This section presents extended modules designed for editing (correcting) SPM data. Using simple data editing tools presented in chapter Data Edit and Correction it is possible to correct many local scanning defects that can be found on SPM images. There are also many error sources within SPM methods that lead to global errors, like low frequencies modulated on the data or data drift in the slow scanning axis.
Compensate Drift calculates and/or corrects drift in the fast scanning axis (horizontal). This adverse effect can be caused by thermal effects or insufficient mechanical rigidity of the measuring device.
The drift graph, which is one of possible outputs, represents the horizontal shift of individual rows compared to a reference row (which could be in principle chosen arbitrarily, in practice the zero shift is chosen to minimize the amount of data sticking out of the image after compensation), with the row y-coordinate on the abscissa.
The drift is determined in two steps:
Option Exclude linear skew subtracts the linear term from the calculated drift, it can be useful when the image is anisotropic and its features are supposed to be oriented in a direction not paralled to the image sides.
One excellent way of removing frequency based of noise from an image is to use Fourier filtering. First, the Fourier transform of the image is calculated. Next, a filter is applied to this transform. Finally, the inverse transform is applied to obtain a filtered image. Gwyddion uses the Fast Fourier Transform (or FFT) to make this intensive calculation much faster.
Within the 1D FFT filter the frequencies that should be removed from spectrum (suppress type: null) or supressed to value of neighbouring frequencies (suppress type: suppress) can be selected by marking appropriate areas in the power spectrum graph. The selection can be inverted easily using the Filter type choice. 1D FFT filter can be used both for horizontal and vertical direction.
2D FFT filter acts similarly as the 1D variant (see above) but using 2D FFT transform. Therefore, the spatial frequencies that should be filtered must be selected in 2D using mask editor. As the frequencies are related to center of the image (corresponding to zero frequency), the mask can be snapped to the center (coordinate system origin) while being edited. There are also different display and output modes that are self-explanatory – image or FFT coefficients can be outputted by module (or both).
Note that the filter usually resamples the data to size that fits to the available FFT algorithm (FFTW or Gwyddion FFT). As this may affect results, the resampled image size information is stated in the module window.
General distortion in the horizontal plane can be compensated, or created, with Polynomial distortion. It performs transforms that can be expressed as
where Px and Py are polynomials up to the third total order with user-defined coefficients. Note the direction of the coordinate transform – the reverse direction would not guarantee an unambiguous mapping.
The polynomial coefficients are entered as scale-free, i.e. as if the coordinate ranges were always [0, 1]. If Instant updates are enabled, pressing Enter in a coefficient entry (or just leaving moving keyboard focus elsewhere) updates the preview.
Calculates denoised image on the basis of two measurements of the same area - one performed in x direction and on 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 ). Module performs FFT of both images, combines information from both images in reciprocal space, and then performs backward FFT in order to get denoised image. It is useful namely for large scars and fast scanning axis stripes removal.