, a rotating disk with a slot is disposed in a light beam with decreasing speed from a defined maximum rotational speed to a defined minimum speed, while magnitudes and times of signals are read out and stored. Vernier pairs of signals occur in adjacent readout intervals, and non-vernier signals exclude the verniers. Readout times for verniers are used to estimate a preliminary function of rotations versus time. From the function are estimated an occurrence time for each pair and period of disk rotation at the time. Vernier fraction is the ratio of one signal in the pair to the sum of the pair. A time offset is the product of vernier fraction, slot fraction of the disk and the estimated period. Occurrence times corrected with the time offset are utilized to fit a corrected function of disk rotations versus time. Points of time for the non-vernier signals are determined from the corrected function, each point corresponding to disk rotations to a corresponding non-vernier signal. These points of time are employed with corresponding signals for linearly calibrating the photodetector.

    17.
    发明专利
    未知

    公开(公告)号:DE69333054D1

    公开(公告)日:2003-07-24

    申请号:DE69333054

    申请日:1993-01-07

    Abstract: A method of establishing a precision wavelength point in a spectrometric instrument with a calibration source of a spectral peak of precisely identified wavelength and a nominal calibration of spectral wavelength versus spectral locations. A calibration profile representative of the at least one spectral peak is produced from which a centroid wavelength of the calibration profile with respect to the spectral locations is estimated. The calibration profile is reversed about the centroid wavelength to create a reversed profile. A combined profile is produced by addition. The calibration data are fitted to the combined profile to determine an offset between the estimated centroid wavelength and the primary spectral peak, whereby the offset defines the primary peak location with respect to the spectral locations.

    20.
    发明专利
    未知

    公开(公告)号:DE69315607D1

    公开(公告)日:1998-01-22

    申请号:DE69315607

    申请日:1993-01-07

    Abstract: A method of establishing a precision wavelength point in a spectrometric instrument with a calibration source of a spectral peak of precisely identified wavelength and a nominal calibration of spectral wavelength versus spectral locations. A calibration profile representative of the at least one spectral peak is produced from which a centroid wavelength of the calibration profile with respect to the spectral locations is estimated. The calibration profile is reversed about the centroid wavelength to create a reversed profile. A combined profile is produced by addition. The calibration data are fitted to the combined profile to determine an offset between the estimated centroid wavelength and the primary spectral peak, whereby the offset defines the primary peak location with respect to the spectral locations.

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