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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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treeafc52015ffc2c74e0266653eecef1c8ef8ba5d91 /src/slalib/sun67.htx/node16.html
downloadcalfuse-d54fe7c1f704a63824c5bfa0ece65245572e9b27.tar.gz
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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_AIRMAS - Air Mass</TITLE>
+<META NAME="description" CONTENT="SLA_AIRMAS - Air Mass">
+<META NAME="keywords" CONTENT="sun67">
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+<BR>
+<B>Up:</B> <A NAME="tex2html585" HREF="node13.html">SUBPROGRAM SPECIFICATIONS</A>
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+<BR> <HR> <P>
+<P><!--End of Navigation Panel-->
+<H2><A NAME="SECTION00043000000000000000">SLA_AIRMAS - Air Mass</A>
+<A NAME="xref_SLA_AIRMAS">&#160;</A><A NAME="SLA_AIRMAS">&#160;</A>
+</H2>
+ <DL>
+<DT><STRONG>ACTION:</STRONG>
+<DD>Air mass at given zenith distance (double precision).
+<DT><STRONG>CALL:</STRONG>
+<DD><TT>D&nbsp;=&nbsp;sla_AIRMAS (ZD)</TT>
+<P> </DL>
+<P> <DL>
+<DT><STRONG>GIVEN:</STRONG>
+<DD>
+<BR>
+<TABLE CELLPADDING=3>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>ZD</EM></TD>
+<TH ALIGN="LEFT"><B>D</B></TH>
+<TD ALIGN="LEFT" NOWRAP>observed zenith distance (radians)</TD>
+</TR>
+</TABLE></DL>
+<P> <DL>
+<DT><STRONG>RETURNED:</STRONG>
+<DD>
+<BR>
+<TABLE CELLPADDING=3>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>sla_AIRMAS</EM></TD>
+<TH ALIGN="LEFT"><B>D</B></TH>
+<TD ALIGN="LEFT" NOWRAP>air mass (1 at zenith)</TD>
+</TR>
+</TABLE></DL>
+<P> <DL>
+<DT><STRONG>NOTES:</STRONG>
+<DD><DL COMPACT>
+<DT>1.
+<DD>The <I>observed</I> zenith distance referred to above means
+``as affected by refraction''.
+<DT>2.
+<DD>The routine uses Hardie's (1962) polynomial fit to Bemporad's
+ data for the relative air mass, <I>X</I>, in units of thickness at the
+ zenith as tabulated by Schoenberg (1929). This is adequate for all
+ normal needs as it is accurate to better than
+ 0.1% up to <I>X</I> = 6.8 and better than 1% up to <I>X</I> = 10.
+ Bemporad's tabulated values are unlikely to be trustworthy
+ to such accuracy
+ because of variations in density, pressure and other
+ conditions in the atmosphere from those assumed in his work.
+ <DT>3.
+<DD>The sign of the ZD is ignored.
+ <DT>4.
+<DD>At zenith distances greater than about <IMG WIDTH="56" HEIGHT="27" ALIGN="MIDDLE" BORDER="0"
+ SRC="img8.gif"
+ ALT="$\zeta = 87^{\circ}$"> the
+ air mass is held constant to avoid arithmetic overflows.
+ </DL></DL>
+<P> <DL>
+<DT><STRONG>REFERENCES:</STRONG>
+<DD><DL COMPACT>
+<DT>1.
+<DD>Hardie, R.H., 1962, in <I>Astronomical Techniques</I>
+ed. W.A. Hiltner, University of Chicago Press, p180.
+<DT>2.
+<DD>Schoenberg, E., 1929, Hdb. d. Ap.,
+ Berlin, Julius Springer, 2, 268.
+ </DL></DL>
+<BR> <HR>
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+ SRC="contents_motif.gif"></A>
+<BR>
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+<BR>
+<B>Up:</B> <A NAME="tex2html585" HREF="node13.html">SUBPROGRAM SPECIFICATIONS</A>
+<BR>
+<B> Previous:</B> <A NAME="tex2html579" HREF="node15.html">SLA_AFIN - Sexagesimal character string to angle</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>