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authorJoseph Hunkeler <jhunkeler@gmail.com>2015-03-04 21:21:30 -0500
committerJoseph Hunkeler <jhunkeler@gmail.com>2015-03-04 21:21:30 -0500
commitd54fe7c1f704a63824c5bfa0ece65245572e9b27 (patch)
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+<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 3.2//EN">
+<!--Converted with LaTeX2HTML 97.1 (release) (July 13th, 1997)
+ by Nikos Drakos (nikos@cbl.leeds.ac.uk), CBLU, University of Leeds
+* revised and updated by: Marcus Hennecke, Ross Moore, Herb Swan
+* with significant contributions from:
+ Jens Lippman, Marek Rouchal, Martin Wilck and others -->
+<HTML>
+<HEAD>
+<TITLE>Efficiency considerations</TITLE>
+<META NAME="description" CONTENT="Efficiency considerations">
+<META NAME="keywords" CONTENT="sun67">
+<META NAME="resource-type" CONTENT="document">
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+ SRC="contents_motif.gif"></A>
+<BR>
+<B> Next:</B> <A NAME="tex2html2602" HREF="node216.html">The Hipparcos Catalogue and the ICRS</A>
+<BR>
+<B>Up:</B> <A NAME="tex2html2600" HREF="node213.html">Apparent Place to Observed Place</A>
+<BR>
+<B> Previous:</B> <A NAME="tex2html2596" HREF="node214.html">Refraction</A>
+<BR> <HR> <P>
+<P><!--End of Navigation Panel-->
+<H3><A NAME="SECTION000513200000000000000">
+Efficiency considerations</A>
+</H3>
+The complete apparent place to observed place transformation
+can be carried out by calling
+sla_AOP.
+For improved efficiency
+in cases of more than one star or a sequence of times, the
+target-independent calculations can be done once by
+calling
+sla_AOPPA,
+the time can be updated by calling
+sla_AOPPAT,
+and
+sla_AOPQK
+can then be used to perform the
+apparent-to-observed transformation. The reverse transformation
+is available through
+sla_OAP
+and
+sla_OAPQK.
+(<I>n.b.</I> These routines use accurate but computationally-expensive
+refraction algorithms for zenith distances beyond about <IMG WIDTH="26" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
+ SRC="img33.gif"
+ ALT="$76^\circ$">.For many purposes, in-line code tailored to the accuracy requirements
+of the application will be preferable, for example ignoring UT1-UTC,
+omitting diurnal aberration and using
+sla_REFZ
+to apply the refraction.)
+<P>
+<BR> <HR>
+<A NAME="tex2html2601" HREF="node216.html">
+<IMG WIDTH="37" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="next" SRC="next_motif.gif"></A>
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+<IMG WIDTH="26" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="up" SRC="up_motif.gif"></A>
+<A NAME="tex2html2595" HREF="node214.html">
+<IMG WIDTH="63" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="previous" SRC="previous_motif.gif"></A> <A HREF="sun67.html#stardoccontents"><IMG ALIGN="BOTTOM" BORDER="0"
+ SRC="contents_motif.gif"></A>
+<BR>
+<B> Next:</B> <A NAME="tex2html2602" HREF="node216.html">The Hipparcos Catalogue and the ICRS</A>
+<BR>
+<B>Up:</B> <A NAME="tex2html2600" HREF="node213.html">Apparent Place to Observed Place</A>
+<BR>
+<B> Previous:</B> <A NAME="tex2html2596" HREF="node214.html">Refraction</A>
+<BR> <HR> <P>
+<P><!--End of Navigation Panel-->
+<ADDRESS>
+<I>SLALIB --- Positional Astronomy Library<BR>Starlink User Note 67<BR>P. T. Wallace<BR>12 October 1999<BR>E-mail:ptw@star.rl.ac.uk</I>
+</ADDRESS>
+</BODY>
+</HTML>