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cspice_spkcov

Table of contents
Abstract
I/O
Parameters
Examples
Particulars
Exceptions
Files
Restrictions
Required_Reading
Literature_References
Author_and_Institution
Version
Index_Entries

Abstract


   CSPICE_SPKCOV finds the coverage window for a specified ephemeris object
   in a specified SPK file.

I/O


   Given:

      spkfnm   the name(s) of SPICE SPK file(s).

               [n,c1] = size(spkfnm); char = class(spkfnm)

                 or

               [1,n] = size(spkfnm); cell = class(spkfnm)

      idcode   the integer ID code of an object for which ephemeris data are
               expected to exist in the specified SPK file.

               [1,1] = size(idcode); int32 = class(idcode)

      room     a parameter specifying the maximum number of intervals that
               can be accommodated by the dynamically allocated workspace
               window used internally by this routine.

               [1,1] = size(room); int32 = class(room)

               It's not necessary to compute an accurate estimate of how
               many intervals will be returned in `cover'; rather, the
               user can pick a size considerably larger than what's
               really required.

      cover_i  an optional input describing a either an empty window or a
               window array created from a previous cspice_spkcov call.

               [2m,1] = size(cover_i), double = class(cover_i)

                  or

               [0,0] = size(cover_i), double = class(cover_i)

               Inclusion of this window argument results in an output window
               consisting of a union of the data retrieved from the `spkfnm'
               kernels and the data in `cover_i'.

   the call:

      [cover] = cspice_spkcov( spkfnm, idcode, room, cover_i )

         or

      [cover] = cspice_spkcov( spkfnm, idcode, room )

   returns:

      cover    the window containing the coverage for `idcode', i.e.
               the set of time intervals for which `idcode'
               data exist in the file `spkfnm'.

               [2p,1] = size(cover), double = class(cover)

                  or

               [0,1] = size(cover), double = class(cover)

               The array `cover' contains the pairs of endpoints of these
               intervals.

               Each window defined as a pair of endpoints such that:

                  window 1 = cover(1:2)
                  window 2 = cover(3:4)
                  window 3 = cover(5:6)
                           ...
                  window p = cover(2p-1,2p)

               The interval endpoints contained in `cover' are ephemeris
               times, expressed as seconds past J2000 TDB.

               `cover' returns an empty set if `spkfnm' lacks coverage for
               `idcode'. If `cover_i' exists in the argument list, `cover'
               returns as a union of the coverage data found in 'spkfnm' and
               the data in `cover_i'. `cover' can overwrite `cover_i'.

Parameters


   None.

Examples


   Any numerical results shown for these examples may differ between
   platforms as the results depend on the SPICE kernels used as input
   and the machine specific arithmetic implementation.

   1) Use a simple function to display the SPK IDs found in an SPK or set of
      SPKs, and the time coverage of the data corresponding to those IDs.

      This example calls both cspice_spkobj and cspice_spkcov. In practice,
      algorithms using cspice_spkobj will also use cspice_spkcov and
      vice-versa.

      Use the LSK kernel below to load the leap seconds and time
      constants required for the time conversions.

         naif0012.tls


      Example code begins here.


      function spkcov_ex1( SPK )

         MAXIV  = 1000;
         WINSIZ = 2 * MAXIV;
         LSK    = 'naif0012.tls';

         %
         % Note, neither cspice_spkcov or cspice_spkobj requires this
         % kernel to function. We need the data for output time
         % conversion.
         %
         cspice_furnsh( LSK )

         %
         % Find the set of objects in the SPK file.
         %
         ids = cspice_spkobj( SPK, MAXIV );

         %
         % We want to display the coverage for each object. Loop over
         % the contents of the ID code set, find the coverage for
         % each item in the set, and display the coverage.
         %
         for i=1:numel(ids)

            %
            % Extract the coverage data for object 'ids(i)'.
            %
            cover     = cspice_spkcov( SPK, ids(i), WINSIZ );
            [row,col] = size(cover);

            %
            % Display a simple banner.
            %
            fprintf( '========================================\n')
            fprintf( 'Coverage for object %d\n', ids(i) )

            %
            %  'cover' has dimension 2Nx1, where 'row' has the value 2N with
            %  each window defined as a pair of endpoints such that:
            %
            %  window 1 = cover(1:2)
            %  window 2 = cover(3:4)
            %  window 3 = cover(5:6)
            %        ...
            %  window N = cover(2N-1,2N)
            %
            % Loop from 1 to 'row' with step size 2.
            %
            for j=1:2:row

               %
               % Convert the endpoints to TDB calendar format time strings
               % and display them. Pass the endpoints in an array,
               % so cspice_timout returns an array of time strings.
               %
               % Recall a vectorized input has dimension 1xM so transpose
               % the 'cover' slice.
               %
               timstr = cspice_timout( cover(j:j+1)', ...
                                   'YYYY MON DD HR:MN:SC.### (TDB) ::TDB' );
               fprintf('Interval: %d\n'  , (j+1)/2 )
               fprintf('   Start: %s\n'  , timstr(1,:) )
               fprintf('    Stop: %s\n\n', timstr(2,:) )

            end

         end

         %
         % Empty the kernel pool.
         %
         cspice_kclear


      When this program was executed on a Mac/Intel/Octave6.x/64-bit
      platform, with the following variable as input

         SPK = { 'sat393.bsp', 'ura112.bsp' };

      the output was:


      ========================================
      Coverage for object 3
      Interval: 1
         Start: 1900 JAN 01 00:00:41.183 (TDB)
          Stop: 2099 DEC 24 00:01:07.183 (TDB)

      ========================================
      Coverage for object 6
      Interval: 1
         Start: 1950 JAN 01 00:00:41.183 (TDB)
          Stop: 2050 JAN 01 00:01:08.183 (TDB)

      ========================================
      Coverage for object 7
      Interval: 1
         Start: 1900 JAN 01 00:00:41.183 (TDB)
          Stop: 2099 DEC 24 00:01:07.183 (TDB)

      ========================================
      Coverage for object 10
      Interval: 1
         Start: 1900 JAN 01 00:00:41.183 (TDB)
          Stop: 2099 DEC 24 00:01:07.183 (TDB)

      ========================================
      Coverage for object 399
      Interval: 1
         Start: 1900 JAN 01 00:00:41.183 (TDB)
          Stop: 2099 DEC 24 00:01:07.183 (TDB)

      ========================================
      Coverage for object 610
      Interval: 1
         Start: 1950 JAN 01 00:00:41.183 (TDB)
          Stop: 2050 JAN 01 00:01:08.183 (TDB)

      ========================================
      Coverage for object 611
      Interval: 1
         Start: 1950 JAN 01 00:00:41.183 (TDB)
          Stop: 2050 JAN 01 00:01:08.183 (TDB)

      ========================================
      Coverage for object 612
      Interval: 1
         Start: 1950 JAN 01 00:00:41.183 (TDB)
          Stop: 2050 JAN 01 00:01:08.183 (TDB)

      ========================================
      Coverage for object 613
      Interval: 1
         Start: 1950 JAN 01 00:00:41.183 (TDB)
          Stop: 2050 JAN 01 00:01:08.183 (TDB)

      ========================================
      Coverage for object 614
      Interval: 1
         Start: 1950 JAN 01 00:00:41.183 (TDB)
          Stop: 2050 JAN 01 00:01:08.183 (TDB)

      ========================================
      Coverage for object 615
      Interval: 1
         Start: 1950 JAN 01 00:00:41.183 (TDB)
          Stop: 2050 JAN 01 00:01:08.183 (TDB)

      ========================================
      Coverage for object 616
      Interval: 1
         Start: 1950 JAN 01 00:00:41.183 (TDB)
          Stop: 2050 JAN 01 00:01:08.183 (TDB)

      ========================================
      Coverage for object 617
      Interval: 1
         Start: 1950 JAN 01 00:00:41.183 (TDB)
          Stop: 2050 JAN 01 00:01:08.183 (TDB)

      ========================================
      Coverage for object 632
      Interval: 1
         Start: 1950 JAN 01 00:00:41.183 (TDB)
          Stop: 2050 JAN 01 00:01:08.183 (TDB)

      ========================================
      Coverage for object 633
      Interval: 1
         Start: 1950 JAN 01 00:00:41.183 (TDB)
          Stop: 2050 JAN 01 00:01:08.183 (TDB)

      ========================================
      Coverage for object 634
      Interval: 1
         Start: 1950 JAN 01 00:00:41.183 (TDB)
          Stop: 2050 JAN 01 00:01:08.183 (TDB)

      ========================================
      Coverage for object 649
      Interval: 1
         Start: 1950 JAN 01 00:00:41.183 (TDB)

      [...]


      Warning: incomplete output. Only 100 out of 174 lines have been
      provided.


   2) When Example #1 was executed on a Mac/Intel/Octave6.x/64-bit
      platform, with the following variable as input

         SPK = { 'mgs_ext12_ipng_mgs95j.bsp', 'mgs_ext26_ipng_mgs95j.bsp' };

      the output was:


      ========================================
      Coverage for object -94
      Interval: 1
         Start: 2003 JUL 23 00:00:00.000 (TDB)
          Stop: 2003 OCT 15 01:00:00.000 (TDB)

      Interval: 2
         Start: 2006 OCT 11 00:00:00.000 (TDB)
          Stop: 2006 NOV 08 01:00:00.000 (TDB)


Particulars


   This routine provides an API via which applications can determine
   the coverage a specified SPK file provides for a specified
   ephemeris object.

Exceptions


   1)  If the input file has transfer format, the error
       SPICE(INVALIDFORMAT) is signaled by a routine in the call tree
       of this routine.

   2)  If the input file is not a transfer file but has architecture
       other than DAF, the error SPICE(INVALIDARCHTYPE) is signaled
       by a routine in the call tree of this routine.

   3)  If the input file is a binary DAF file of type other than SPK,
       the error SPICE(INVALIDFILETYPE) is signaled by a routine in
       the call tree of this routine.

   4)  If the SPK file cannot be opened or read, an error is signaled
       by a routine in the call tree of this routine. The output
       window will not be modified.

   5)  If the size of the output window argument `cover' is
       insufficient to contain the actual number of intervals in the
       coverage window for `idcode', an error is signaled by a
       routine in the call tree of this routine.

   6)  If any of the input arguments, `spkfnm', `idcode', `room' or
       `cover_i', is undefined, an error is signaled by the Matlab
       error handling system.

   7)  If any of the input arguments, `spkfnm', `idcode', `room' or
       `cover_i', is not of the expected type, or it does not have
       the expected dimensions and size, an error is signaled by the
       Mice interface.

Files


   This routine reads an SPK file.

Restrictions


   1)  If an error occurs while this routine is updating the window
       `cover_f', the window may be corrupted.

Required_Reading


   DAF.REQ
   MICE.REQ
   SPK.REQ
   TIME.REQ
   WINDOWS.REQ

Literature_References


   None.

Author_and_Institution


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

Version


   -Mice Version 1.3.0, 26-NOV-2021 (EDW) (JDR)

       Changed the argument names "spk" and "size" to "spkfnm" and "room",
       for consistency with other routines.

       Edited the header to comply with NAIF standard. Extended
       -Index_Entries.

       Added -Parameters, -Exceptions, -Files, -Restrictions,
       -Literature_References and -Author_and_Institution sections.

       Eliminated use of "lasterror" in rethrow.

       Removed reference to the function's corresponding CSPICE header from
       -Required_Reading section.

       Updated description of argument "room".

   -Mice Version 1.2.1, 10-MAR-2015 (EDW)

      Edited -I/O section to conform to NAIF standard for Mice documentation.

   -Mice Version 1.2.0, 03-APR-2012 (EDW)

      Edits to Example code and comments. No change to Example code
      functionality.

      Renamed the argument 'size' to 'room'. "size" is a Matlab function name
      and it's seriously dumb to use a function name word as an argument
      name.

      Edited -I/O section to conform to NAIF standard for Mice documentation.

   -Mice Version 1.1.0, 29-DEC-2008 (EDW)

      Edited description of 'size'; 'size' now defines the maximum
      number of intervals for the internal workspace window.

      The 'cover_i' argument may now have the empty array value, [],
      on input.

      Added range restriction on size.

      Corrected several typos.

   -Mice Version 1.0.0, 18-JUN-2007 (EDW)

Index_Entries


   get coverage window for spk_object
   get coverage start and stop time for spk_object
   get coverage start and stop time for ephemeris_object
   get coverage start and stop time for body


Fri Dec 31 18:44:26 2021