# include <math.h>
# include <stdlib.h>
# include <stdio.h>
# include <time.h>

# include "asa111.h"

/******************************************************************************/

void normal_01_cdf_values ( int *n_data, double *x, double *fx )

/******************************************************************************/
/*
  Purpose:

    NORMAL_01_CDF_VALUES returns some values of the Normal 01 CDF.

  Discussion:

    In Mathematica, the function can be evaluated by:

      Needs["Statistics`ContinuousDistributions`"]
      dist = NormalDistribution [ 0, 1 ]
      CDF [ dist, x ]

  Licensing:

    This code is distributed under the GNU LGPL license. 

  Modified:

    28 August 2004

  Author:

    John Burkardt

  Reference:

    Milton Abramowitz, Irene Stegun,
    Handbook of Mathematical Functions,
    National Bureau of Standards, 1964,
    ISBN: 0-486-61272-4,
    LC: QA47.A34.

    Stephen Wolfram,
    The Mathematica Book,
    Fourth Edition,
    Cambridge University Press, 1999,
    ISBN: 0-521-64314-7,
    LC: QA76.95.W65.

  Parameters:

    Input/output, int *N_DATA.  The user sets N_DATA to 0 before the
    first call.  On each call, the routine increments N_DATA by 1, and
    returns the corresponding data; when there is no more data, the
    output value of N_DATA will be 0 again.

    Output, double *X, the argument of the function.

    Output, double *FX, the value of the function.
*/
{
# define N_MAX 17

  double fx_vec[N_MAX] = { 
     0.5000000000000000E+00,  
     0.5398278372770290E+00,  
     0.5792597094391030E+00,  
     0.6179114221889526E+00,  
     0.6554217416103242E+00,  
     0.6914624612740131E+00,  
     0.7257468822499270E+00,  
     0.7580363477769270E+00,  
     0.7881446014166033E+00,  
     0.8159398746532405E+00,  
     0.8413447460685429E+00,  
     0.9331927987311419E+00,  
     0.9772498680518208E+00,  
     0.9937903346742239E+00,  
     0.9986501019683699E+00,  
     0.9997673709209645E+00,  
     0.9999683287581669E+00 };

  double x_vec[N_MAX] = { 
     0.0000000000000000E+00,    
     0.1000000000000000E+00,  
     0.2000000000000000E+00,  
     0.3000000000000000E+00,  
     0.4000000000000000E+00,  
     0.5000000000000000E+00,  
     0.6000000000000000E+00,  
     0.7000000000000000E+00,  
     0.8000000000000000E+00,  
     0.9000000000000000E+00,  
     0.1000000000000000E+01,  
     0.1500000000000000E+01,  
     0.2000000000000000E+01,  
     0.2500000000000000E+01,  
     0.3000000000000000E+01,  
     0.3500000000000000E+01,  
     0.4000000000000000E+01 };

  if ( *n_data < 0 )
  {
    *n_data = 0;
  }

  *n_data = *n_data + 1;

  if ( N_MAX < *n_data )
  {
    *n_data = 0;
    *x = 0.0;
    *fx = 0.0;
  }
  else
  {
    *x = x_vec[*n_data-1];
    *fx = fx_vec[*n_data-1];
  }

  return;
# undef N_MAX
}
/******************************************************************************/

double ppnd ( double p, int *ifault )

/******************************************************************************/
/*
  Purpose:

    PPND produces the normal deviate value corresponding to lower tail area = P.

  Licensing:

    This code is distributed under the GNU LGPL license. 

  Modified:

    06 November 2010

  Author:

    Original FORTRAN77 version by J Beasley, S Springer.
    C version by John Burkardt.

  Reference:

    J Beasley, S Springer,
    Algorithm AS 111:
    The Percentage Points of the Normal Distribution,
    Applied Statistics,
    Volume 26, Number 1, 1977, pages 118-121.

  Parameters:

    Input, double P, the value of the cumulative probability
    densitity function.  0 < P < 1.

    Output, integer *IFAULT, error flag.
    0, no error.
    1, P <= 0 or P >= 1.  PPND is returned as 0.

    Output, double PPND, the normal deviate value with the property that
    the probability of a standard normal deviate being less than or
    equal to PPND is P.
*/
{
  double a0 = 2.50662823884;
  double a1 = -18.61500062529;
  double a2 = 41.39119773534;
  double a3 = -25.44106049637;
  double b1 = -8.47351093090;
  double b2 = 23.08336743743;
  double b3 = -21.06224101826;
  double b4 = 3.13082909833;
  double c0 = -2.78718931138;
  double c1 = -2.29796479134;
  double c2 = 4.85014127135;
  double c3 = 2.32121276858;
  double d1 = 3.54388924762;
  double d2 = 1.63706781897;
  double r;
  double split = 0.42;
  double value;

  *ifault = 0;
/*
  0.08 < P < 0.92
*/
  if ( fabs ( p - 0.5 ) <= split )
  {
    r = ( p - 0.5 ) * ( p - 0.5 );

    value = ( p - 0.5 ) * ( ( ( 
        a3   * r 
      + a2 ) * r 
      + a1 ) * r 
      + a0 ) / ( ( ( ( 
        b4   * r 
      + b3 ) * r 
      + b2 ) * r 
      + b1 ) * r 
      + 1.0 );
  }
/*
  P < 0.08 or P > 0.92,
  R = min ( P, 1-P )
*/
  else if ( 0.0 < p && p < 1.0 )
  {
    if ( 0.5 < p )
    {
      r = sqrt ( - log ( 1.0 - p ) );
    }
    else
    {
      r = sqrt ( - log ( p ) );
    }

    value = ( ( ( 
        c3   * r 
      + c2 ) * r 
      + c1 ) * r 
      + c0 ) / ( ( 
        d2   * r 
      + d1 ) * r 
      + 1.0 );

    if ( p < 0.5 )
    {
      value = - value;
    }
  }
/*
  P <= 0.0 or 1.0 <= P
*/
  else
  {
    *ifault = 1;
    value = 0.0;
  }

  return value;
}
/******************************************************************************/

void timestamp ( )

/******************************************************************************/
/*
  Purpose:

    TIMESTAMP prints the current YMDHMS date as a time stamp.

  Example:

    17 June 2014 09:45:54 AM

  Licensing:

    This code is distributed under the GNU LGPL license. 

  Modified:

    17 June 2014

  Author:

    John Burkardt

  Parameters:

    None
*/
{
# define TIME_SIZE 40

  static char time_buffer[TIME_SIZE];
  const struct tm *tm;
  time_t now;

  now = time ( NULL );
  tm = localtime ( &now );

  strftime ( time_buffer, TIME_SIZE, "%d %B %Y %I:%M:%S %p", tm );

  printf ( "%s\n", time_buffer );

  return;
# undef TIME_SIZE
}