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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_ZD - to Zenith Distance</TITLE>
+<META NAME="description" CONTENT="SLA_ZD - to Zenith Distance">
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+<H2><A NAME="SECTION0004183000000000000000">&#160;</A><A NAME="xref_SLA_ZD">&#160;</A><A NAME="SLA_ZD">&#160;</A>
+<BR>
+SLA_ZD - <IMG WIDTH="27" HEIGHT="27" ALIGN="MIDDLE" BORDER="0"
+ SRC="img65.gif"
+ ALT="$h,\delta$"> to Zenith Distance
+</H2>
+ <DL>
+<DT><STRONG>ACTION:</STRONG>
+<DD>Hour angle and declination to zenith distance
+(double precision).
+<P> <DT><STRONG>CALL:</STRONG>
+<DD><TT>D&nbsp;=&nbsp;sla_ZD (HA, DEC, PHI)</TT>
+<P> </DL>
+<P> <DL>
+<DT><STRONG>GIVEN:</STRONG>
+<DD>
+<BR>
+<TABLE CELLPADDING=3>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>HA</EM></TD>
+<TH ALIGN="LEFT"><B>D</B></TH>
+<TD ALIGN="LEFT" NOWRAP>hour angle in radians</TD>
+</TR>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>DEC</EM></TD>
+<TD ALIGN="LEFT"><B>D</B></TD>
+<TD ALIGN="LEFT" NOWRAP>declination in radians</TD>
+</TR>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>PHI</EM></TD>
+<TD ALIGN="LEFT"><B>D</B></TD>
+<TD ALIGN="LEFT" NOWRAP>latitude in radians</TD>
+</TR>
+</TABLE></DL>
+<P> <DL>
+<DT><STRONG>RETURNED:</STRONG>
+<DD>
+<BR>
+<TABLE CELLPADDING=3>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>sla_ZD</EM></TD>
+<TH ALIGN="LEFT"><B>D</B></TH>
+<TD ALIGN="LEFT" NOWRAP>zenith distance (radians, <IMG WIDTH="35" HEIGHT="25" ALIGN="MIDDLE" BORDER="0"
+ SRC="img234.gif"
+ ALT="$0\!-\!\pi$">)</TD>
+</TR>
+</TABLE></DL>
+<P> <DL>
+<DT><STRONG>NOTES:</STRONG>
+<DD><DL COMPACT>
+<DT>1.
+<DD>The latitude must be geodetic. In critical applications,
+corrections for polar motion should be applied (see sla_POLMO).
+<DT>2.
+<DD>In some applications it will be important to specify the
+ correct type of hour angle and declination in order to
+ produce the required type
+ of zenith distance. In particular, it may be
+ important to distinguish between the zenith distance
+ as affected by refraction, which would require the
+ <I>observed</I> <IMG WIDTH="41" HEIGHT="29" ALIGN="MIDDLE" BORDER="0"
+ SRC="img29.gif"
+ ALT="$[\,h,\delta\,]$">, and the zenith distance <I>in vacuo</I>,
+ which would require the <I>topocentric</I> <IMG WIDTH="41" HEIGHT="29" ALIGN="MIDDLE" BORDER="0"
+ SRC="img29.gif"
+ ALT="$[\,h,\delta\,]$">. If
+ the effects of diurnal aberration can be neglected, the
+ <I>apparent</I> <IMG WIDTH="41" HEIGHT="29" ALIGN="MIDDLE" BORDER="0"
+ SRC="img29.gif"
+ ALT="$[\,h,\delta\,]$"> may be used instead of the
+ <I>topocentric</I> <IMG WIDTH="41" HEIGHT="29" ALIGN="MIDDLE" BORDER="0"
+ SRC="img29.gif"
+ ALT="$[\,h,\delta\,]$">. <DT>3.
+<DD>No range checking of arguments is done.
+ <DT>4.
+<DD>In applications which involve many zenith distance calculations,
+ rather than calling the present routine it will be more
+ efficient to use inline code, having previously computed fixed
+ terms such as sine and cosine of latitude, and perhaps sine and
+ cosine of declination.
+ </DL></DL>
+<P>
+<BR>
+<P>
+<BR> <HR>
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+ SRC="contents_motif.gif"></A>
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+<BR>
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+<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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