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SLA_PREBN - Precession Matrix (FK4)

ACTION:
Generate the matrix of precession between two epochs, using the old, pre IAU 1976, Bessel-Newcomb model, in Andoyer's formulation.
CALL:
CALL sla_PREBN (BEP0, BEP1, RMATP)
GIVEN:

BEP0 D beginning Besselian epoch
BEP1 D ending Besselian epoch
RETURNED:

RMATP D(3,3) precession matrix
NOTE:
The matrix is in the sense:
v$_{1}$ = M$\cdot$v$_{0}$
where v$_{1}$ is the star vector relative to the mean equator and equinox of epoch BEP1, M is the $3\times3$ matrix RMATP and v$_{0}$ is the star vector relative to the mean equator and equinox of epoch BEP0.
REFERENCE:
Smith et al., 1989. Astr.J. 97, 269.


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Next: SLA_PREC - Precession Matrix (FK5)
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Previous: SLA_POLMO - Polar Motion

SLALIB --- Positional Astronomy Library
Starlink User Note 67
P. T. Wallace
19 December 2005
E-mail:ussc@star.rl.ac.uk

Copyright © 2009 Science and Technology Facilities Council