VERTICAL SCANNING INTERFEROMETRY VSI

1. VERTICAL SCANNING INTERFEROMETRY VSI

2. SURFACE TEXTURE IS ROUGHNESS & WAVINESS waviness lay (direction of dominant pattern) • Roughness is closely spaced irregularities such as cutting tool marks, disk texture, grit on a grinding wheel. • Waviness is more widely spaced irregularities such as disk runout and magnetic head crown. roughness profile roughness spacing waviness spacing

3. Ra • Roughness average (Ra) is the measure of the surface profile arithmetic average deviation from the center line. Units are in English, metric, or waves.

4. Rq • Root mean square roughness average (Rq) is the root mean square of the distance of the filtered or unfiltered roughness profile from its mean line. An older term for Rq is RMS. Because this parameter squares deviations from the mean, it is more sensitive to peaks and valleys. Units are in English, metric, and waves.

5. Rp, Rv, Rt • Roughness peak (Rp) is the highest peak distance from the mean line. • Roughness valley (Rv) is the lowest valley distance from the mean line. • Roughness peak to valley (Rt) is the distance from the lowest valley to the highest peak. mean line Rt = Rp + Rv Rt Rp Rv

6. APPLICATIONS • Ra is a stable, easily implemented parameter. • Rq is more sensitive to peaks and valleys. Better for discriminating different types of surfaces. • Peaks are important for friction and wear. • Valleys are significant for lubrication.

7. Ra, Rq, Rt LIMITATIONS The standard roughness parameters such as Ra, Rq, or Rt are not sensitive to spatial structure. They all treat positive and negative heights equally. Same Ra ,Rq, and Rt Same Ra ,Rq, and Rt

8. SURFACE FILTERING • Surface filtering is user defined roughness and waviness! • Roughness is closely spaced irregularities such as cutting tool marks, disk texture, grit on a grinding wheel. This can be more closely analyzed by subtracting the shape of the sample.

9. SURFACE FILTERING(Continued) • Waviness is more widely spaced irregularities such as disk runout, magnetic head crown, etc. This can be more closely analyzed by using a low pass filter. • Flaws are discrete infrequent irregularities such as disk damage due to head slap, contamination, ESD damage, etc.

10. Typical Interferometer • A -The expanded beam exiting from the light source is divided by beamsplitter into two beams. CCD C A Reference arm • B - One beam is reflected from the Reference Mirror, and the other one from the Sample. Reference Mirror B Test arm Beamsplitter • C - These two beams are recombined by the beamsplitter to interfere. Sample Optical Path Difference (OPD) - difference in optical path lengths that beams travel in the reference and test arms. • D - The imaging lens images the interferogram onto the CCD camera.

11. Tilt of one of Mirrors in Interferometer CCD then reflected beam (wavefront) also is tilted. If one of the mirrors is slightly tilted, Reference Mirror Beamsplitter Sample For two tilted and flat wavefronts an interferogram in form of straight, parallel light and dark bands will be formed.

12. Interferogram

13. 4 3 2  Intensity profile of interferogram. Interferogram, (interference pattern or fringe pattern) Interferogram for Flat Wavefronts with Tilt Two interfering wavefronts Multiple  distances between wavefronts, where  is the wavelength of the source. Tested beam (wavefront) Reference beam (wavefront). Interference between two wavefronts is constructive at these multiple  points, destructive at others, forming an interferogram. Fringe spacing corresponds to  path difference between wavefronts.

14. 9 8 7 6 5 4 3 3 2 2 1 1 1 Tilt between Sample and Reference Mirror Interferograms represent increasing amount of tilt between interfering wavefronts, however the direction of tilt is unknown. Number and fringe spacing is changing with tilt.

15. NULL FRINGES When wavefronts are parallel then the fringes are nulled and almost uniform intensity is visible in the field of view. Change in Tilt Causes Change in Number of Fringes. Number and fringe spacing is changing with tilt.

16. Change in Arms Length Shifts Fringes. Change in length of one of the arms introduces a phase shift between interfering wavefronts causing fringes to shift to a new location. Note that number of fringes and their orientation remains the same.

17. Two-beam Interference Fringes Sinusoidal profile of fringes can be represented by the equation: or I=Ibackground+2Iamplitudecos(f + f(t)) where I1 and I2 ¯ are intensities of two beams, phaseshift measured object phase is a distance between the two interfering beams, called Optical Path Difference (OPD) 1- 2 ¯

18. When one wavefront is spherical and the other is flat, and in addition there is some tilt between interfering wavefronts, then the fringes will be curved. When tilt is not present, the fringes are circular. Interferograms for Spherical Sample

19. The fringes can represent a concave wavefront instead convex wavefront as on previous slide. Interferograms for Spherical Sample

20. 2 3 2d 2d Surface Height Scaling Factor 1 Incident beam Tested object d Heights in the reflected wavefront are double the actual heights of tested object 4 Fringe spacing corresponds to  /2 surface height change. d Heights of reflected wavefront need to be scaled times 1/2.

21. l 2 ( )( ) D S Height Error & Fringe Deviation Fringe spacing S corresponds to l /2 surface height change with respect to the reference surface. D(x,y) Fringe deviation corresponds to surface height error S Quick estimation of maximum deviation from straightness

22. Typical Interferogram for Flat Surface Fringes Phase map  3 2

23. Typical Interferogram for Spherical Surface Fringes Phase map

24. Typical Interferogram for Cylindrical Surfaces Phase map Fringes

25. White Light Interferogram

26. White Light Fringes • Interferogram can be obtained with a white light source, such as halogen lamp. Fringes for: blue light green light yellow light red light • Beams at different wavelengths interfere. • Sets of fringes for different wavelengths are created. • Spacing between fringes depends on wavelength.

27. White Light Fringes • The sum of all interference signals is observed forming a fringe pattern with quickly decreasing modulation. • Fringe modulation achieves a maximum for equal optical paths of both beams (there OPD=0). • White light fringe modulation decreases very fast thus optical paths of both beams has to be set with a great caution.

28. Profile Interferograms of Diffraction Grating Red Light White Light

29. White Light Interference Fringes • Fringes form bands of contour of equal height on the surface with respect to the reference surface. • Fringe contrast will be greatest at point of equal path length or “best focus”

30. Principles of Vertical Scanning Interferometry • A difference between the reference and test optical paths causes a difference in phase • Interference is perfectly constructive only when there is ZERO optical path difference • Best focus corresponds to zero optical path difference

31. Computerized Interferogram Analysis For large height range or rough samples Vertical resolution about 3nm Uses light of wide bandwidth i.e. white light

32. Focus

33. Focus

34. Vertical Scanning Interferometry • Measure changes in surface height up to 1mm. • Measure the intensity at each pixel as the objective is moving vertically. • Analyze the intensity while moving through focus to determine the height of the surface at each pixel.

35. Typical White Light Fringes for Stepped Surface Phase map Fringes From a single interferogram and no apriori knowledge we can not determine if the step is up or down.

36. Intensity at Two Points while Focusing on a Step

37. Typical Interferometer CCD Reference Mirror Beamsplitter Sample

38. Translator Mirau Interferometer • Interference • Microscope Diagram Digitized Intensity Data Detector Array Beamsplitter Illuminator Microscope Objective Light Source Field Stop Aperture Stop Sample

39. Focus Position B Vertical Scanning Interferometer VSI White Light Interferograms Focus Position A As the scan moves different areas of the part being measured come into focus (have zero OPD or maximum contrast between fringes). A determination of the point of maximum contrast and knowledge of the motor position allows a reconstruction of the surface shape.

40. VSI result

41. Typical White Light Fringes for Rough Surface Focus Position A Focus Position A

42. Intensity Signal Through Focus where Intensity Coherence envelope OPD 0

43. Principles Of Operation • The coherence function has a maximum when the OPD is zero (i.e. when you are in best focus). • Position of the peak of the coherence function gives a relative measure of surface height. • Locate the peak of the coherence function at every pixel in order to reconstruct the surface.

44. Advantages of VSI • True 3D measurement of surface area. • Ability to measure non-specular surfaces. • Good results with low contrast fringes. • Results independent of intensity variations across field of view. • Vertical height limited only by scanner and objective working distance. • No step height ambiguities. • Tested area always in focus.

45. Go to VSI option screen VSI Menu Select this Icon for the Measurement Options Dialog

46. Computerized Interferogram Analysis

47. Computerized Interferometric Microscope For Surface Profile PSI High Precision VSI Large Dynamic Range