| vprjp |
|
Table of contents
Procedure
VPRJP ( Vector projection onto plane )
SUBROUTINE VPRJP ( VIN, PLANE, VOUT )
Abstract
Project a vector onto a specified plane, orthogonally.
Required_Reading
PLANES
Keywords
GEOMETRY
MATH
PLANE
VECTOR
Declarations
IMPLICIT NONE
INTEGER UBPL
PARAMETER ( UBPL = 4 )
DOUBLE PRECISION VIN ( 3 )
DOUBLE PRECISION PLANE ( UBPL )
DOUBLE PRECISION VOUT ( 3 )
Brief_I/O
VARIABLE I/O DESCRIPTION
-------- --- --------------------------------------------------
VIN I Vector to be projected.
PLANE I A SPICE plane onto which VIN is projected.
VOUT O Vector resulting from projection.
UBPL P SPICE plane upper bound.
Detailed_Input
VIN is a 3-vector that is to be orthogonally projected
onto a specified plane.
PLANE is a SPICE plane that represents the geometric
plane onto which VIN is to be projected.
The normal vector component of a SPICE plane has
unit length.
Detailed_Output
VOUT is the vector resulting from the orthogonal
projection of VIN onto PLANE. VOUT is the closest
point in the specified plane to VIN.
Parameters
UBPL is the upper bound of a SPICE plane array.
Exceptions
1) If the normal vector of the input plane does not have unit
length (allowing for round-off error), the error
SPICE(NONUNITNORMAL) is signaled.
Files
None.
Particulars
Projecting a vector VIN orthogonally onto a plane can be thought
of as finding the closest vector in the plane to VIN. This
"closest vector" always exists; it may be coincident with the
original vector.
Two related routines are VPRJPI, which inverts an orthogonal
projection of a vector onto a plane, and VPROJ, which projects
a vector orthogonally onto another vector.
Examples
The numerical results shown for this example 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) Find the closest point in the ring plane of a planet to a
spacecraft located at a point (in body-fixed coordinates).
Example code begins here.
PROGRAM VPRJP_EX1
IMPLICIT NONE
C
C Local parameters.
C
C Upper bound of plane length.
C
INTEGER UBPL
PARAMETER ( UBPL = 4 )
C
C Local variables.
C
DOUBLE PRECISION NORM ( 3 )
DOUBLE PRECISION ORIG ( 3 )
DOUBLE PRECISION PROJ ( 3 )
DOUBLE PRECISION RINGPL ( UBPL )
DOUBLE PRECISION SCPOS ( 3 )
C
C Set the spacecraft location and define the normal
C vector as the normal to the equatorial plane, and
C the origin at the body/ring center.
C
DATA SCPOS / -29703.16955D0,
. 879765.72163D0,
. -137280.21757D0 /
DATA NORM / 0.D0, 0.D0, 1.D0 /
DATA ORIG / 0.D0, 0.D0, 0.D0 /
C
C Create the plane structure.
C
CALL NVP2PL ( NORM, ORIG, RINGPL )
C
C Project the position vector onto the ring plane.
C
CALL VPRJP ( SCPOS, RINGPL, PROJ )
WRITE(*,'(A)') 'Projection of S/C position onto ring '
. // 'plane:'
WRITE(*,'(3F17.5)') PROJ
END
When this program was executed on a Mac/Intel/gfortran/64-bit
platform, the output was:
Projection of S/C position onto ring plane:
-29703.16955 879765.72163 0.00000
Restrictions
1) It is recommended that the input plane be created by one of
the SPICELIB routines
NVC2PL ( Normal vector and constant to plane )
NVP2PL ( Normal vector and point to plane )
PSV2PL ( Point and spanning vectors to plane )
In any case the input plane must have a unit length normal
vector and a plane constant consistent with the normal
vector.
Literature_References
[1] G. Thomas and R. Finney, "Calculus and Analytic Geometry,"
7th Edition, Addison Wesley, 1988.
Author_and_Institution
N.J. Bachman (JPL)
J. Diaz del Rio (ODC Space)
W.L. Taber (JPL)
Version
SPICELIB Version 1.1.0, 24-AUG-2021 (NJB) (JDR)
Added error check for non-unit plane normal vector.
Changed check-in style to discovery.
Added IMPLICIT NONE statement.
Edited the header to comply with NAIF standard. Added complete
code example. Added documentation of the parameter UBPL.
SPICELIB Version 1.0.1, 10-MAR-1992 (WLT)
Comment section for permuted index source lines was added
following the header.
SPICELIB Version 1.0.0, 01-NOV-1990 (NJB)
|
Fri Dec 31 18:37:06 2021