Index of Functions: A B C D E F G H I J K L M N O P Q R S T U V W X
Index Page dskcls_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
       dskcls_c ( DSK, close file )

       void dskcls_c ( SpiceInt      handle,
                       SpiceBoolean  optmiz )
#### Abstract
       Close a DSK file.
#### Required_Reading
       DAS
       DSK
#### Keywords
       DAS
       DSK
       FILES
       TOPOGRAPHY
#### Brief_I/O
       VARIABLE  I/O  DESCRIPTION
       --------  ---  --------------------------------------------------
       handle     I   Handle assigned to the opened DSK file.
       optmiz     I   Flag indicating whether to segregate the DSK.
#### Detailed_Input
       handle      is the DAS file handle associated with the file.
                   The file may be open for read or write access.

       optmiz      is a logical flag indicating whether the DSK
                   should be segregated before it is closed. This
                   option applies only to files open for write
                   access. The value of `optmiz' has no effect for
                   files opened for read access.

                   See the DAS Required Reading das.req for a
                   discussion of segregation of DAS files.
#### Detailed_Output
       None. This routine operates by side effects.
#### Parameters
       None.
#### Exceptions
       1)  If an error occurs when the file is closed, the error is
           signaled by a routine in the call tree of this routine.
#### Files
       See argument `handle'.
#### Particulars
       This routine provides a DSK-level interface for closing DSK files.

       In cases where DSKs opened for write access are to be closed
       without segregation, this interface is slightly simpler than that
       available at the DAS level.
#### 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) Create a three-segment DSK file using plate model data for
          Phobos. Use latitudinal, rectangular, and planetodetic
          coordinates in the respective segments. This is not a
          realistic example, but it serves to demonstrate use of
          the supported coordinate systems.

          Use the DSK kernel below to provide, for simplicity, the
          input plate and vertex data. The selected input file has one
          segment.

             phobos_3_3.bds

          Example code begins here.

          /.
             Program dskcls_ex1

             Example program for dskw02_c, dskmi2_c, and dskrb2_c

             Create a three-segment DSK file using plate model data for
             Phobos. Use latitudinal, rectangular, and planetodetic
             coordinates in the respective segments.

             For simplicity, use an existing DSK file to provide the
             input plate and vertex data. The selected input file has one
             segment.

                Version 1.0.0 22-JAN-2016 (NJB)

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

          int main()
          {

             /.
             Local constants
             ./
             #define FILSIZ          256
             #define LNSIZE           81
             #define NCOR              4
             #define NSEG              3
             #define NAMLEN           21

             /.
             Local variables
             ./

             /.
             Below, we declare large arrays static to avoid stack
             overflow problems.
             ./

             SpiceBoolean            found;

             SpiceChar               cornam [ NCOR ][ NAMLEN ] =
                                     { "radius",
                                       "Z-coordinate",
                                       "Z-coordinate",
                                       "altitude" };

             SpiceChar             * dsk;
             SpiceChar             * frame;
             SpiceChar             * indsk;

             SpiceDLADescr           dladsc;

             SpiceDouble             corpar [ SPICE_DSK_NSYPAR ];
             SpiceDouble             f;
             SpiceDouble             finscl;
             SpiceDouble             first;
             SpiceDouble             last;
             SpiceDouble             mncor1;
             SpiceDouble             mncor2;
             SpiceDouble             mncor3;
             SpiceDouble             mxcor1;
             SpiceDouble             mxcor2;
             SpiceDouble             mxcor3;
             SpiceDouble             re;
             SpiceDouble             rp;

             /.
             Note: the values of SPICE_DSK02_MAXVRT and
             SPICE_DSK02_MAXPLT declared in SpiceDSK.h,
             integer spatial index dimension SPICE_DSK02_SPAISZ,
             and the workspace dimension SPICE_DSK02_MAXCEL
             are very large. Smaller buffers can be used for most
             applications.
             ./
             static SpiceDouble      spaixd [ SPICE_DSK02_SPADSZ ];
             static SpiceDouble      vrtces [ SPICE_DSK02_MAXVRT ][3];

             SpiceInt                center;
             SpiceInt                corscl;
             SpiceInt                corsys;
             SpiceInt                dclass;
             SpiceInt                handle;
             SpiceInt                i;
             SpiceInt                inhan;
             SpiceInt                np;
             SpiceInt                nv;
             static SpiceInt         plates [ SPICE_DSK02_MAXPLT ][3];
             SpiceInt                segno;
             static SpiceInt         spaixi [ SPICE_DSK02_SPAISZ ];
             SpiceInt                spaisz;
             SpiceInt                surfid;
             SpiceInt                voxpsz;
             SpiceInt                voxlsz;
             static SpiceInt         work   [ SPICE_DSK02_MAXCEL ][2];
             SpiceInt                worksz;

             /.
             Assign names of input and output DSK files.
             ./
             indsk = "phobos_3_3.bds";
             dsk   = "phobos_3_3_3seg.bds";

             /.
             Open input DSK for read access; find first segment.
             ./
             dasopr_c ( indsk, &inhan );
             dlabfs_c ( inhan, &dladsc, &found );

             /.
             Fetch vertices and plates from input DSK file.

             Note that vertex and plate indices are 1-based.
             ./
             printf ( "Reading input data...\n" );

             dskv02_c ( inhan, &dladsc, 1, SPICE_DSK02_MAXVRT,
                        &nv,   vrtces                           );
             dskp02_c ( inhan, &dladsc, 1, SPICE_DSK02_MAXPLT,
                        &np,   plates                           );

             printf ( "Done.\n" );

             /.
             Set input array sizes required by dskmi2_c.
             ./
             voxpsz = SPICE_DSK02_MAXVXP;
             voxlsz = SPICE_DSK02_MXNVLS;
             worksz = SPICE_DSK02_MAXCEL;
             spaisz = SPICE_DSK02_SPAISZ;

             /.
             Set fine and coarse voxel scales. (These usually
             need to determined by experimentation.)
             ./
             finscl = 5.0;
             corscl = 4;

             /.
             Open a new DSK file.
             ./
             dskopn_c ( dsk, dsk, 0, &handle );

             /.
             Create three segments and add them to the file.
             ./
             for ( segno = 1;  segno <= NSEG;  segno++ )
             {
                /.
                Create spatial index. We won't generate a
                vertex-plate mapping, so we set the flag
                for creating this map to "false."
                ./
                printf ( "Creating segment %d\n", (int)segno );
                printf ( "Creating spatial index...\n" );

                dskmi2_c ( nv,     vrtces,     np,     plates,
                           finscl, corscl,     worksz, voxpsz,
                           voxlsz, SPICEFALSE, spaisz, work,
                           spaixd, spaixi                    );

                printf ( "Done.\n" );

                /.
                Set up inputs describing segment attributes:

                - Central body: Phobos
                - Surface ID code: user's choice.
                  We use the segment number here.
                - Data class: general (arbitrary) shape
                - Body-fixed reference frame
                - Time coverage bounds (TBD)
                ./
                center = 401;
                surfid = segno;
                dclass = SPICE_DSK_GENCLS;
                frame  = "IAU_PHOBOS";

                first = -50 * jyear_c();
                last  =  50 * jyear_c();

                /.
                Set the coordinate system and coordinate system
                bounds based on the segment index.

                Zero out the coordinate parameters to start.
                ./
                for ( i = 0;  i < SPICE_DSK_NSYPAR;  i++ )
                {
                   corpar[i] = 0.0;
                }

                if ( segno == 1 )
                {
                   /.
                   Use planetocentric latitudinal coordinates. Set
                   the longitude and latitude bounds.
                   ./
                   corsys = SPICE_DSK_LATSYS;

                   mncor1 = -pi_c();
                   mxcor1 =  pi_c();
                   mncor2 = -pi_c()/2;
                   mxcor2 =  pi_c()/2;
                }
                else if ( segno == 2 )
                {

                   /.
                   Use rectangular coordinates. Set the
                   X and Y bounds.

                   The bounds shown here were derived from
                   the plate data. They lie slightly outside
                   of the range spanned by the plates.
                   ./
                   corsys = SPICE_DSK_RECSYS;

                   mncor1 = -1.3;
                   mxcor1 =  1.31;
                   mncor2 = -1.21;
                   mxcor2 =  1.2;
                }
                else
                {
                   /.
                   Set the coordinate system to planetodetic.
                   ./
                   corsys    = SPICE_DSK_PDTSYS;

                   mncor1    = -pi_c();
                   mxcor1    =  pi_c();
                   mncor2    = -pi_c()/2;
                   mxcor2    =  pi_c()/2;

                   /.
                   We'll use equatorial and polar radii from
                   pck00010.tpc. These normally would be fetched
                   at run time, but for simplicity, we'll use
                   hard-coded values.
                   ./
                   re        = 13.0;
                   rp        =  9.1;
                   f         = ( re - rp ) / re;

                   corpar[0] = re;
                   corpar[1] = f;
                }
                /.
                Compute plate model radius bounds.
                ./
                printf ( "Computing %s bounds of plate set...\n",
                         cornam[corsys-1]                        );

                dskrb2_c ( nv,     vrtces, np,      plates,
                           corsys, corpar, &mncor3, &mxcor3 );

                printf ( "Done.\n" );

                /.
                Write the segment to the file.
                ./
                printf ( "Writing segment...\n" );

                dskw02_c ( handle,
                           center, surfid, dclass, frame,  corsys,
                           corpar, mncor1, mxcor1, mncor2, mxcor2,
                           mncor3, mxcor3, first,  last,   nv,
                           vrtces, np,     plates, spaixd, spaixi );

                printf ( "Done.\n" );
             }

             /.
             Segregate the data records in the DSK file and
             close the file.
             ./
             printf ( "Segregating and closing DSK file...\n" );

             dskcls_c ( handle, SPICETRUE );

             printf ( "Done.\n" );

             return ( 0 );
          }

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

          Reading input data...
          Done.
          Creating segment 1
          Creating spatial index...
          Done.
          Computing radius bounds of plate set...
          Done.
          Writing segment...
          Done.
          Creating segment 2
          Creating spatial index...
          Done.
          Computing Z-coordinate bounds of plate set...
          Done.
          Writing segment...
          Done.
          Creating segment 3
          Creating spatial index...
          Done.
          Computing altitude bounds of plate set...
          Done.
          Writing segment...
          Done.
          Segregating and closing DSK file...
          Done.

          Note that after run completion, a new DSK exists in the output
          directory.

       2) Close a new DSK file using DAS segregation. `handle'
          is the DAS file handle of the DSK.

          This is the normal choice for DSK creation.

             dskcls_c ( HANDLE, SPICETRUE )

       3) Close a new DSK file without using DAS segregation. The
          close operation will be fast, but reading the file will be
          less efficient than if the file had been segregated.

             dskcls_c ( HANDLE, SPICEFALSE )

       4) Close an existing DSK file that had been opened
          for read access. In this case `optmiz' is ignored:

             dskcls_c ( HANDLE, SPICEFALSE )

          or

             dskcls_c ( HANDLE, SPICETRUE )
#### Restrictions
       1)  This routine should not be called by user applications
           that have loaded a DSK file via furnsh_c. Such applications
           should call the functions unload_c or kclear_c instead.
#### Literature_References
       None.
#### Author_and_Institution
       N.J. Bachman        (JPL)
       J. Diaz del Rio     (ODC Space)
#### Version
       -CSPICE Version 1.0.1, 06-JUL-2021 (JDR)

           Edited the header to comply with NAIF standard. Added
           complete code example based on example in dskmi2_c.

       -CSPICE Version 1.0.0, 23-JAN-2016 (NJB)
#### Index_Entries
       close a DSK file
#### Link to routine dskcls_c source file dskcls_c.c

    Fri Dec 31 18:41:04 2021