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| author | Darrell Anderson <darrella@hushmail.com> | 2014-01-21 22:06:48 -0600 |
|---|---|---|
| committer | Timothy Pearson <kb9vqf@pearsoncomputing.net> | 2014-01-21 22:06:48 -0600 |
| commit | 0b8ca6637be94f7814cafa7d01ad4699672ff336 (patch) | |
| tree | d2b55b28893be8b047b4e60514f4a7f0713e0d70 /tde-i18n-en_GB/docs/tdeedu/kstars/meridian.docbook | |
| parent | a1670b07bc16b0decb3e85ee17ae64109cb182c1 (diff) | |
| download | tde-i18n-0b8ca6637be94f7814cafa7d01ad4699672ff336.tar.gz tde-i18n-0b8ca6637be94f7814cafa7d01ad4699672ff336.zip | |
Beautify docbook files
Diffstat (limited to 'tde-i18n-en_GB/docs/tdeedu/kstars/meridian.docbook')
| -rw-r--r-- | tde-i18n-en_GB/docs/tdeedu/kstars/meridian.docbook | 41 |
1 files changed, 5 insertions, 36 deletions
diff --git a/tde-i18n-en_GB/docs/tdeedu/kstars/meridian.docbook b/tde-i18n-en_GB/docs/tdeedu/kstars/meridian.docbook index 067464da584..17284fabcf8 100644 --- a/tde-i18n-en_GB/docs/tdeedu/kstars/meridian.docbook +++ b/tde-i18n-en_GB/docs/tdeedu/kstars/meridian.docbook @@ -1,41 +1,10 @@ <sect1 id="ai-meridian"> <sect1info> -<author -><firstname ->Jason</firstname -> <surname ->Harris</surname -> </author> +<author><firstname>Jason</firstname> <surname>Harris</surname> </author> </sect1info> -<title ->The Local Meridian</title> -<indexterm -><primary ->Local Meridian</primary> -<seealso ->Hour Angle</seealso -> <seealso ->Celestial Sphere</seealso -> </indexterm> -<para ->The Local Meridian is an imaginary <link linkend="ai-greatcircle" ->Great Circle</link -> on the <link linkend="ai-csphere" ->Celestial Sphere</link -> that is perpendicular to the local <link linkend="ai-horizon" ->Horizon</link ->. It passes through the North point on the Horizon, through the <link linkend="ai-cpoles" ->Celestial Pole</link ->, up to the <link linkend="ai-zenith" ->Zenith</link ->, and through the South point on the Horizon. </para -><para ->Because it is fixed to the local Horizon, stars will appear to drift past the Local Meridian as the Earth spins. You can use an object's <link linkend="equatorial" ->Right Ascension</link -> and the <link linkend="ai-sidereal" ->Local Sidereal Time</link -> to determine when it will cross your Local Meridian (see <link linkend="ai-hourangle" ->Hour Angle</link ->). </para> +<title>The Local Meridian</title> +<indexterm><primary>Local Meridian</primary> +<seealso>Hour Angle</seealso> <seealso>Celestial Sphere</seealso> </indexterm> +<para>The Local Meridian is an imaginary <link linkend="ai-greatcircle">Great Circle</link> on the <link linkend="ai-csphere">Celestial Sphere</link> that is perpendicular to the local <link linkend="ai-horizon">Horizon</link>. It passes through the North point on the Horizon, through the <link linkend="ai-cpoles">Celestial Pole</link>, up to the <link linkend="ai-zenith">Zenith</link>, and through the South point on the Horizon. </para><para>Because it is fixed to the local Horizon, stars will appear to drift past the Local Meridian as the Earth spins. You can use an object's <link linkend="equatorial">Right Ascension</link> and the <link linkend="ai-sidereal">Local Sidereal Time</link> to determine when it will cross your Local Meridian (see <link linkend="ai-hourangle">Hour Angle</link>). </para> </sect1> |