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The interpolation in the IDL program includes three commonly used methods: (1) simple linear interpolation, as described in Eq. (3)–(4); (2) least squares quadratic fit for each four-point neighborhood (x[i-1], x[i], x[i + 1], x[i + 2]) surrounding the interval; and (3) SPLINE fit, which is a polynomial function fitting function for the four surrounding points.
The best fitting function for all three models in the sense of a minimum —is (7).
Note 2: polr is the fitting function for the MASS package.
Hence, in the present study, we derived a fitting function for better explanation of the GNSS time series and prediction of the short-term evolution of postseismic deformation.
Fig. 2. Temperature-dependent transformations of 1 h-heated samples of SiO2 spheres of 1.5 μm diameter, measurements of neck diameter as a function of heating temperature, and the fitting function for surface diffusion sintering.
If the best fitting function for an ILD function was either a Boltzmann or an exponential function, the ILD function was termed monotonic.
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Using a spatial individual-based simulation model for simulating different movement behaviours, we derive fitting functions for the functional relationship between the parameters of the dispersal function and several details of movement behaviour.
Models include a first-level general linear model (GLM) analysis for fMRI data, a GLM implementation of the simplified reference tissue model (SRTM) with time-varying changes in "binding potentials", a second-level random-effects of mixed-effects model for summarizing first-level GLM analyses, and fitting functions for performing common fits of MRI data (e.g., T1, T2, ADC, DTI, …).
Two fitting functions for the skewed wind load factors of tubular-angle steel cross-arms were determined by nonlinear fitting analysis.
The models are derived by comparisons against beam theory, and the values of the parameters are presented in the form of fitting functions for a large range of arc angles.
Users can customize the predefined functions for the extraction of the spectrum from the echellogram and adjust the parameters for the fitting functions for the spectra of celestial objects, using "fine-tuning" options, as necessary.
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CEO of Professional Science Editing for Scientists @ prosciediting.com