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authorTimothy Pearson <kb9vqf@pearsoncomputing.net>2011-12-03 11:05:10 -0600
committerTimothy Pearson <kb9vqf@pearsoncomputing.net>2011-12-03 11:05:10 -0600
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+<sect1 id="ai-meridian">
+<sect1info>
+<author
+><firstname
+>Jason</firstname
+> <surname
+>Harris</surname
+> </author>
+</sect1info>
+<title
+>Den lokale meridian</title>
+<indexterm
+><primary
+>Den lokale meridian</primary>
+<seealso
+>Timevinkel</seealso
+> <seealso
+>Himmelkuglen (himmelsfæren)</seealso
+> </indexterm>
+<para
+>Den lokale meridian er en tilsyneladende <link linkend="ai-greatcircle"
+>storcirkel </link
+> på <link linkend="ai-csphere"
+>himmelkuglen</link
+> der står vinkelret på <link linkend="ai-horizon"
+>horisonten</link
+>. Meridianen går gennem horisontens nordpunkt, <link linkend="ai-cpoles"
+> himlens poler</link
+>, <link linkend="ai-zenith"
+>zenit</link
+> og horisontens sydpunkt. </para
+><para
+>Fordi meridianen er knyttet til horisonten lige der hvor du ser fra, ser alle stjerner ud til at passerer den lokale meridian, når jorden drejer. Du kan bruge et himmelobjekts <link linkend="equatorial"
+> rektascension</link
+> og den <link linkend="ai-sidereal"
+>lokale sideriske tid</link
+> til at bestemme hvornår det vil passere din lokale meridian. (se <link linkend="ai-hourangle"
+>timevinkel </link
+>). </para>
+</sect1>
+