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	<title>Combs method - Revision history</title>
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	<updated>2026-06-06T19:58:37Z</updated>
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		<title>en&gt;Melcombe: remove cat, no &quot;probability interpretation&quot; here</title>
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		<updated>2010-12-23T16:19:23Z</updated>

		<summary type="html">&lt;p&gt;remove cat, no &amp;quot;probability interpretation&amp;quot; here&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;The &amp;#039;&amp;#039;&amp;#039;solar zenith angle&amp;#039;&amp;#039;&amp;#039; is the angle measured from directly overhead to the geometric centre of the sun&amp;#039;s disc, as described using a [[horizontal coordinate system]]. The &amp;#039;&amp;#039;&amp;#039;solar elevation angle&amp;#039;&amp;#039;&amp;#039; is the altitude of the [[sun]], the angle between the horizon and the centre of the sun&amp;#039;s disc. If we write &amp;#039;&amp;#039;θ&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;&amp;#039;&amp;#039;s&amp;#039;&amp;#039;&amp;lt;/sub&amp;gt; for the solar zenith angle, then the solar elevation angle &amp;#039;&amp;#039;α&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;&amp;#039;&amp;#039;s&amp;#039;&amp;#039;&amp;lt;/sub&amp;gt;&amp;amp;nbsp;=&amp;amp;nbsp;90°&amp;amp;nbsp;&amp;amp;ndash;&amp;amp;nbsp;&amp;#039;&amp;#039;θ&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;&amp;#039;&amp;#039;s&amp;#039;&amp;#039;&amp;lt;/sub&amp;gt;.&amp;lt;ref&amp;gt;{{cite doi|10.1016/B978-012369407-2/50005-X}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==Formulas==&lt;br /&gt;
&lt;br /&gt;
===Solar zenith angle===&lt;br /&gt;
The solar zenith angle, &amp;#039;&amp;#039;θ&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;&amp;#039;&amp;#039;s&amp;#039;&amp;#039;&amp;lt;/sub&amp;gt; is estimated using results from [[spherical trigonometry]] by&amp;lt;ref&amp;gt;{{cite book | page = 317 | title = Fundamentals of Atmospheric Modeling | first = Mark Z. | last = Jacobson | publisher = Cambridge University Press | year = 2005 | isbn = 0521548659 | edition = 2}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;hartmann&amp;quot;&amp;gt;{{cite book | title = Global Physical Climatology | first = Dennis L. | last = Hartmann | publisher = Academic Press | page = 30 | year = 1994 | isbn = 0080571638}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
:&amp;lt;math&amp;gt; \cos \theta_s = \sin \varphi \sin \delta + \cos \varphi \cos \delta \cos h&amp;lt;/math&amp;gt;&lt;br /&gt;
where&lt;br /&gt;
* &amp;#039;&amp;#039;θ&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;&amp;#039;&amp;#039;s&amp;#039;&amp;#039;&amp;lt;/sub&amp;gt; is the &amp;#039;&amp;#039;solar zenith angle&amp;#039;&amp;#039;&lt;br /&gt;
* &amp;#039;&amp;#039;h&amp;#039;&amp;#039; is the [[hour angle]], in the local [[solar time]].&lt;br /&gt;
* &amp;#039;&amp;#039;δ&amp;#039;&amp;#039; is the current [[declination of the Sun]]&lt;br /&gt;
* &amp;#039;&amp;#039;φ&amp;#039;&amp;#039; is the local [[latitude]].&lt;br /&gt;
&lt;br /&gt;
===Solar elevation angle===&lt;br /&gt;
The solar elevation angle is the altitude of the sun, the angle between the horizon and the centre of the sun&amp;#039;s disc. The approximate value can be calculated with the following formula:&lt;br /&gt;
:&amp;lt;math&amp;gt;\sin \alpha_\mathrm{s} = \cos h \cos \delta \cos \varphi + \sin \delta \sin \varphi&amp;lt;/math&amp;gt;&lt;br /&gt;
where&lt;br /&gt;
* &amp;#039;&amp;#039;α&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;&amp;#039;&amp;#039;s&amp;#039;&amp;#039;&amp;lt;/sub&amp;gt; is the &amp;#039;&amp;#039;solar elevation angle&amp;#039;&amp;#039;, &amp;#039;&amp;#039;α&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;&amp;#039;&amp;#039;s&amp;#039;&amp;#039;&amp;lt;/sub&amp;gt;&amp;amp;nbsp;=&amp;amp;nbsp;90°&amp;amp;nbsp;&amp;amp;ndash;&amp;amp;nbsp;&amp;#039;&amp;#039;θ&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;&amp;#039;&amp;#039;s&amp;#039;&amp;#039;&amp;lt;/sub&amp;gt;&lt;br /&gt;
* &amp;#039;&amp;#039;h&amp;#039;&amp;#039; is the [[hour angle]], in the local [[solar time]].&lt;br /&gt;
* &amp;#039;&amp;#039;δ&amp;#039;&amp;#039; is the current [[declination of the Sun]]&lt;br /&gt;
* &amp;#039;&amp;#039;φ&amp;#039;&amp;#039; is the local [[latitude]].&lt;br /&gt;
&lt;br /&gt;
===Caveats===&lt;br /&gt;
The values calculated above are approximations due to the distinction between [[Latitude#Geodetic and geocentric latitudes|common/geodetic latitude]] and [[Latitude#Geocentric latitude|geocentric latitude]]. However, the two values [[Latitude#Comparison of selected types|differ]] by less than 12 [[minutes of arc]].&lt;br /&gt;
&lt;br /&gt;
The formulas neglect the effect of [[atmospheric refraction]].&lt;br /&gt;
&lt;br /&gt;
The formula for solar elevation angle was derived using the [[trigonometric addition formulas]] from the solar zenith angle formula&amp;lt;ref&amp;gt;{{cite journal | title = On the computation of solar elevation angles and the determination of sunrise and sunset times | page = 3 | first = Harold M. | last = Woolf | journal = NASA technical memorandu, X-1646 | year = 1968 | location = Washington, D.C.}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==Applications==&lt;br /&gt;
&lt;br /&gt;
===Sunrise/Sunset===&lt;br /&gt;
The approximate times of sunset and sunrise occur when the zenith angle is 90°, where the hour angle &amp;#039;&amp;#039;h&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;0&amp;lt;/sub&amp;gt; satisfies&amp;lt;ref name=&amp;quot;hartmann&amp;quot; /&amp;gt;&lt;br /&gt;
::&amp;lt;math&amp;gt;\cos h_0 = -\tan \phi \tan \delta.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Precise times of sunset and [[Sunrise#Angle|sunrise]] occur when the upper limb of the Sun appears, as refracted by the atmosphere, to be on the horizon.&lt;br /&gt;
&lt;br /&gt;
===Albedo===&lt;br /&gt;
A weighted daily average zenith angle, used in computing the local [[albedo of the Earth]], is given by&lt;br /&gt;
::&amp;lt;math&amp;gt;\overline{\cos \theta_s} = \frac{\int_{-h_0}^{h_0} Q \cos \theta_s \text{d}h}{\int_{-h_0}^{h_0} Q \text{d}h}&amp;lt;/math&amp;gt;&lt;br /&gt;
where &amp;#039;&amp;#039;Q&amp;#039;&amp;#039; is the instantaneous [[insolation]].&amp;lt;ref name=&amp;quot;hartmann&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Summary of special angles===&lt;br /&gt;
For example, the solar elevation angle is :&lt;br /&gt;
* 90° if you are on the equator, a day of equinox, at a solar hour of twelve&lt;br /&gt;
* near 0° at the sunset or at the sunrise&lt;br /&gt;
* between -90° and 0° during the night&lt;br /&gt;
&lt;br /&gt;
An exact calculation is given in [[position of the Sun]]. Other approximations exist elsewhere.&amp;lt;ref&amp;gt;{{cite web|last=livioflores-ga|url=http://answers.google.com/answers/threadview/id/782886.html|publisher=Google|title=Equation to know where the Sun is at a given place at a given date-time|accessdate=9 March 2013}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== See also ==&lt;br /&gt;
&lt;br /&gt;
* [[Altitude (astronomy)]]&lt;br /&gt;
* [[Horizontal coordinate system]]&lt;br /&gt;
* [[Solar azimuth angle]]&lt;br /&gt;
* [[Sun]]&lt;br /&gt;
* [[Sun path]]&lt;br /&gt;
* [[Position of the Sun]]&lt;br /&gt;
* [[Sunrise]]&lt;br /&gt;
* [[Sunset]]&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
&lt;br /&gt;
&amp;lt;references/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{{DEFAULTSORT:Solar Elevation Angle}}&lt;br /&gt;
[[Category:Horizontal coordinate system]]&lt;br /&gt;
[[Category:Sun]]&lt;br /&gt;
[[Category:Solar energy]]&lt;/div&gt;</summary>
		<author><name>en&gt;Melcombe</name></author>
	</entry>
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