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<TITLE>palDh2e palDh2e
- Horizon to equatorial coordinates: Az,El to HA,Dec
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- Horizon to equatorial coordinates: Az,El to HA,Dec
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<H2><A NAME="SECTION000312000000000000000"></A><A NAME="____palDh2e_"></A>
<BR>
palDh2e
palDh2e
- Horizon to equatorial coordinates: Az,El to HA,Dec
</H2>
<DL>
<DT><STRONG>Description:</STRONG></DT>
<DD><DL>
<DD>Convert horizon to equatorial coordinates.
</DD>
</DL>
<BR>
</DD>
<DT><STRONG>Invocation:</STRONG></DT>
<DD><DL>
<DD><TT> palDh2e( double az, double el, double phi, double <SPAN CLASS="MATH"><IMG
WIDTH="13" HEIGHT="18" ALIGN="BOTTOM" BORDER="0"
SRC="img1.png"
ALT="$*$"></SPAN> ha, double <SPAN CLASS="MATH"><IMG
WIDTH="13" HEIGHT="18" ALIGN="BOTTOM" BORDER="0"
SRC="img1.png"
ALT="$*$"></SPAN> dec );
</TT>
</DD>
</DL>
<BR>
</DD>
<DT><STRONG>Arguments:</STRONG></DT>
<DD>
<BR> <DL>
<DT><STRONG>
az = double (Given)
</STRONG></DT>
<DD>
Azimuth (radians)
</DD>
<DT><STRONG>
el = double (Given)
</STRONG></DT>
<DD>
Elevation (radians)
</DD>
<DT><STRONG>
phi = double (Given)
</STRONG></DT>
<DD>
Observatory latitude (radians)
</DD>
<DT><STRONG>
ha = double <SPAN CLASS="MATH"><IMG
WIDTH="13" HEIGHT="18" ALIGN="BOTTOM" BORDER="0"
SRC="img1.png"
ALT="$*$"></SPAN> (Returned)
</STRONG></DT>
<DD>
Hour angle (radians)
</DD>
<DT><STRONG>
dec = double <SPAN CLASS="MATH"><IMG
WIDTH="13" HEIGHT="18" ALIGN="BOTTOM" BORDER="0"
SRC="img1.png"
ALT="$*$"></SPAN> (Returned)
</STRONG></DT>
<DD>
Declination (radians)
</DD>
</DL>
<BR>
</DD>
<DT><STRONG>Notes:</STRONG></DT>
<DD><UL>
<LI>All the arguments are angles in radians.
<P>
</LI>
<LI>The sign convention for azimuth is north zero, east <SPAN CLASS="MATH"><IMG
WIDTH="18" HEIGHT="31" ALIGN="MIDDLE" BORDER="0"
SRC="img2.png"
ALT="$+$"></SPAN>pi/2.
<P>
</LI>
<LI>HA is returned in the range <SPAN CLASS="MATH"><IMG
WIDTH="18" HEIGHT="31" ALIGN="MIDDLE" BORDER="0"
SRC="img2.png"
ALT="$+$"></SPAN>/-pi. Declination is returned
in the range <SPAN CLASS="MATH"><IMG
WIDTH="18" HEIGHT="31" ALIGN="MIDDLE" BORDER="0"
SRC="img2.png"
ALT="$+$"></SPAN>/-pi/2.
<P>
</LI>
<LI>The latitude is (in principle) geodetic. In critical
applications, corrections for polar motion should be applied.
<P>
</LI>
<LI>In some applications it will be important to specify the
correct type of elevation in order to produce the required
type of HA,Dec. In particular, it may be important to
distinguish between the elevation as affected by refraction,
which will yield the <TT>"</TT>observed<TT>"</TT> HA,Dec, and the elevation
in vacuo, which will yield the <TT>"</TT>topocentric<TT>"</TT> HA,Dec. If the
effects of diurnal aberration can be neglected, the
topocentric HA,Dec may be used as an approximation to the
<TT>"</TT>apparent<TT>"</TT> HA,Dec.
<P>
</LI>
<LI>No range checking of arguments is done.
<P>
</LI>
<LI>In applications which involve many such 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.
</LI>
</UL>
<BR>
</DD>
</DL>
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