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Go up to 5 Common problems with wavefront reduction.
Go forward to 5.2 Problems with the program.

5.1 Problems affecting the the reconstructed wavefront.

5.1.1 Corrected extra-focal images look under or over sized.

If you have not selected manually set extra-focal image diameter, the expected size of the extra-focal image is computed from the f-ratio and the extra-focal distance. In either case the CCD camera pixel size is then used to compute the number of pixels expected across the extra-focal image. This is one of the most critical numbers needed for the program, and you should try to specify parameters so that the diameter is known within 1% or better. An error in this diameter (a scaling error) will lead to errors in determining the wavefront. Unfortunately it is not possible for the program to detect in an general manner when this happens. Often you will have little indication that the wavefront reconstruction is incorrect when the program uses an incorrect extra-focal image size.

5.1.2 Focus apparently wrong.

When the data reduction has finished, both corrected extra-focal images should be the same size. If this is not the case and the reconstructed wavefront contains a large focus term, then you probably have either problems background subtraction, or the integrated flux in each extrafocal image is different. To see the corrected extra-focal images, carry out a data reduction sequence, then invoke the Displays :: Display buffer menu item. In the resulting Display image buffer window perform the following operations:
  1. Select the Display destination radio button labeled Left.
  2. Select radio-button labeled Corrected extra-focal image 1.
  3. Press the Display button.
  4. Select the Display destination radio button labeled Right.
  5. Select radio-button labeled Corrected extra-focal image 2.
  6. Press the Display button.
You should now have both corrected extra-focal images displayed, one in each of the display buffers. The images should be the same size and circular. The images should be uniformly illuminated, except for high frequency structure that should appear positive in 1 image and negative in the other. The image radii should be roughly that specified in the Desired radius of output wavefront field of the Edit :: Algorithm parameters form. If one or more of the above conditions is not true, a problem with the data or the data-reduction is strongly indicated.

There are two main causes for an incorrect focus value, either a bad backgroud subtraction, or different different integrated intensity in the two extra-focal images.

5.1.2.1 Checking background subtraction.

Verify that bad background subtraction is the problem by loading your images in the usual way, and checking the background values, in comparison to the values inside the extra-focal images. If the background values are all of the same sign, and exceed a few percent of the image value, then you have inadequate background subtraction. Sometimes you may find that the background varies with focus position. In this case you can solve the problem by taking one dark image for each extra-focal image position. Since Dark images are subtracted when the extra-focal image is first loaded into the program you can apply these dark's to the appropriate ef image by following the following sequence of operations:
  1. Load first dark frame.
  2. Load first extra-focal image.
  3. Load second dark frame.
  4. Load second extra-focal image.
If this does not work, you need to improve the baffling of your extra-focal image camera, or use a separate image processing package to pre-process your images.

If you wish you may modify the image loading code (found in the file ef_file_menu_open.tcl) to apply more sophisticated processing.

If the residual from background subtraction is not uniform over the extra-focal image, you will also see spurious higher order aberrations generated by the program.

5.1.2.2 Checking integrated intensity.

If the background subtractions appears to be satisfacory there are still focus errors in the reconstructon, you should suspect that the extra-focal images have different integrated light levels. To test this try enabling theNormalise extra-focal images toggle in the Edit::Image pre-processing form. Now re-load the extra-focal images and try the data-reduction again. The normalistion fuction is normally disabled, because it can introduce problems if the images are too close to focus, or if there is any structure other than the extra-focal images themselves. Do not use this function unless it is really necessary.

5.1.3 Bad Quad Astigmatism.

In general the curvature technique has lower SNR for aberration terms which have no curvature. These terms include tip/tilt, astigmatism and Quad astigmatism, Zernikes 2,3,5,6,14,15 respectively. Zernike 14 is particularly prone to error, because it has the same symmetry as the image pixelation. If the reconstructed wavefront map contains a cross pattern which aligns with the x,y axis, you should carefully inspect your extrafocal images for any of the following problems.

5.1.4 Slow convergence.

You should find that the residual wavefront aberrations for those Zernike terms that are corrected by the algorithm are less than 10 percent of the total aberration. If this is not the case, and aberrations do not fall rapidly with continued manual iterations, then you may have a problem with large high order aberrations. Usually this will involve large aberrations near the edges of the wavefront. Evidence for this will appear as very bright arcs, and dark areas near the periphery of the extra-focal images. Essentially these parts of the extra-focal images may be near to non-linearity, while the rest of the image is good. Under these circumstances, there is likely to be some cross-coupling between high order aberrations an low order aberrations, with quite poor accuracy on the reconstructed wavefront. If the quality of the data is good, you may try using the highorder reduction sequence, available under the Edit :: Select reduction sequence. This sequence will correct higher order Zernikes and potentially give more accurate results. However with data of questionable quality, or with a very large central obscuration, the algorithm may become unstable in this mode. Instability is indicated if the two corrected extrafocal images are not circularly symmetric and/or significantly differ from each other.
Laplacian Optics Inc.     Email:   laplace@laplacian.com

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