mlib_VolumeRayCast_Blocked(3MLIB)			    mediaLib Library Functions				 mlib_VolumeRayCast_Blocked(3MLIB)

NAME

       mlib_VolumeRayCast_Blocked,     mlib_VolumeRayCast_Blocked_Parallel_Nearest_U8_U8,     mlib_VolumeRayCast_Blocked_Parallel_Nearest_S16_S16,
       mlib_VolumeRayCast_Blocked_Parallel_Trilinear_U8_U8,	    mlib_VolumeRayCast_Blocked_Parallel_Trilinear_S16_S16,	   mlib_VolumeRay-
       Cast_Blocked_Divergent_Nearest_U8_U8,   mlib_VolumeRayCast_Blocked_Divergent_Nearest_S16_S16,  mlib_VolumeRayCast_Blocked_Divergent_Trilin-
       ear_U8_U8, mlib_VolumeRayCast_Blocked_Divergent_Trilinear_S16_S16 - cast a ray (or rays) through a 3D data set

SYNOPSIS

       cc [ flag... ] file... -lmlib [ library... ]
       #include <mlib.h>

       mlib_status mlib_VolumeRayCast_Blocked_Parallel_Nearest_U8_U8(mlib_rays *rays, const mlib_blkvolume *blk, void *buffer);

       mlib_status mlib_VolumeRayCast_Blocked_Parallel_Nearest_S16_S16(mlib_rays *rays, const mlib_blkvolume *blk, void *buffer);

       mlib_status mlib_VolumeRayCast_Blocked_Parallel_Trilinear_U8_U8(mlib_rays *rays, const mlib_blkvolume *blk, void *buffer);

       mlib_status mlib_VolumeRayCast_Blocked_Parallel_Trilinear_S16_S16(mlib_rays *rays, const mlib_blkvolume *blk, void *buffer);

       mlib_status mlib_VolumeRayCast_Blocked_Divergent_Nearest_U8_U8(mlib_rays *rays, const mlib_blkvolume *blk, void *buffer);

       mlib_status mlib_VolumeRayCast_Blocked_Divergent_Nearest_S16_S16(mlib_rays *rays, const mlib_blkvolume *blk, void *buffer);

       mlib_status mlib_VolumeRayCast_Blocked_Divergent_Trilinear_U8_U8(mlib_rays *rays, const mlib_blkvolume *blk, void *buffer);

       mlib_status mlib_VolumeRayCast_Blocked_Divergent_Trilinear_S16_S16(mlib_rays *rays, const mlib_blkvolume *blk, void *buffer);

DESCRIPTION

       Each of these functions casts a ray (or rays) through a three-dimensional(3D) data set, then computes and returns the interpolated samples
       at each step along the way.

       In trilinear interpolation, the value at point P is computed from its eight surrounding neighbors based on the equation below.

       P = (1-a)*(1-b)*(1-c)*P0 +
	   a*(1-b)*(1-c)*Px + (1-a)*b*(1-c)*Py + (1-a)*(1-b)*c*Pz +
	   a*b*(1-c)*Pxy + a*(1-b)*c*Pxz + (1-a)*b*c*Pyz +
	   a*b*c*Pxyz

       where a, b, and c are the fractional parts of the coordinates of point P.

       The trilinear interpolation is represented by the following figure:

	      Please see the online man page on docs.sun.com or a print copy for the diagram.

       Figure that represents the trilinear interpolation

       In nearest neighbor operation, the sample value at point P is replaced by the value of the nearest neighbor voxel.

PARAMETERS

       Each of the functions takes the following arguments:

       rays	       Casting rays.

       blk	       Volume data in the blocked format.

       buffer	       Working buffer.

RETURN VALUES

       Each of the functions returns MLIB_SUCCESS if successful. Otherwise it returns MLIB_FAILURE.

ATTRIBUTES

       See attributes(5) for descriptions of the following attributes:

       +-----------------------------+-----------------------------+
       |      ATTRIBUTE TYPE	     |	    ATTRIBUTE VALUE	   |
       +-----------------------------+-----------------------------+
       |Interface Stability	     |Evolving			   |
       +-----------------------------+-----------------------------+
       |MT-Level		     |MT-Safe			   |
       +-----------------------------+-----------------------------+

SEE ALSO

       mlib_VolumeRayCast_General(3MLIB), attributes(5)

SunOS 5.10							    10 Nov 2004 				 mlib_VolumeRayCast_Blocked(3MLIB)