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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
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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>SLA_XY2XY - Apply Linear Model to an </TITLE>
+<META NAME="description" CONTENT="SLA_XY2XY - Apply Linear Model to an ">
+<META NAME="keywords" CONTENT="sun67">
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+ SRC="contents_motif.gif"></A>
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+<B> Next:</B> <A NAME="tex2html2377" HREF="node196.html">SLA_ZD - to Zenith Distance</A>
+<BR>
+<B>Up:</B> <A NAME="tex2html2375" HREF="node13.html">SUBPROGRAM SPECIFICATIONS</A>
+<BR>
+<B> Previous:</B> <A NAME="tex2html2369" HREF="node194.html">SLA_WAIT - Time Delay</A>
+<BR> <HR> <P>
+<P><!--End of Navigation Panel-->
+<H2><A NAME="SECTION0004182000000000000000">&#160;</A><A NAME="xref_SLA_XY2XY">&#160;</A><A NAME="SLA_XY2XY">&#160;</A>
+<BR>
+SLA_XY2XY - Apply Linear Model to an <IMG WIDTH="42" HEIGHT="29" ALIGN="MIDDLE" BORDER="0"
+ SRC="img20.gif"
+ ALT="$[\,x,y\,]$"></H2>
+ <DL>
+<DT><STRONG>ACTION:</STRONG>
+<DD>Transform one <IMG WIDTH="42" HEIGHT="29" ALIGN="MIDDLE" BORDER="0"
+ SRC="img20.gif"
+ ALT="$[\,x,y\,]$"> into another using a linear model of the type
+produced by the sla_FITXY routine.
+<P> <DT><STRONG>CALL:</STRONG>
+<DD><TT>CALL sla_XY2XY (X1,Y1,COEFFS,X2,Y2)</TT>
+<P> </DL>
+<P> <DL>
+<DT><STRONG>GIVEN:</STRONG>
+<DD>
+<BR>
+<TABLE CELLPADDING=3>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>X1,Y1</EM></TD>
+<TH ALIGN="LEFT"><B>D</B></TH>
+<TD ALIGN="LEFT" NOWRAP><IMG WIDTH="42" HEIGHT="29" ALIGN="MIDDLE" BORDER="0"
+ SRC="img20.gif"
+ ALT="$[\,x,y\,]$"> before transformation</TD>
+</TR>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>COEFFS</EM></TD>
+<TD ALIGN="LEFT"><B>D(6)</B></TD>
+<TD ALIGN="LEFT" NOWRAP>transformation coefficients (see note)</TD>
+</TR>
+</TABLE></DL>
+<P> <DL>
+<DT><STRONG>RETURNED:</STRONG>
+<DD>
+<BR>
+<TABLE CELLPADDING=3>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>X2,Y2</EM></TD>
+<TH ALIGN="LEFT"><B>D</B></TH>
+<TD ALIGN="LEFT" NOWRAP><IMG WIDTH="42" HEIGHT="29" ALIGN="MIDDLE" BORDER="0"
+ SRC="img20.gif"
+ ALT="$[\,x,y\,]$"> after transformation</TD>
+</TR>
+</TABLE></DL>
+<P> <DL>
+<DT><STRONG>NOTES:</STRONG>
+<DD><DL COMPACT>
+<DT>1.
+<DD>The model relates two sets of <IMG WIDTH="42" HEIGHT="29" ALIGN="MIDDLE" BORDER="0"
+ SRC="img20.gif"
+ ALT="$[\,x,y\,]$"> coordinates as follows.
+Naming the six elements of COEFFS <I>a</I>,<I>b</I>,<I>c</I>,<I>d</I>,<I>e</I> &amp; <I>f</I>,
+the present routine performs the transformation:
+ <BLOCKQUOTE><I>x<SUB>2</SUB></I> = <I>a</I> + <I>bx<SUB>1</SUB></I> + <I>cy<SUB>1</SUB></I> <BR>
+ <I>y<SUB>2</SUB></I> = <I>d</I> + <I>ex<SUB>1</SUB></I> + <I>fy<SUB>1</SUB></I></BLOCKQUOTE>
+ <DT>2.
+<DD>See also sla_FITXY, sla_PXY, sla_INVF, sla_DCMPF.
+ </DL></DL>
+<BR> <HR>
+<A NAME="tex2html2376" HREF="node196.html">
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+<A NAME="tex2html2368" HREF="node194.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="tex2html2377" HREF="node196.html">SLA_ZD - to Zenith Distance</A>
+<BR>
+<B>Up:</B> <A NAME="tex2html2375" HREF="node13.html">SUBPROGRAM SPECIFICATIONS</A>
+<BR>
+<B> Previous:</B> <A NAME="tex2html2369" HREF="node194.html">SLA_WAIT - Time Delay</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>
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+</HTML>