From d54fe7c1f704a63824c5bfa0ece65245572e9b27 Mon Sep 17 00:00:00 2001 From: Joseph Hunkeler Date: Wed, 4 Mar 2015 21:21:30 -0500 Subject: Initial commit --- src/slalib/sun67.htx/node18.html | 135 +++++++++++++++++++++++++++++++++++++++ 1 file changed, 135 insertions(+) create mode 100644 src/slalib/sun67.htx/node18.html (limited to 'src/slalib/sun67.htx/node18.html') diff --git a/src/slalib/sun67.htx/node18.html b/src/slalib/sun67.htx/node18.html new file mode 100644 index 0000000..e3aee75 --- /dev/null +++ b/src/slalib/sun67.htx/node18.html @@ -0,0 +1,135 @@ + + + + +SLA_AMP - Apparent to Mean + + + + + + + + + + + + +

+ +next + +up + +previous +
+ Next: SLA_AMPQK - Quick Apparent to Mean +
+Up: SUBPROGRAM SPECIFICATIONS +
+ Previous: SLA_ALTAZ - Velocities etc. for Altazimuth Mount +

+

+

SLA_AMP - Apparent to Mean +   +

+
+
ACTION: +
Convert star $[\,\alpha,\delta\,]$ from geocentric apparent to +mean place (post IAU 1976). +

CALL: +
CALL sla_AMP (RA, DA, DATE, EQ, RM, DM) +

+

+
GIVEN: +
+
+ + + + + + + + + + + + + +
RA,DADapparent $[\,\alpha,\delta\,]$ (radians)
DATEDTDB for apparent place (JD-2400000.5)
EQDequinox: Julian epoch of mean place
+

+
RETURNED: +
+
+ + + + + +
RM,DMDmean $[\,\alpha,\delta\,]$ (radians)
+

+
NOTES: +
+
1. +
The distinction between the required TDB and TT is +always negligible. Moreover, for all but the most +critical applications UTC is adequate. +
2. +
The accuracy is limited by the routine sla_EVP, called + by sla_MAPPA, which computes the Earth position and + velocity using the methods of Stumpff. The maximum + error is about 0.3 milliarcsecond. +
3. +
Iterative techniques are used for the aberration and + light deflection corrections so that the routines + sla_AMP (or sla_AMPQK) and sla_MAP (or sla_MAPQK) are + accurate inverses; even at the edge of the Sun's disc + the discrepancy is only about 1 nanoarcsecond. +
4. +
Where multiple apparent places are to be converted to + mean places, for a fixed date and equinox, it is more + efficient to use the sla_MAPPA routine to compute the + required parameters once, followed by one call to + sla_AMPQK per star. +
+

+
REFERENCES: +
+
1. +
1984 Astronomical Almanac, pp B39-B41. +
2. +
Lederle & Schwan, 1984. Astr.Astrophys. 134, 1-6. +
+

+ +next + +up + +previous +
+ Next: SLA_AMPQK - Quick Apparent to Mean +
+Up: SUBPROGRAM SPECIFICATIONS +
+ Previous: SLA_ALTAZ - Velocities etc. for Altazimuth Mount +

+

+

+SLALIB --- Positional Astronomy Library
Starlink User Note 67
P. T. Wallace
12 October 1999
E-mail:ptw@star.rl.ac.uk
+
+ + -- cgit