Next: SLA_BEAR - Direction Between Points on a Sphere
Up: SUBPROGRAM SPECIFICATIONS
Previous: SLA_ATMDSP - Atmospheric Dispersion
SLA_AV2M - Rotation Matrix from Axial Vector
- ACTION:
- Form the rotation matrix corresponding to a given axial vector
(single precision).
- CALL:
- CALL sla_AV2M (AXVEC, RMAT)
- GIVEN:
-
| AXVEC |
R(3) |
axial vector (radians) |
- RETURNED:
-
| RMAT |
R(3,3) |
rotation matrix |
- NOTES:
- A rotation matrix describes a rotation about some
arbitrary axis, called the Euler axis. The
axial vector supplied to this routine
has the same direction as the Euler axis, and its
magnitude is the amount of rotation in radians.
- If AXVEC is null, the unit matrix is returned.
- The reference frame rotates clockwise as seen looking along
the axial vector from the origin.
Next: SLA_BEAR - Direction Between Points on a Sphere
Up: SUBPROGRAM SPECIFICATIONS
Previous: SLA_ATMDSP - Atmospheric Dispersion
SLALIB --- Positional Astronomy Library
Starlink User Note 67
P. T. Wallace
19 December 2005
E-mail:ussc@star.rl.ac.uk
Copyright © 2010 Science and Technology Facilities Council