This section describes functions for marking and correction of various artefacts in SPM data related to the line by line acquisition. Scan line alignment and correction methods frequently involve heavy data modification which should be avoided if possible. Unfortunately, scan line defects are ubiquitous and, also frequently, correction may be the only way to proceed. Nevertheless, they should be applied with care.
See also section Data Editing and Correction for methods that deal with general local defects.
Profiles taken in the fast scanning axis (usually x-axis) can be mutually shifted by some amount or have slightly different slopes. The basic line correction function → → deals with this type of discrepancy using several different correction algorithms:
A basic correction method, based on finding a representative height of each scan line and subtracting it, thus moving the lines to the same height. Here the line median is used as the representative height.
This method differs from Median only in the quantity used: modus of the height distribution. Of course, the modus is only estimated because only a finite set of heights is avaiable.
The Polynomial method fits a polynomial of given degree and subtracts if from the line. For polynomial degree of 0 the mean value of each row is subtracted. Degree 1 means removal of linear slopes, degree 2 bow removal, etc.
In contrast to shifting a representative height for each line,shifts the lines so that the median of height differences (between vertical neighbour pixels) becomes zero. Therefore it better preserves large features while it is more sensitive to completely bogus lines.
This algorithm is somewhat experimental but it may be useful sometimes. It minimizes a certain line difference function that gives more weight to flat areas and less weight to areas with large slopes.
Inspired by Facet level, this method tilts individual scan lines to make the prevalent normals vertical. This only removes tilt; line height offsets are preserved. In one dimension it is generally a somewhat less effective strategy than for images. However, it can correct the tilt in some cases when other methods do not work at all.
Trimmed mean lies between the standard mean value and median, depending on how large fraction of lowest and highest values are trimmed. For no trimming (0) this method is equivalent to mean value subtraction, i.e. Polynomial with degree 0, for maximum possible trimming (0.5) it is equivalent to Median.
This method similarly offers a continous transition between Median difference and mean value subtraction. It makes zero the trimmed means of height differences (between vertical neighbour pixels). For the maximum possible trimming (0.5) it is equivalent to Median difference. Since the mean difference is the same as the difference of mean values (unlike for medians), for no trimming (0) it is again equivalent to Polynomial with degree 0.
Similarly as in the two-dimensional polynomial levelling, the background, i.e. values subtracted from individual rows can be extracted to another image. Or plotted in a graph since the value is the same for the entire row.
The line correction function support masking, allowing the exclusion of large features that could distract the corection algorithms. The masking options are offered only if a mask is present though. Note the Path level tools described below offers a different method of choosing the image parts important for alignment. It can be more convenient in some cases.
The Path Leveling tool can be used to correct the heights in an arbitrary subset of rows in complicated images.
First, one selects a number of straight lines on the data. The intersections of these lines with the rows then form a set of points in each row that is used for leveling. The rows are moved up or down to minimize the difference between the heights of the points of adjacent rows. Rows that are not intersected by any line are not moved (relatively to neighbouring rows).
Functionattempts to deal with shifts that may occur in the middle of a scan line. It tries to identify misaligned segments within the rows and correct the height of each such segment individually. Therefore it is often able to correct data with discontinuities in the middle of a row. This function is somewhat experimental and the exact way it works can be subject to futher changes.
Function Laplace's interpolation for correction.finds scan lines with vertically inverted features and marks them with a mask. Line inversion is an artefact which occasionally occurs for instance in Magnetic Force Microscopy. Since the line is generally only inverted very approximately, value inversion would be a poor correction and one should usually use
Mark Scars module can create a mask
of the points treated as scars. Unlike
which directly interpolates the located defects, this module lets you
interactively set several parameters which can fine-tune the scar
After clickingthe new scar mask will be applied to the image. Other modules or tools can then be run to edit this data.
Scars (or stripes, strokes) are parts of the image that are corrupted by a very common scanning error: local fault of the closed loop. Line defects are usually parallel to the fast scanning axis in the image. This function will automatically find and remove these scars, using neighbourhood lines to “fill-in” the gaps. The method is run with the last settings used in Mark Scars.
The function denoises and image on the basis of two measurements of the same area – one performed in x direction and one in y direction (and rotated back to be aligned the same way as the x-direction one). It is based on work of E. Anguiano and M. Aguilar (see ).
The denoising works by performing the Fourier transform of both images, combining the information them in the frequency space, and then using backward Fourier transform in order to get the denoised image. It is useful namely for the removal of large scars and fast scanning axis stripes.