Stray light measurement and compensation

• US 4,526,470 A
• Filed: 03/05/1982
• Issued: 07/02/1985
• Est. Priority Date: 03/05/1982
• Status: Expired due to Term

• Current Assignee: Beckman Instruments, Inc. (Danaher Corporation)
• Original Assignee: Beckman Instruments, Inc. (Danaher Corporation)
• Inventors: Kaye, Wilbur I.
• Primary Examiner(s): Evans, F. L.
• Application Number:
  US06/355,281
• Time in Patent Office: 1,215 Days
• Field of Search: 356/300, 356/319-325
• US Class Current: 356/319
• CPC Class Codes: G01J 3/28 Investigating the spectrum using colour filters G01J3/51
• CPC Class Codes: G01J 3/42 Absorption spectrometry; Double beam spectrometry; Flicker spectrometry; Reflection spectrometry beam switching arrangements G01J3/08
• CPC Class Codes: G01N 2201/064 Stray light conditioning

Abstract

Methods for stray light measurement and compensation in spectrophotometers are disclosed. In one exemplary embodiment, stray light is determined as a convolution of a selected detected radiant power spectrum and a monochromator slit function. Such a stray light measurement may be made with or without the sample in an optical path between a source and detector within the spectrophotometer. When made with the sample in the optical path, the resulting stray light measurement may be used to compensate sample absorbance or transmittance measurements. In accordance with another embodiment of the present invention, sample absorbance or transmittance may be compensated in a method including measuring sample detected radiant power at a wavelength outside an interval of significant detected radiant power within which a sample measurement compensated for stray is desired.

Claims

1. A method for determining stray light in a spectrophotometer at a first wavelength where the spectrophotometer has an optical path including a monochromator generating an output beam having a central wavelength and a predetermined slit function, a detector positioned to receive radiation from the monochromator, and means for substantially limiting detector response to radiation within an interval of significant detected radiant power, the interval of significant detected radiant power including the first wavelength, the method comprising the steps of:

(a) measuring a detected radiant power spectrum for a range of central wavelengths including at least the interval of significant detected radiant power,

(b) summing the product of the slit function and the detected radiant power spectrum over a first range of summation wavelengths including at least the interval of significant detected radiant power, but not including wavelengths within a predetermined interval around the first wavelength, and

(c) scaling the result of step (b) by a constant to determine stray light, the constant having a value such that a summation of the products of the slit function and the detected radiant power spectrum over a second range of summation wavelengths including at least the interval of significant detected radiant power, when scaled by the constant, is equal to a detected radiant power at a second wavelength outside the interval of significant detected radiant power.

2. The method of claim 1 wherein the spectrophotometer includes sample receiving means adapted to receive a sample such that the sample is in the optical path, and wherein step (a) comprises measuring the detected radiant power spectrum with a sample in the optical path such that the detected radiant power spectrum includes a detected radiant power at the first wavelength.

3. The method of claim 2 further including

(d) subtracting the stray light determined by step (c) from the detected radiant power at the first wavelength to determine a detected radiant power at the first wavelength compensated for stray light;

(e) measuring a detected radiant power without a sample in the optical path at the first wavelength; and

(f) dividing the result of step (d) by the result of step (e) to determine sample transmittance at the first wavelength corrected for stray light.

4. The method of claim 1 further including

(d) determining a detected radiant power at the first wavelength, and

(e) forming a ratio of the result of step (c) to the detected radiant power of step (d) to determine a stray light ratio.

5. The method of claim 2 further including

(d) measuring a detected radiant power without the sample in the optical path at the first wavelength, and

(e) forming a ratio of the result of step (c) to the detected radiant power of step (d) to determine a stray light ratio.

6. The method of claim 1 wherein step (b) includes selecting the slit function value for each product according to the difference between the first wavelength and the summation wavelength for the respective product.

7. The method of claim 6 wherein the slit function value for each product of step (c) is selected according to the difference between the first wavelength and the summation wavelength for the respective product.

8. A convolution method for determining stray light in a spectrophotometer at a first wavelength where the spectrophotometer has an optical path including a monochromator generating an output beam having a central wavelength and having a predetermined slit function, a detector positioned to receive radiation from the monochromator, and means for substantially limiting detector response to radiation having wavelengths within an interval of significant detected radiant power, the interval of significant detected radiant power including the first wavelength, the method comprising the steps of:

(a) measuring a detected radiant power spectrum for a range of central wavelengths including at least the interval of significant detected radiant power;

(b) measuring a detected radiant power at a second wavelength outside the interval of significant detected radiant power;

(c) selecting a first plurality of summation wavelengths over a range of wavelengths including at least the interval of significant detected radiant power;

(d) summing the products of the slit function and the detected radiant power spectrum for the first plurality of summation wavelengths, the slit function for each such product determined by the difference between the first wavelength and the summation wavelength for the respective product, the detected radiant power for each product determined by the summation wavelength for the respective product;

(e) selecting a constant such that the result of step (d) scaled by the constant is equal to the detected radiant power at the second wavelength;

(f) selecting a second plurality of summation wavelengths over a range of wavelengths including at least the interval of significant detected radiant power, but not including wavelengths within a predetermined interval around the first wavelength;

(g) summing the products of the slit function and the detected radiant power spectrum for the second plurality of summation wavelengths, the slit function for each such product determined by the difference between the first wavelength and the summation wavelength for the respective product, the detected radiant power spectrum for each such product determined by the summation wavelength for the respective product; and

(h) scaling the result of step (g) by the constant to determine stray light.

9. The method of claim 8 wherein the spectrophotometer includes sample receiving means adapted to receive a sample such that the sample is in the optical path, and wherein step (a) comprises measuring the detected radiant power spectrum with a sample in the optical path such that the detected radiant power spectrum includes a detected radiant power at the first wavelength.

10. The method of claim 9 further including

(i) subtracting the stray light determined by step (h) from the detected radiant power at the first wavelength to determine a detected radiant power at the first wavelength compensated for stray light;

(j) measuring a detected radiant power without a sample in the optical path at the first wavelength; and

(k) dividing the result of step (i) by the result of step (j) to determine sample transmittance at the first wavelength corrected for stray light.

11. A method for compensating sample transmittance at a first wavelength for stray light in a spectrophotometer where the spectrophotometer has an optical path including a monochromator generating an output beam having an adjustable central wavelength, a detector positioned to receive radiant power from the monochromator, and means for substantially limiting detector response to radiation having wavelengths within an interval of significant detected radiant power, the interval of significant detected radiant power including the first wavelength, the method comprising the steps of

determining a reference detected radiant power with the central wavelength at the first wavelength without the sample in the optical path;

determining a second detected radiant power with the central wavelength at the first wavelength with the sample in the optical path;

determining a third detected radiant power with the central wavelength at a second wavelength outside the interval of significant detected radiant power with the sample in the optical path; and

subtracting the third detected radiant power from the second detected radiant power and determining the ratio of the result to the reference detected radiant power to determine sample transmittance corrected for stray light.

12. A method for compensating sample transmittance at a first wavelength for stray light in a spectrophotometer where the spectrophotometer has an optical path including a monochromator generating an output beam having an adjustable central wavelength, a detector positioned to receive radiant power from the monochromator, the method comprising the steps of

(a) substantially limiting detector response to radiation having wavelengths within an interval of significant detected radiant power, the interval of significant detected radiant power including the first wavelength;

(b) determining a reference detected radiant power with the central wavelength at the first wavelength without the sample in the optical path;

(c) determining a second detected radiant power with the central wavelength at the first wavelength with the sample in the optical path;

(d) determining a third detected radiant power with the central wavelength at a second wavelength outside the interval of significant detected radiant power with the sample in the optical path; and

(e) subtracting the third detected radiant power from the second detected radiant power and determining the ratio of the result to the reference detected radiant power.

13. The method of claim 12 wherein step (a) includes limiting detector response by means of a blocking filter.