Exact(3)
How well the total (T) thyroid interpolated the L and R MRT values was calculated as a coefficient of variation of interpolation, CV interpolation), from the standard deviation of the distances to interpolation, d = MRTTotal − min{MRTL, MRTR}, divided by the mean of their interpolation interval, ii = |MRTL − MRTR|.
The large difference stems from the dependence of the interpolation error on the width of the interpolation interval, e.g. for the BDF and the Adams-Moulton formula, this interval is four times larger.
The usefulness of our approach is its capacity to reliably predict a 29 day (or a 63 day interval estimated by interpolation) interval of relapse detection from crossing the WT1 ratio of 50, a relatively low ratio.
Similar(57)
The Wavelet and scalar coefficients are only dependant on the measured raw data of a surface and the filtering and lifting factors calculated by a cubic spline interpolation in an interval.
For each interpolation instant, the interval of nonuniform samples, within which lies is determined.
For suitable collocation points, we use the ( N − m + 1 ) nodes of the shifted Legendre-Gauss interpolation on the interval [ 0, T ].
Assume that (x^{(theta,vartheta)}_{N,j}), (0leqslant jleqslant N), are the zeros of the Jacobi-Gauss interpolation on the interval ((-1, 1)) and (varpi^{(theta,vartheta)}_{N,j}), (0leqslant jleqslant N), are the corresponding weights of this interpolation.
The nodes of the exponential Jacobi-Gauss interpolation on the interval ((0,infty)) are the zeros of (EJ_{N+1}^{(theta, vartheta)}(x)), which are denoted by (x^{(theta,vartheta)}_{R,N,j}), (0leqslant jleqslant N).
To accommodate the differences between the fault geometry, we applied a piecewise linear interpolation with an interval of 4 km for rectangular fault elements of 4 km × 4 km.
The nonlinear FDE is collocated at ( N − m + 1 ) nodes of the modified generalized Laguerre-Gauss interpolation on the interval Λ, and then the problem reduces to the ( N + 1 ) system of algebraic equations.
Denote the nodes and the corresponding Christoffel numbers of the shifted Legendre-Gauss interpolation on the interval ((0,tau_{m})) by (t_{tau_{m},k}^{N_{m}}) and (omega_{tau_{m},k}^{N_{m}}), (0leq kleq N_{m}), respectively.
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