08-07-2007
Only one think I mention is that I used the the rdsk path for the dd command (use a bigger blk size it is mutch faster!!!) and that there was a / failed inside your command (maybe only a typing error)
joerg
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LEARN ABOUT OPENSOLARIS
mlib_volumeraycast_blocked_divergent_trilinear_s16_s16
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:
Printed copy or docs.sun.com displays a 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 |Committed |
+-----------------------------+-----------------------------+
|MT-Level |MT-Safe |
+-----------------------------+-----------------------------+
SEE ALSO
mlib_VolumeRayCast_General(3MLIB), attributes(5)
SunOS 5.11 2 Mar 2007 mlib_VolumeRayCast_Blocked(3MLIB)