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The minimum width of the fringe was about 4.9 times the pixel size, thus satisfying the sampling theorem.
In Fig. 5, peak count of the fringe degraded and the width of the fringe become wider with increasing distance from the fringe center.
If the non-crystalline content determined by WAXD integration is 100-63 = 47%, giving the fractional value (A), and the dimension associated with crystalline diffraction (L) from the 200 Scherrer calculation for straw is 2.8 nm, then the apparent width of the fringe for straw is found to be 0.43 nm.
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The spectral widths of the sky fringes are proportional to the width of the fringes.
The width of the fringes expands 170 km in east-west direction.
Because the FPI temperature is essentially measured from the width of the fringes, the larger finesse allows more accurate measurements of the temperature, and may contribute to differentiate the OH contamination.
The accuracy of the temperature determination strongly depends on the accuracy of the center determination of the interference fringes, because temperatures obtained by FPIs correspond to the width of the fringes.
This is because the wind velocity is determined from the shift of fringe peak locations which is less affected by the center location and azimuthal integration, while the temperature is determined by the width of the fringes, which are directly affected by the center location through the azimuthal fitting.
A similar calculation for the eucalyptus pulp gives the apparent width of the fibril fringe as 0.48 nm.
The object modulated by sinusoidal fringes is shown in Fig. 13a, the width of sinusoidal fringe is 16 pixels, and the object modulated by phase-coding fringes is shown in Fig. 13b.
The long strip was measured again in this part, and the width of sinusoidal fringe is 21.33 pixels (Fig. 17a d), and the period numbers while using the phase-coding fringe are 48, 24, 16, and 12.
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