Simple matrix method for stray-light correction in imaging instruments

• US 20090059210A1
• Filed: 08/13/2008
• Published: 03/05/2009
• Est. Priority Date: 08/15/2007
• Status: Active Grant

• Current Assignee: Keith R. Lykke, Steven W. Brown, Yoshihiro Ohno, Yuqin Zong
• Original Assignee: Keith R. Lykke, Steven W. Brown, Yoshihiro Ohno, Yuqin Zong
• Inventors: Zong, Yuqin, Brown, Steven W., Lykke, Keith R., Ohno, Yoshihiro
• Granted Patent: US 8,554,009 B2
• Time in Patent Office: Days
• US Class Current: 356/124
• CPC Class Codes: G01J 1/08 Arrangements of light sources specially adapted for photometry standard sources, also using luminescent or radioactive material
• CPC Class Codes: G01J 1/4228 arrangements with two or more detectors, e.g. for sensitivity compensation
• CPC Class Codes: G01J 3/28 Investigating the spectrum using colour filters G01J3/51
• CPC Class Codes: G02B 27/0018 with means for preventing ghost images anti-reflection coatings G02B1/11
• CPC Class Codes: H04N 17/002 for television cameras
• CPC Class Codes: H04N 23/80 Camera processing pipelines; Components thereof
• CPC Class Codes: H04N 23/81 for suppressing or minimising disturbance in the image signal generation
• CPC Class Codes: H04N 25/61 the noise originating only from the lens unit, e.g. flare, shading, vignetting or "cos4"

Abstract

A simple matrix method and computer program product for stray-light correction in imaging instruments is provided. The stray-light correction method includes receiving raw signals from an imaging instrument and characterizing the imaging instrument for a set of point spread functions. For high resolution imaging instruments, the raw signals may be compressed to reduce the size of the correction matrix. Based on stray-light distribution functions derived from the point spread functions, a correction matrix is derived. This fast correction is performed by a matrix multiplication to the measured raw signals, and may reduce stray-light errors by more than one order of magnitude. Using the stray-light corrected instrument, significant reductions may be made in overall measurement uncertainties in radiometry, colorimetry, photometry and other applications. Because the PSFs may include other types of undesired responses, the stray-light correction also eliminates other types of errors, e.g., interreflection between a CCD and the detector window.

Claims

1. A simple matrix method for stray-light correction in an imaging instrument, comprising the steps of:

determining a set of point spread functions for the imaging instrument;

deriving a stray-light distribution function for each of said point spread functions;

based on the derived stray-light distribution functions, obtaining a stray-light distribution matrix; and

deriving a stray-light correction matrix, including inverting the stray-light distribution matrix and an identity matrix.

2. The method of claim 1, wherein the step of determining a set of point spread functions includes the step of:

receiving, from the imaging instrument, measured raw signals of a light source.

3. The method of claim 2, wherein the measured raw signals represent radiance or luminance of a light source.

4. The method of claim 2, wherein the light source is a point source.

5. The method of claim 2, further comprising:

binning or compressing the measured raw signals to reduce the number of measured raw signals.

6. The method of claim 2, further comprising:

binning or compressing the measured raw signals, thus reducing the number of measured raw signals without reducing the resolution of an image that is received with the measured raw signals.

7. The method of claim 1, wherein the obtaining step includes the steps of:

interpolating or extrapolating among the derived stray-light distribution functions to obtain additional stray-light distribution functions.

8. The method of claim 1, wherein the obtaining step includes the step of:

transforming each stray-light distribution function to a one-dimensional column vector.

9. The method of claim 1, further comprising the step of:

correcting stray-light errors based on the stray-light correction matrix.

10. A computer program product comprising a computer useable medium having computer readable code embodied therein for a simple matrix method for stray-light correction, the computer program product comprising:

point spread function code for causing the computer to determine a set of point spread functions for the imaging instrument;

stray-light distribution function code for causing the computer to derive a stray-light distribution function for each of said point spread functions;

stray-light distribution matrix code for causing the computer to obtain a stray-light distribution matrix based on the derived stray-light distribution functions; and

stray-light correction matrix code for causing the computer to derive a stray-light correction matrix, including code for causing the computer to invert the stray-light distribution matrix and an identity matrix.

11. The computer program product of claim 10, wherein the point spread function code includes receiving code for causing the computer to receive, from the imaging instrument, measured raw signals for radiance or luminance of a point source.

12. The computer program product of claim 10, wherein the stray-light distribution matrix code includes interpolation/extrapolation code for causing the computer to interpolate or extrapolate among the derived stray-light distribution functions to obtain additional stray-light distribution functions.

13. The computer program product of claim 10, wherein the stray-light distribution matrix code includes transformation code for causing the computer to transform each of the obtained stray-light distribution functions to a one-dimensional column vector.

14. The computer program product of claim 10, further comprising:

binning/compressing code for causing the computer to bin or compress the measured raw signals to a lesser number of signals.

15. The computer program product of claim 10, further comprising:

stray-light correction code for causing the computer to correct stray-light errors based on the stray-light correction matrix.

16. The computer program product of claim 10, further comprising:

binning/compressing code for causing the computer to bin or compress the measured raw signals to a lesser number of signals, without reducing the resolution of an image that is received with the measured raw signals.

17. A simple matrix method for stray-light correction in an imaging instrument, comprising the steps of:

receiving, from the imaging instrument, measured raw signals of a light source;

binning or compressing the measured raw signals to reduce the number of measured raw signals;

based on the binned/compressed raw signals, determining a set of point spread functions for the imaging instrument;

deriving a stray-light distribution function for each of said point spread functions;

based on the derived stray-light distribution functions, obtaining a stray-light distribution matrix; and

deriving a stray-light correction matrix, including inverting the stray-light distribution matrix and an identity matrix.

18. The method of claim 17, wherein the measured raw signals include signals that represent radiance or luminance of a light source.

19. The method of claim 18, wherein the light source is a point source.

20. The method of claim 17, wherein the obtaining step includes the steps of:

interpolating or extrapolating among the derived stray-light distribution functions to obtain additional stray-light distribution functions.

21. The method of claim 18, wherein the obtaining step includes the step of:

transforming each stray-light distribution function to a one-dimensional column vector.

23. The method of claim 21, further comprising:

correcting stray-light errors based on the stray-light correction matrix.

24. The method of claim 21, wherein the binning or compression technique is further configured to reduce the number of elements in the correction matrix without reducing the resolution of an image that is received with the measured raw signals.

22. A simple matrix method for stray-light correction in an imaging instrument, comprising the steps of:

receiving, from the imaging instrument, measured raw signals of a light source;

based on the raw signals, determining a set of point spread functions for the imaging instrument;

deriving a stray-light distribution function for each of said point spread functions;

based on the derived stray-light distribution functions, obtaining a stray-light distribution matrix;

deriving a stray-light correction matrix, including inverting the stray-light distribution matrix and an identity matrix, wherein the stray-light correction matrix includes a number of elements; and

applying a binning or compression technique to reduce the number of elements in the correction matrix.