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	<title>2018年IOAA理论第3题-大气折射 - 版本历史</title>
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	<updated>2026-04-29T17:03:12Z</updated>
	<subtitle>本wiki的该页面的版本历史</subtitle>
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	<entry>
		<id>https://www.astro-init.top/index.php?title=2018%E5%B9%B4IOAA%E7%90%86%E8%AE%BA%E7%AC%AC3%E9%A2%98-%E5%A4%A7%E6%B0%94%E6%8A%98%E5%B0%84&amp;diff=393&amp;oldid=prev</id>
		<title>2019年8月8日 (四) 07:50 Quan787</title>
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		<updated>2019-08-08T07:50:28Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;←上一版本&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;2019年8月8日 (四) 07:50的版本&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l10&quot; &gt;第10行：&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;第10行：&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==中文翻译==&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==中文翻译==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''(T3)大气折射(&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;10 points&lt;/del&gt;)'''&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''(T3)大气折射(&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;10分&lt;/ins&gt;)'''&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;考虑北京(φ = 40°)在春分日的日出.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;考虑北京(φ = 40°)在春分日的日出.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Quan787</name></author>
		
	</entry>
	<entry>
		<id>https://www.astro-init.top/index.php?title=2018%E5%B9%B4IOAA%E7%90%86%E8%AE%BA%E7%AC%AC3%E9%A2%98-%E5%A4%A7%E6%B0%94%E6%8A%98%E5%B0%84&amp;diff=388&amp;oldid=prev</id>
		<title>Quan787：创建页面，内容为“{{需要解答}} ==英文原题== '''(T3) Atmospheric Refraction (10 points)'''  Consider sunrise at Beijing (φ=40°) on the vernal equinox day.   (a) Let us say r&lt;…”</title>
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		<updated>2019-08-08T07:46:36Z</updated>

		<summary type="html">&lt;p&gt;创建页面，内容为“{{需要解答}} ==英文原题== &amp;#039;&amp;#039;&amp;#039;(T3) Atmospheric Refraction (10 points)&amp;#039;&amp;#039;&amp;#039;  Consider sunrise at Beijing (φ=40°) on the vernal equinox day.   (a) Let us say r&amp;lt;…”&lt;/p&gt;
&lt;p&gt;&lt;b&gt;新页面&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{需要解答}}&lt;br /&gt;
==英文原题==&lt;br /&gt;
'''(T3) Atmospheric Refraction (10 points)'''&lt;br /&gt;
&lt;br /&gt;
Consider sunrise at Beijing (φ=40°) on the vernal equinox day. &lt;br /&gt;
&lt;br /&gt;
(a) Let us say r&amp;lt;sub&amp;gt;l&amp;lt;/sub&amp;gt;, r&amp;lt;sub&amp;gt;d&amp;lt;/sub&amp;gt;, r&amp;lt;sub&amp;gt;r&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;u&amp;lt;/sub&amp;gt; are distances from the centre of the undistorted disk of the Sun to the edge of the disk towards the directions left, down, right and up respectively. What will be the hierarchical relation (&amp;lt;, =, &amp;gt;) between the four radii just after the sunrise? &lt;br /&gt;
&lt;br /&gt;
(b) What is the correction in the time of rise of the top edge of the disk as compared to the case without atmosphere? You may assume that typically atmospheric refraction near the horizon is 35’. Please only consider the apparent diurnal motion.&lt;br /&gt;
&lt;br /&gt;
==中文翻译==&lt;br /&gt;
'''(T3)大气折射(10 points)'''&lt;br /&gt;
&lt;br /&gt;
考虑北京(φ = 40°)在春分日的日出.&lt;br /&gt;
&lt;br /&gt;
(a)	令r&amp;lt;sub&amp;gt;l&amp;lt;/sub&amp;gt;,r&amp;lt;sub&amp;gt;d&amp;lt;/sub&amp;gt;,r&amp;lt;sub&amp;gt;r&amp;lt;/sub&amp;gt;和r&amp;lt;sub&amp;gt;u&amp;lt;/sub&amp;gt;分别为从没有畸变的日面中心向左,向下,向右,向上到日面边缘的距离.问日出后, 这四个半径的大小关系(&amp;lt; , = , &amp;gt;)?&lt;br /&gt;
&lt;br /&gt;
(b)	如果没有大气层,日面上边缘升起的时间应该做怎样的修正.你可以假设为大气折射在地平线附近是35’的典型情形.请只考虑周日视动&lt;br /&gt;
&lt;br /&gt;
[[分类:大气折射]]&lt;/div&gt;</summary>
		<author><name>Quan787</name></author>
		
	</entry>
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