lamsf(3f) - [M_datapac:SPARSITY] compute the Tukey-Lambda sparsity function
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Input Arguments
Output Arguments
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SUBROUTINE LAMSF(P,Alamba,Sf)
REAL(kind=wp),intent(in) :: P REAL(kind=wp),intent(in) :: Alamba REAL(kind=wp),intent(out) :: Sf
LAMSF(3f) computes the sparsity function value for the (Tukey) lambda distribution with tail length parameter value = ALAMBA.In general, the probability density function for this distribution is not simple.
The percent point function for this distribution is
g(P) = ((P**ALAMBA)-((1-P)**ALAMBA))/ALAMBANote that the sparsity function of a distribution is the derivative of the percent point function, and also is the reciprocal of the probability density function (but in units of P rather than X).
P The value (between 0.0 and 1.0) at which the sparsity function is to be evaluated. ALAMBA The value of Lambda (the Tail Length parameter). If ALAMBA is positive, then P should be between 0.0 and 1.0, inclusively.If ALAMBA is non-positive, then P should be between 0.0 and 1.0, exclusively.
SF The sparsity function value for the Tukey Lambda distribution
Sample program:
program demo_lamsf use M_datapac, only : lamsf implicit none ! call lamsf(x,y) end program demo_lamsfResults:
The original DATAPAC library was written by James Filliben of the Statistical Engineering Division, National Institute of Standards and Technology.
John Urban, 2022.05.31
CC0-1.0
o Filliben, Simple and Robust Linear Estimation of the Location Parameter of a Symmetric Distribution (Unpublished PH.D. Dissertation, Princeton University), 1969, pages 21-44, 229-231, pages 53-58. o Filliben, The Percent Point Function, (Unpublished Manuscript), 1970, pages 28-31. o Hastings, Mosteller, Tukey, and Windsor, Low Moments for Small
Samples: A Comparative Study of Order Statistics, Annals of Mathematical Statistics, 18, 1947, pages 413-426.
Nemo Release 3.1 | lamsf (3) | February 23, 2025 |