Kundt tube spacing fit

ID: kundt-tube-spacing-fit

Write the measured positions of consecutive maxima of sound pressure amplitude as . The arbitrary origin is fitted along with the half-wavelength by linear regression; forcing the line through zero would turn a ruler-origin offset into an erroneous slope. For independent equal-variance position errors of standard deviation ,
As an original example, choose , and . Add stipulated position errors at . Their sum and index-weighted sum vanish, so the fitted values remain and , giving . These are synthetic inputs, not measurements of a particular air sample.
With stipulated and independent drive-frequency uncertainty , first-order uncertainty propagation gives
This statistical calculation omits common scale-calibration error, thermal drift and mode misidentification. Counting more positions reduces independent localization error; it cannot correct a wrong family of extrema or an incorrectly calibrated ruler.
Figure 1.
Pressure and fluid motion give shifted patterns but the same half-wavelength spacing
. Original lossless mode and synthetic regression example. Absolute spatial mode shapes show the positions of maxima; signed time traces at show their relative phase. The six positions and residuals are stipulated model data. No historical dust pattern or measured trace is reproduced. Source. Details.

New to topics? Read the docs here!