/* plnsns.f -- translated by f2c (version 19980913).
   You must link the resulting object file with the libraries:
	-lf2c -lm   (in that order)
*/

#include "f2c.h"

/* Table of constant values */

static integer c__2 = 2;
static integer c__1 = 1;

/* $Procedure      PLNSNS ( Planetographic Longitude Sense ) */
integer plnsns_(integer *bodid)
{
    /* System generated locals */
    integer ret_val;

    /* Builtin functions */
    /* Subroutine */ int s_copy(char *, char *, ftnlen, ftnlen);

    /* Local variables */
    doublereal rate;
    char item[32], type__[1];
    integer n;
    logical found;
    integer value;
    extern /* Subroutine */ int repmi_(char *, char *, integer *, char *, 
	    ftnlen, ftnlen, ftnlen), gdpool_(char *, integer *, integer *, 
	    integer *, doublereal *, logical *, ftnlen), dtpool_(char *, 
	    logical *, integer *, char *, ftnlen, ftnlen);

/* $ Abstract */

/*    This function returns the quotient of the planetographic */
/*    and planetocentric longitude for a user specified body. */

/* $ Disclaimer */

/*     THIS SOFTWARE AND ANY RELATED MATERIALS WERE CREATED BY THE */
/*     CALIFORNIA INSTITUTE OF TECHNOLOGY (CALTECH) UNDER A U.S. */
/*     GOVERNMENT CONTRACT WITH THE NATIONAL AERONAUTICS AND SPACE */
/*     ADMINISTRATION (NASA). THE SOFTWARE IS TECHNOLOGY AND SOFTWARE */
/*     PUBLICLY AVAILABLE UNDER U.S. EXPORT LAWS AND IS PROVIDED "AS-IS" */
/*     TO THE RECIPIENT WITHOUT WARRANTY OF ANY KIND, INCLUDING ANY */
/*     WARRANTIES OF PERFORMANCE OR MERCHANTABILITY OR FITNESS FOR A */
/*     PARTICULAR USE OR PURPOSE (AS SET FORTH IN UNITED STATES UCC */
/*     SECTIONS 2312-2313) OR FOR ANY PURPOSE WHATSOEVER, FOR THE */
/*     SOFTWARE AND RELATED MATERIALS, HOWEVER USED. */

/*     IN NO EVENT SHALL CALTECH, ITS JET PROPULSION LABORATORY, OR NASA */
/*     BE LIABLE FOR ANY DAMAGES AND/OR COSTS, INCLUDING, BUT NOT */
/*     LIMITED TO, INCIDENTAL OR CONSEQUENTIAL DAMAGES OF ANY KIND, */
/*     INCLUDING ECONOMIC DAMAGE OR INJURY TO PROPERTY AND LOST PROFITS, */
/*     REGARDLESS OF WHETHER CALTECH, JPL, OR NASA BE ADVISED, HAVE */
/*     REASON TO KNOW, OR, IN FACT, SHALL KNOW OF THE POSSIBILITY. */

/*     RECIPIENT BEARS ALL RISK RELATING TO QUALITY AND PERFORMANCE OF */
/*     THE SOFTWARE AND ANY RELATED MATERIALS, AND AGREES TO INDEMNIFY */
/*     CALTECH AND NASA FOR ALL THIRD-PARTY CLAIMS RESULTING FROM THE */
/*     ACTIONS OF RECIPIENT IN THE USE OF THE SOFTWARE. */

/* $ Required_Reading */

/*     None. */

/* $ Keywords */

/*     PCK */

/* $ Declarations */
/* $ Brief_I/O */

/*     VARIABLE  I/O  DESCRIPTION */
/*     --------  ---  -------------------------------------------------- */
/*     BODID      I   is the NAIF id-code of some solar system object. */

/*     Function returns planetographic/planetocentric */

/* $ Detailed_Input */

/*     BODID      is the NAIF id-code of some planet, asteroid, comet */
/*                or natural satellite of a planet. */

/* $ Detailed_Output */

/*     Based upon loaded PCK values in the kernel pool, the function */
/*     returns the quotient */

/*           planetographic longitude */
/*           ------------------------ */
/*           planetocentric longitude */

/*     for the body specified by BODID.  I.e.  1 if planetographic */
/*     and planetocentric longitude are the same for the input body, */
/*     -1 if the planetographic and planetocentric longitude are */
/*     opposite for the specified body.  If PCK information for */
/*     the specified body can not be located in the kernel pool */
/*     the function returns the value 0. */

/* $ Parameters */

/*     None. */

/* $ Exceptions */

/*     Error free. */

/*     1) If sufficient orientation information for the object */
/*     specified by BODID is not available in the kernel pool, */
/*     the function returns the value 0. */

/* $ Files */

/*     A text PCK kernel must be loaded via the routine FURNSH */
/*     that contains the orientation information for the body specified */
/*     by BODID. */

/* $ Particulars */

/*     This routine returns the multiplicative factor needed */
/*     to convert planetographic longitude to planetocentric */
/*     longitude. */

/*     This routine relies on the proper orientation for the */
/*     specified body having been loaded in the kernel pool. */

/* $ Examples */

/*     Suppose that you have the planetographic coordinates */
/*     of some point on the surface of an object and that you */
/*     need to convert these coordinates to bodyfixed rectangular */
/*     coordinates.  This conversion requires knowledge of the */
/*     sense of planetographic longitude.  The code fragment below */
/*     shows how you go about using this routine to perform the */
/*     conversion. */

/*     We assume that the variables LAT, LONG, HEIGHT contain the */
/*     planetographic latitude, longitude and height above the */
/*     reference surface of some point.  Moreover, let F be the */
/*     flattening factor for the reference spheroid. */

/*     ( F = (Equatorial Radius - Polar Radius ) / Equatorial Radius ) */

/*     Finally, let EQRAD be the equatorial radius. */

/*     We first need to convert planetographic longitude to */
/*     planetocentric longitude. */

/*        FACTOR = PLNSNS(BODID) */

/*        IF ( FACTOR .EQ. 0 ) THEN */

/*           WRITE (*,*) 'Sorry, we don''t have data available.' */
/*           STOP */

/*        END IF */

/*     Compute the planetocentric longitude */

/*        PCLONG = FACTOR * LONG */

/*     Now convert the planetographic coordinates with */
/*     planetographic longitude replaced by planetocentric */
/*     longitude rectangular coordinates.  (Note the conversion */
/*     to planetocentric longitude is required because GEOREC */
/*     assumes that the ordering latitude, longitude, altitude */
/*     is a right handed ordering.  Replacing planetographic */
/*     longitude by planetocentric longitude ensures that we */
/*     have a right handed coordinate system.) */

/*        CALL GEOREC ( LAT, PCLONG, HEIGHT, EQRAD, F, REC ) */



/* $ Restrictions */

/*     None. */

/* $ Literature_References */

/*     None. */

/* $ Author_and_Institution */

/*     W.L. Taber      (JPL) */

/* $ Version */

/* -    SPICELIB Version 1.0.1, 11-MAY-2009 (BVS) */

/*        Replaced LDPOOL with FURNSN in the header. Re-ordered header */
/*        sections. */

/* -    SPICELIB Version 1.0.0, 7-JAN-1997 (WLT) */


/* -& */
/* $ Index_Entries */

/*     Determine the sense of planetographic longitude. */

/* -& */

/*     The earth is a special case so we just handle it here. */

    if (*bodid == 399) {
	ret_val = 1;
	return ret_val;
    }

/*     Create the name of the item to look up in the kernel pool. */

    s_copy(item, "BODY#_PM", (ftnlen)32, (ftnlen)8);
    repmi_(item, "#", bodid, item, (ftnlen)32, (ftnlen)1, (ftnlen)32);

/*     See if this item exists in the kernel pool. */

    dtpool_(item, &found, &n, type__, (ftnlen)32, (ftnlen)1);
    if (! found || *(unsigned char *)type__ != 'N' || n < 2) {
	value = 0;
    } else {
	gdpool_(item, &c__2, &c__1, &n, &rate, &found, (ftnlen)32);

/*        If the rate of change of the prime meridian is negative */
/*        the planetocentric and planetographic longitude are the */
/*        same... */

	if (rate < 0.) {
	    value = 1;
	} else {

/*           ...otherwise they have opposite signs. */

	    value = -1;
	}
    }
    ret_val = value;
    return ret_val;
} /* plnsns_ */

