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halfpi_c

Table of contents
Procedure
Abstract
Required_Reading
Keywords
Brief_I/O
Detailed_Input
Detailed_Output
Parameters
Exceptions
Files
Particulars
Examples
Restrictions
Literature_References
Author_and_Institution
Version
Index_Entries

Procedure

   halfpi_c ( Half the value of pi ) 

   SpiceDouble halfpi_c ( void )

Abstract

   Return half the value of pi (the ratio of the circumference of
   a circle to its diameter).

Required_Reading

   None.

Keywords

   CONSTANTS


Brief_I/O

   The function returns half the value of pi.

Detailed_Input

   None.

Detailed_Output

   The function returns half the value of pi (the ratio of
   a circle's circumference to its diameter), determined by
   the ACOS function. That is,

         halfpi_c = acos ( -1.0 ) * 0.50

Parameters

   None.

Exceptions

   Error free.

Files

   None.

Particulars

   The first time the function is referenced, the value is computed
   as shown above. The value is saved, and returned directly upon
   subsequent reference.

Examples

   The numerical results shown for these examples may differ across
   platforms. The results depend on the SPICE kernels used as
   input, the compiler and supporting libraries, and the machine
   specific arithmetic implementation.

   1) The following code example returns the double precision value of
      the constant pi/2.0 and prints it out.

      Example code begins here.


      /.
         Program halfpi_ex1
      ./
      #include <stdio.h>
      #include "SpiceUsr.h"

      int main ()
      {
         /.
         Print the double precision value of pi/2.0
         ./
         printf( "Half pi: %25.22f\n", halfpi_c( ) );

         return ( 0 );
      }


      When this program was executed on a Mac/Intel/cc/64-bit
      platform, the output was:


      Half pi:  1.5707963267948965579990


   2) Compute the transformation from inertial to body fixed
      coordinates, given the directions of the north pole and prime
      meridian of the body.

      When using the following values for Pluto, extracted from the
      PCK kernel pck00010.tpc:

         Right ascension (deg): 132.993
         Declination     (deg):  -6.163
         Prime meridian  (deg): 302.695

      at ephemeris epoch 2000 Jan 1 12:00:00 TDB, the result should
      match that obtained using the following call:

         pxform_c ( "J2000", "IAU_PLUTO", 0.0, tipm );

      Use the PCK kernel below to load the triaxial ellipsoidal shape
      model and orientation data for Pluto.

         pck00010.tpc


      Example code begins here.


      /.
         Program halfpi_ex2
      ./
      #include <stdio.h>
      #include "SpiceUsr.h"

      int main ( )
      {
         /.
         Compute the transformation from inertial to body
         fixed coordinates, given the directions of the north
         pole and prime meridian of the body.

         Local variables.
         ./
         SpiceDouble   ra;
         SpiceDouble   dec;
         SpiceDouble   w;
         SpiceDouble   tipm [3][3];

         /.
         Load the PCK.
         ./
         furnsh_c ( "pck00010.tpc" );

         /.
         Assign the values for Pluto, in radians.
         ./
         ra  = 132.993 * rpd_c( );
         dec =  -6.163 * rpd_c( );
         w   = 302.695 * rpd_c( );

         /.
         The transformation is defined by the compound
         rotation

           [W] [pi/2 - Dec] [RA + pi/2]
              3            1           3
         ./
         rotate_c (        ra + halfpi_c(), 3, tipm );
         rotmat_c ( tipm, halfpi_c() - dec, 1, tipm );
         rotmat_c ( tipm, w,                3, tipm );

         /.
         Print the results
         ./
         printf( "Rotation matrix, from pole direction "
                 "and prime\nmeridian:\n"                  );
         printf( "   %12.6f %12.6f %12.6f\n",
                        tipm[0][0], tipm[1][0], tipm[2][0] );
         printf( "   %12.6f %12.6f %12.6f\n",
                        tipm[0][1], tipm[1][1], tipm[2][1] );
         printf( "   %12.6f %12.6f %12.6f\n",
                        tipm[0][2], tipm[1][2], tipm[2][2] );

         /.
         Use pxform_c to obtain the same transformation.
         ./
         pxform_c ( "J2000", "IAU_PLUTO", 0.0, tipm );
         printf( "\nRotation matrix, from pxform_c:\n"     );
         printf( "   %12.6f %12.6f %12.6f\n",
                        tipm[0][0], tipm[1][0], tipm[2][0] );
         printf( "   %12.6f %12.6f %12.6f\n",
                        tipm[0][1], tipm[1][1], tipm[2][1] );
         printf( "   %12.6f %12.6f %12.6f\n",
                        tipm[0][2], tipm[1][2], tipm[2][2] );

         return ( 0 );
      }


      When this program was executed on a Mac/Intel/cc/64-bit
      platform, the output was:


      Rotation matrix, from pole direction and prime
      meridian:
            -0.333489    -0.655091    -0.677968
            -0.434428    -0.531449     0.727210
            -0.836694     0.537045    -0.107357

      Rotation matrix, from pxform_c:
            -0.333489    -0.655091    -0.677968
            -0.434428    -0.531449     0.727210
            -0.836694     0.537045    -0.107357

Restrictions

   None.

Literature_References

   None.

Author_and_Institution

   J. Diaz del Rio     (ODC Space)
   E.D. Wright         (JPL)

Version

   -CSPICE Version 1.0.1, 13-AUG-2021 (JDR)

       Edited the header to comply with NAIF standard. Created simple example
       for retrieving pi/2.0 value, and converted code fragment into full
       example code.

   -CSPICE Version 1.0.0, 08-FEB-1998 (EDW)

Index_Entries

   half the value of pi
Fri Dec 31 18:41:08 2021