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	<id>https://energyeducation.ca/wiki/index.php?action=history&amp;feed=atom&amp;title=Earth%27s_energy_budget</id>
	<title>Earth&#039;s energy budget - Revision history</title>
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	<updated>2026-09-02T10:40:59Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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		<id>https://energyeducation.ca/wiki/index.php?title=Earth%27s_energy_budget&amp;diff=10187&amp;oldid=prev</id>
		<title>Jmdonev: 1 revision imported</title>
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		<updated>2021-09-27T00:03:09Z</updated>

		<summary type="html">&lt;p&gt;1 revision imported&lt;/p&gt;
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				&lt;td colspan=&quot;1&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;1&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 00:03, 27 September 2021&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-notice&quot; lang=&quot;en&quot;&gt;&lt;div class=&quot;mw-diff-empty&quot;&gt;(No difference)&lt;/div&gt;
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		<author><name>Jmdonev</name></author>
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		<id>https://energyeducation.ca/wiki/index.php?title=Earth%27s_energy_budget&amp;diff=10186&amp;oldid=prev</id>
		<title>energy&gt;Ethan.boechler at 20:17, 10 September 2021</title>
		<link rel="alternate" type="text/html" href="https://energyeducation.ca/wiki/index.php?title=Earth%27s_energy_budget&amp;diff=10186&amp;oldid=prev"/>
		<updated>2021-09-10T20:17:04Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 20:17, 10 September 2021&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-l1&quot;&gt;Line 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;[[Category:Done 2018-05-18]]  &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;[[Category:Done 2018-05-18]]  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-deleted&quot;&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;[[Category:Translated to French]]&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-deleted&quot;&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;[[fr:Bilan énergétique de la Terre]]&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;&amp;lt;onlyinclude&amp;gt;&amp;#039;&amp;#039;&amp;#039;Earth&amp;#039;s energy budget&amp;#039;&amp;#039;&amp;#039; refers to the tracking of how much [[energy]] is flowing into and out of the Earth&amp;#039;s [[climate]], where the energy is going, and if the energy coming in balances with the energy going out.&amp;lt;/onlyinclude&amp;gt;&amp;lt;ref name=&amp;quot;RE1&amp;quot;&amp;gt;John Cook, Hayden Washington. (May 8, 2015). &amp;#039;&amp;#039;Climate Change Denial: Heads in the Sand&amp;#039;&amp;#039;, 1st Edition. Washington, DC, Earthscan 2011.&amp;lt;/ref&amp;gt; Understanding the Earth&amp;#039;s energy budget can help to predict future effects of [[global warming]], and to understand the various [[Earth&amp;#039;s energy flows|flows of energy on the Earth]]. Additionally, knowing how Earth&amp;#039;s energy budget balances can provide insight into how the [[Solar energy to the Earth|energy from the Sun]] interacts with the [[atmosphere]]. For example, this is important when examining the affects of  [[greenhouse gases]] in the atmosphere—to ensure conditions on Earth are habitable. For the energy budget to balance, all that needs to occur is:&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;&amp;lt;onlyinclude&amp;gt;&amp;#039;&amp;#039;&amp;#039;Earth&amp;#039;s energy budget&amp;#039;&amp;#039;&amp;#039; refers to the tracking of how much [[energy]] is flowing into and out of the Earth&amp;#039;s [[climate]], where the energy is going, and if the energy coming in balances with the energy going out.&amp;lt;/onlyinclude&amp;gt;&amp;lt;ref name=&amp;quot;RE1&amp;quot;&amp;gt;John Cook, Hayden Washington. (May 8, 2015). &amp;#039;&amp;#039;Climate Change Denial: Heads in the Sand&amp;#039;&amp;#039;, 1st Edition. Washington, DC, Earthscan 2011.&amp;lt;/ref&amp;gt; Understanding the Earth&amp;#039;s energy budget can help to predict future effects of [[global warming]], and to understand the various [[Earth&amp;#039;s energy flows|flows of energy on the Earth]]. Additionally, knowing how Earth&amp;#039;s energy budget balances can provide insight into how the [[Solar energy to the Earth|energy from the Sun]] interacts with the [[atmosphere]]. For example, this is important when examining the affects of  [[greenhouse gases]] in the atmosphere—to ensure conditions on Earth are habitable. For the energy budget to balance, all that needs to occur is:&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;&amp;lt;center&amp;gt;&amp;lt;math&amp;gt;Energy\;in=Energy\;out&amp;lt;/math&amp;gt;&amp;lt;/center&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;&amp;lt;center&amp;gt;&amp;lt;math&amp;gt;Energy\;in=Energy\;out&amp;lt;/math&amp;gt;&amp;lt;/center&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;==Earth&amp;#039;s Energy Balance==&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;==Earth&amp;#039;s Energy Balance==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;The two major components that must be investigated to determine if the Earth&#039;s energy budget balances is the incoming energy from the Sun and the outgoing infrared [[radiation]] from the Earth and its atmosphere. Looking &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;more closely &lt;/del&gt;at the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;interactions &lt;/del&gt;that occur &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;in &lt;/del&gt;the atmosphere and &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;on &lt;/del&gt;the surface of the Earth can help to understand &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;more of &lt;/del&gt;&#039;&#039;how&#039;&#039; the Earth&#039;s energy budget &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;balances by investigating the energy flows&lt;/del&gt;. Figure 1 shows the current understanding of how energy flows generally look on the Earth.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;The two major components that must be investigated to determine if the Earth&#039;s energy budget balances is the incoming energy from the Sun and the outgoing infrared [[radiation]] from the Earth and its atmosphere. Looking at the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;energy flows &lt;/ins&gt;that occur &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;between &lt;/ins&gt;the atmosphere and the surface of the Earth can help to understand &#039;&#039;how&#039;&#039; the Earth&#039;s energy budget &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;is balanced&lt;/ins&gt;. Figure 1 shows the current understanding of how energy flows generally look on the Earth.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;[[File:EnergyBudget3.png|400px|framed|center|Figure 1. Detailed diagram showing incoming and outgoing energy in a balanced example of Earth&amp;#039;s energy budget, with incoming and outgoing values of 341 W/m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;. General flows of energy on the surface and in the atmosphere are shown as well.&amp;lt;ref&amp;gt;&amp;#039;&amp;#039;Created internally by a member of the Energy Education team.&amp;#039;&amp;#039; Adapted from: R. Wolfson, Figure 12.5 in &amp;#039;&amp;#039;Energy, Environment and Climate&amp;#039;&amp;#039;, 2nd ed. New York, U.S.A.: Norton, 2012, pp. 331&amp;lt;/ref&amp;gt;]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;[[File:EnergyBudget3.png|400px|framed|center|Figure 1. Detailed diagram showing incoming and outgoing energy in a balanced example of Earth&amp;#039;s energy budget, with incoming and outgoing values of 341 W/m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;. General flows of energy on the surface and in the atmosphere are shown as well.&amp;lt;ref&amp;gt;&amp;#039;&amp;#039;Created internally by a member of the Energy Education team.&amp;#039;&amp;#039; Adapted from: R. Wolfson, Figure 12.5 in &amp;#039;&amp;#039;Energy, Environment and Climate&amp;#039;&amp;#039;, 2nd ed. New York, U.S.A.: Norton, 2012, pp. 331&amp;lt;/ref&amp;gt;]]&lt;/div&gt;&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-l15&quot;&gt;Line 15:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 17:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;The incoming energy to the Earth and the outgoing energy from the Earth do not actually balance. This imbalance is partially caused by the incoming energy from the Sun—which varies with the seasons and changes in the composition of the Earth&amp;#039;s atmosphere.&amp;lt;ref name=&amp;quot;wolfson&amp;quot;&amp;gt;R. Wolfson, (May 8, 2015). &amp;#039;&amp;#039;Energy, Environment and Climate&amp;#039;&amp;#039;, 2nd ed. New York, U.S.A.: Norton, 2012.&amp;lt;/ref&amp;gt; Changes in the composition of Earth&amp;#039;s atmosphere alters the quantity of energy absorbed and reflected by the atmosphere seen in Figure 1. Changing factors such as these result in a very small, but significant energy imbalance on the Earth.  &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;The incoming energy to the Earth and the outgoing energy from the Earth do not actually balance. This imbalance is partially caused by the incoming energy from the Sun—which varies with the seasons and changes in the composition of the Earth&amp;#039;s atmosphere.&amp;lt;ref name=&amp;quot;wolfson&amp;quot;&amp;gt;R. Wolfson, (May 8, 2015). &amp;#039;&amp;#039;Energy, Environment and Climate&amp;#039;&amp;#039;, 2nd ed. New York, U.S.A.: Norton, 2012.&amp;lt;/ref&amp;gt; Changes in the composition of Earth&amp;#039;s atmosphere alters the quantity of energy absorbed and reflected by the atmosphere seen in Figure 1. Changing factors such as these result in a very small, but significant energy imbalance on the Earth.  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;As human activities increase the amount of [[carbon dioxide]] in the atmosphere, the energy imbalance continues to grow. Today, the energy imbalance amounts to approximately &amp;lt;math&amp;gt;0.9 \frac{W}{m^2}&amp;lt;/math&amp;gt; &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;of &lt;/del&gt;energy is coming in&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;, &lt;/del&gt;than is leaving the Earth.&amp;lt;ref name=&quot;wolfson&quot;/&amp;gt; Compared to flow values in the hundreds of [[watt]]s per [[meter]] squared, this imbalance seems negligible. However, to account for this imbalance, the Earth&#039;s temperature will increase in response. As well, since the amounts of carbon dioxide and other greenhouse gases in our atmosphere are increasing, this value is projected to increase at a rate of &amp;lt;math&amp;gt;0.3 \frac{W}{m^2}&amp;lt;/math&amp;gt; per decade, contributing even more to increasing temperatures.&amp;lt;ref&amp;gt;M. Balmaseda, J.Fasullo, and E. Trenberth. (May 8, 2015). &#039;&#039;Earth&#039;s Energy Imbalance&#039;&#039; [Online]. Available: http://www.cgd.ucar.edu/staff/trenbert/trenberth.papers/T_F_B_energyImb_JCLI_14.pdf&amp;lt;/ref&amp;gt; It is this imbalance in the energy budget that results in increasing temperatures on the Earth, one of the most significant effects of [[climate change]].  &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;As human activities increase the amount of [[carbon dioxide]] in the atmosphere, the energy imbalance continues to grow. Today, the energy imbalance amounts to approximately &amp;lt;math&amp;gt;0.9 \frac{W}{m^2}&amp;lt;/math&amp;gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;. This means that more &lt;/ins&gt;energy is coming in &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;(and being absorbed) &lt;/ins&gt;than is leaving the Earth.&amp;lt;ref name=&quot;wolfson&quot;/&amp;gt; Compared to flow values in the hundreds of [[watt]]s per [[meter]] squared, this imbalance seems negligible. However, to account for this imbalance, the Earth&#039;s temperature will increase in response. As well, since the amounts of carbon dioxide and other greenhouse gases in our atmosphere are increasing, this value is projected to increase at a rate of &amp;lt;math&amp;gt;0.3 \frac{W}{m^2}&amp;lt;/math&amp;gt; per decade, contributing even more to increasing temperatures.&amp;lt;ref&amp;gt;M. Balmaseda, J.Fasullo, and E. Trenberth. (May 8, 2015). &#039;&#039;Earth&#039;s Energy Imbalance&#039;&#039; [Online]. Available: http://www.cgd.ucar.edu/staff/trenbert/trenberth.papers/T_F_B_energyImb_JCLI_14.pdf&amp;lt;/ref&amp;gt; It is this imbalance in the energy budget that results in increasing temperatures on the Earth, one of the most significant effects of [[climate change]].  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;==References==&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;==References==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;{{reflist}}&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;{{reflist}}&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;[[Category:Uploaded]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;[[Category:Uploaded]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>energy&gt;Ethan.boechler</name></author>
	</entry>
	<entry>
		<id>https://energyeducation.ca/wiki/index.php?title=Earth%27s_energy_budget&amp;diff=6179&amp;oldid=prev</id>
		<title>Jmdonev: 1 revision imported</title>
		<link rel="alternate" type="text/html" href="https://energyeducation.ca/wiki/index.php?title=Earth%27s_energy_budget&amp;diff=6179&amp;oldid=prev"/>
		<updated>2018-05-18T22:53:07Z</updated>

		<summary type="html">&lt;p&gt;1 revision imported&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;1&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;1&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 22:53, 18 May 2018&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-notice&quot; lang=&quot;en&quot;&gt;&lt;div class=&quot;mw-diff-empty&quot;&gt;(No difference)&lt;/div&gt;
&lt;/td&gt;&lt;/tr&gt;&lt;/table&gt;</summary>
		<author><name>Jmdonev</name></author>
	</entry>
	<entry>
		<id>https://energyeducation.ca/wiki/index.php?title=Earth%27s_energy_budget&amp;diff=6178&amp;oldid=prev</id>
		<title>Jmdonev at 18:57, 11 May 2018</title>
		<link rel="alternate" type="text/html" href="https://energyeducation.ca/wiki/index.php?title=Earth%27s_energy_budget&amp;diff=6178&amp;oldid=prev"/>
		<updated>2018-05-11T18:57:40Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 18:57, 11 May 2018&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-l1&quot;&gt;Line 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;[[Category:Done &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;2015&lt;/del&gt;-&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;07&lt;/del&gt;-&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;24&lt;/del&gt;]]  &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;[[Category:Done &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;2018&lt;/ins&gt;-&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;05&lt;/ins&gt;-&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;18&lt;/ins&gt;]]  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;&amp;lt;onlyinclude&amp;gt;&#039;&#039;&#039;Earth&#039;s energy budget&#039;&#039;&#039; refers to the tracking of how much [[energy]] is flowing into and out of the Earth&#039;s [[climate]], where the energy is going, and if the energy in balances with the energy out.&amp;lt;/onlyinclude&amp;gt;&amp;lt;ref name=&quot;RE1&quot;&amp;gt;John Cook, Hayden Washington. (May 8, 2015). &#039;&#039;Climate Change Denial: Heads in the Sand&#039;&#039;, 1st Edition. Washington, DC, Earthscan 2011.&amp;lt;/ref&amp;gt; Understanding the Earth&#039;s energy budget can help to predict future effects of [[global warming]], &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;as well as helping &lt;/del&gt;to understand [[Earth&#039;s energy flows|flows of energy on the Earth]]. Additionally, knowing how Earth&#039;s energy budget balances can provide insight into how the [[Solar energy to the Earth|energy from the Sun]] interacts with the [[atmosphere]] &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;- specifically with &lt;/del&gt;the [[greenhouse gases]] in the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;atmosphere - to create &lt;/del&gt;conditions &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;that make the &lt;/del&gt;Earth habitable. For the energy budget to balance, all that needs to occur is:&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;&amp;lt;onlyinclude&amp;gt;&#039;&#039;&#039;Earth&#039;s energy budget&#039;&#039;&#039; refers to the tracking of how much [[energy]] is flowing into and out of the Earth&#039;s [[climate]], where the energy is going, and if the energy &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;coming &lt;/ins&gt;in balances with the energy &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;going &lt;/ins&gt;out.&amp;lt;/onlyinclude&amp;gt;&amp;lt;ref name=&quot;RE1&quot;&amp;gt;John Cook, Hayden Washington. (May 8, 2015). &#039;&#039;Climate Change Denial: Heads in the Sand&#039;&#039;, 1st Edition. Washington, DC, Earthscan 2011.&amp;lt;/ref&amp;gt; Understanding the Earth&#039;s energy budget can help to predict future effects of [[global warming]], &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;and &lt;/ins&gt;to understand &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;the various &lt;/ins&gt;[[Earth&#039;s energy flows|flows of energy on the Earth]]. Additionally, knowing how Earth&#039;s energy budget balances can provide insight into how the [[Solar energy to the Earth|energy from the Sun]] interacts with the [[atmosphere]]&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;. For example, this is important when examining &lt;/ins&gt;the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;affects of  &lt;/ins&gt;[[greenhouse gases]] in the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;atmosphere—to ensure &lt;/ins&gt;conditions &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;on &lt;/ins&gt;Earth &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;are &lt;/ins&gt;habitable. For the energy budget to balance, all that needs to occur is:&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;&amp;lt;center&amp;gt;&amp;lt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;m&lt;/del&gt;&amp;gt;Energy\;in=Energy\;out&amp;lt;/&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;m&lt;/del&gt;&amp;gt;&amp;lt;/center&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;&amp;lt;center&amp;gt;&amp;lt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;math&lt;/ins&gt;&amp;gt;Energy\;in=Energy\;out&amp;lt;/&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;math&lt;/ins&gt;&amp;gt;&amp;lt;/center&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;==Earth&amp;#039;s Energy Balance==&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;==Earth&amp;#039;s Energy Balance==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;The two major components that must be investigated to determine if the Earth&#039;s energy budget balances is the incoming energy from the Sun and the outgoing infrared [[radiation]] from the Earth and its atmosphere. Looking more closely at the interactions that occur in the atmosphere and on the surface of the Earth can help to understand more of &#039;&#039;how&#039;&#039; the Earth&#039;s energy budget balances by investigating the energy flows. Figure 1 shows the current understanding of how energy flows on the Earth &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;look in broad terms&lt;/del&gt;.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;The two major components that must be investigated to determine if the Earth&#039;s energy budget balances is the incoming energy from the Sun and the outgoing infrared [[radiation]] from the Earth and its atmosphere. Looking more closely at the interactions that occur in the atmosphere and on the surface of the Earth can help to understand more of &#039;&#039;how&#039;&#039; the Earth&#039;s energy budget balances by investigating the energy flows. Figure 1 shows the current understanding of how energy flows &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;generally look &lt;/ins&gt;on the Earth.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;[[File:EnergyBudget3.png|400px|framed|center|Figure 1. Detailed diagram showing incoming and outgoing energy in a balanced example of Earth&amp;#039;s energy budget, with incoming and outgoing values of 341 W/m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;. General flows of energy on the surface and in the atmosphere are shown as well.&amp;lt;ref&amp;gt;&amp;#039;&amp;#039;Created internally by a member of the Energy Education team.&amp;#039;&amp;#039; Adapted from: R. Wolfson, Figure 12.5 in &amp;#039;&amp;#039;Energy, Environment and Climate&amp;#039;&amp;#039;, 2nd ed. New York, U.S.A.: Norton, 2012, pp. 331&amp;lt;/ref&amp;gt;]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;[[File:EnergyBudget3.png|400px|framed|center|Figure 1. Detailed diagram showing incoming and outgoing energy in a balanced example of Earth&amp;#039;s energy budget, with incoming and outgoing values of 341 W/m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;. General flows of energy on the surface and in the atmosphere are shown as well.&amp;lt;ref&amp;gt;&amp;#039;&amp;#039;Created internally by a member of the Energy Education team.&amp;#039;&amp;#039; Adapted from: R. Wolfson, Figure 12.5 in &amp;#039;&amp;#039;Energy, Environment and Climate&amp;#039;&amp;#039;, 2nd ed. New York, U.S.A.: Norton, 2012, pp. 331&amp;lt;/ref&amp;gt;]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;Earth&#039;s energy budget is vital in establishing the Earth&#039;s climate. When the energy budget balances, the [[temperature]] on the Earth stays relatively constant, with no overall increase or decrease in average temperature. The energy coming in to the Earth comes from the Sun, and over the surface of the planet this incoming radiation has a rate of transport of &amp;lt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;m&lt;/del&gt;&amp;gt;341 \frac{W}{m^2}&amp;lt;/&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;m&lt;/del&gt;&amp;gt;. A thorough explanation of how this value is determined can be found [[Solar energy to the Earth#Calculating Solar Energy to Surface|here]].  &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;Earth&#039;s energy budget is vital in establishing the Earth&#039;s climate. When the energy budget balances, the [[temperature]] on the Earth stays relatively constant, with no overall increase or decrease in average temperature. The energy coming in to the Earth comes from the Sun, and over the surface of the planet this incoming radiation has a rate of transport of &amp;lt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;math&lt;/ins&gt;&amp;gt;341 \frac{W}{m^2}&amp;lt;/&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;math&lt;/ins&gt;&amp;gt;. A thorough explanation of how this value is determined can be found [[Solar energy to the Earth#Calculating Solar Energy to Surface|here]].  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Not &lt;/del&gt;all of this energy reaches the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Earths &lt;/del&gt;atmosphere or surface &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;however, &lt;/del&gt;as some is reflected by [[cloud]]s or the atmosphere. The energy that does pass through is absorbed by the atmosphere or the surface, and then moves around through [[convection]], [[evaporation]], or in the form of [[latent heat]].&amp;lt;ref name=&quot;RE2&quot;&amp;gt;NASA Earth Observatory. (May 8, 2015). &#039;&#039;Climate and Earth&#039;s Energy Budget&#039;&#039; [Online]. Available: http://earthobservatory.nasa.gov/Features/EnergyBalance&amp;lt;/ref&amp;gt; Finally, when the energy exits the Earth it can do so by emission from the surface of the Earth, by clouds, or by the atmosphere. Some of the energy that is radiated by the surface of the Earth is absorbed by clouds and greenhouse gases in the atmosphere and then re-emitted downwards, which is how the surface of the Earth is heated and kept at a habitable temperature. This process of heating is known as the [[The greenhouse effect and Earth&#039;s energy budget|greenhouse effect]]. Overall, the energy that exits the Earth in different forms, when added together is equal to the energy that is absorbed by different parts of the Earth.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;However, not &lt;/ins&gt;all of this energy reaches the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Earth&#039;s &lt;/ins&gt;atmosphere or surface as some is reflected by [[cloud]]s or the atmosphere. The energy that does pass through is absorbed by the atmosphere or the surface, and then moves around through [[convection]], [[evaporation]], or in the form of [[latent heat]].&amp;lt;ref name=&quot;RE2&quot;&amp;gt;NASA Earth Observatory. (May 8, 2015). &#039;&#039;Climate and Earth&#039;s Energy Budget&#039;&#039; [Online]. Available: http://earthobservatory.nasa.gov/Features/EnergyBalance&amp;lt;/ref&amp;gt; Finally, when the energy exits the Earth it can do so by emission from the surface of the Earth, by clouds, or by the atmosphere. Some of the energy that is radiated by the surface of the Earth is absorbed by clouds and greenhouse gases in the atmosphere and then re-emitted downwards, which is how the surface of the Earth is heated and kept at a habitable temperature. This process of heating is known as the [[The greenhouse effect and Earth&#039;s energy budget|greenhouse effect]]. Overall, the energy that exits the Earth in different forms, when added together is equal to the energy that is absorbed by different parts of the Earth.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;==Earth&amp;#039;s Energy Imbalance==&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;==Earth&amp;#039;s Energy Imbalance==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;The incoming energy to the Earth and the outgoing energy from the Earth do not actually balance. This imbalance is partially caused by the incoming energy from the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Sun - which &lt;/del&gt;varies with the seasons &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;- but due also to &lt;/del&gt;changes in the composition of the Earth&#039;s atmosphere.&amp;lt;ref name=&quot;wolfson&quot;&amp;gt;R. Wolfson, (May 8, 2015). &#039;&#039;Energy, Environment and Climate&#039;&#039;, 2nd ed. New York, U.S.A.: Norton, 2012.&amp;lt;/ref&amp;gt; Changes in the composition of Earth&#039;s atmosphere &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;changes &lt;/del&gt;the &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;values &lt;/del&gt;of energy absorbed and reflected by the atmosphere&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;, shown &lt;/del&gt;in Figure 1. Changing factors such as these result in a very small, but significant energy imbalance on the Earth.  &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;The incoming energy to the Earth and the outgoing energy from the Earth do not actually balance. This imbalance is partially caused by the incoming energy from the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Sun—which &lt;/ins&gt;varies with the seasons &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;and &lt;/ins&gt;changes in the composition of the Earth&#039;s atmosphere.&amp;lt;ref name=&quot;wolfson&quot;&amp;gt;R. Wolfson, (May 8, 2015). &#039;&#039;Energy, Environment and Climate&#039;&#039;, 2nd ed. New York, U.S.A.: Norton, 2012.&amp;lt;/ref&amp;gt; Changes in the composition of Earth&#039;s atmosphere &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;alters &lt;/ins&gt;the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;quantity &lt;/ins&gt;of energy absorbed and reflected by the atmosphere &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;seen &lt;/ins&gt;in Figure 1. Changing factors such as these result in a very small, but significant energy imbalance on the Earth.  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;As human activities increase the amount of [[carbon dioxide]] in the atmosphere, the energy imbalance continues to grow. Today, the energy imbalance amounts to approximately &amp;lt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;m&lt;/del&gt;&amp;gt;0.9 \frac{W}{m^2}&amp;lt;/&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;m&lt;/del&gt;&amp;gt; &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;more &lt;/del&gt;energy &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;incoming &lt;/del&gt;than is leaving the Earth.&amp;lt;ref name=&quot;wolfson&quot;/&amp;gt; Compared to flow values in the hundreds of [[watt]]s per [[meter]] squared, this imbalance seems negligible. However, to account for this imbalance, the Earth&#039;s temperature will increase in response. As well, since the amounts of carbon dioxide and other greenhouse gases in our atmosphere are increasing, this value is projected to increase at a rate of &amp;lt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;m&lt;/del&gt;&amp;gt;0.3 \frac{W}{m^2}&amp;lt;/&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;m&lt;/del&gt;&amp;gt; per decade, contributing even more to increasing temperatures.&amp;lt;ref&amp;gt;M. Balmaseda, J.Fasullo, and E. Trenberth. (May 8, 2015). &#039;&#039;Earth&#039;s Energy Imbalance&#039;&#039; [Online]. Available: http://www.cgd.ucar.edu/staff/trenbert/trenberth.papers/T_F_B_energyImb_JCLI_14.pdf&amp;lt;/ref&amp;gt; It is this imbalance in the energy budget that results in increasing temperatures on the Earth, one of the most significant effects of [[climate change]].  &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; 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;As human activities increase the amount of [[carbon dioxide]] in the atmosphere, the energy imbalance continues to grow. Today, the energy imbalance amounts to approximately &amp;lt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;math&lt;/ins&gt;&amp;gt;0.9 \frac{W}{m^2}&amp;lt;/&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;math&lt;/ins&gt;&amp;gt; &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;of &lt;/ins&gt;energy &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;is coming in, &lt;/ins&gt;than is leaving the Earth.&amp;lt;ref name=&quot;wolfson&quot;/&amp;gt; Compared to flow values in the hundreds of [[watt]]s per [[meter]] squared, this imbalance seems negligible. However, to account for this imbalance, the Earth&#039;s temperature will increase in response. As well, since the amounts of carbon dioxide and other greenhouse gases in our atmosphere are increasing, this value is projected to increase at a rate of &amp;lt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;math&lt;/ins&gt;&amp;gt;0.3 \frac{W}{m^2}&amp;lt;/&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;math&lt;/ins&gt;&amp;gt; per decade, contributing even more to increasing temperatures.&amp;lt;ref&amp;gt;M. Balmaseda, J.Fasullo, and E. Trenberth. (May 8, 2015). &#039;&#039;Earth&#039;s Energy Imbalance&#039;&#039; [Online]. Available: http://www.cgd.ucar.edu/staff/trenbert/trenberth.papers/T_F_B_energyImb_JCLI_14.pdf&amp;lt;/ref&amp;gt; It is this imbalance in the energy budget that results in increasing temperatures on the Earth, one of the most significant effects of [[climate change]].  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;==References==&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;==References==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;{{reflist}}&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;{{reflist}}&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;[[Category:Uploaded]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; 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;[[Category:Uploaded]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Jmdonev</name></author>
	</entry>
	<entry>
		<id>https://energyeducation.ca/wiki/index.php?title=Earth%27s_energy_budget&amp;diff=152&amp;oldid=prev</id>
		<title>J.williams: 1 revision imported</title>
		<link rel="alternate" type="text/html" href="https://energyeducation.ca/wiki/index.php?title=Earth%27s_energy_budget&amp;diff=152&amp;oldid=prev"/>
		<updated>2015-08-26T21:30:44Z</updated>

		<summary type="html">&lt;p&gt;1 revision imported&lt;/p&gt;
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				&lt;td colspan=&quot;1&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;1&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 21:30, 26 August 2015&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-notice&quot; lang=&quot;en&quot;&gt;&lt;div class=&quot;mw-diff-empty&quot;&gt;(No difference)&lt;/div&gt;
&lt;/td&gt;&lt;/tr&gt;&lt;/table&gt;</summary>
		<author><name>J.williams</name></author>
	</entry>
	<entry>
		<id>https://energyeducation.ca/wiki/index.php?title=Earth%27s_energy_budget&amp;diff=151&amp;oldid=prev</id>
		<title>J.williams at 22:46, 11 August 2015</title>
		<link rel="alternate" type="text/html" href="https://energyeducation.ca/wiki/index.php?title=Earth%27s_energy_budget&amp;diff=151&amp;oldid=prev"/>
		<updated>2015-08-11T22:46:18Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;[[Category:Done 2015-07-24]] &lt;br /&gt;
&amp;lt;onlyinclude&amp;gt;&amp;#039;&amp;#039;&amp;#039;Earth&amp;#039;s energy budget&amp;#039;&amp;#039;&amp;#039; refers to the tracking of how much [[energy]] is flowing into and out of the Earth&amp;#039;s [[climate]], where the energy is going, and if the energy in balances with the energy out.&amp;lt;/onlyinclude&amp;gt;&amp;lt;ref name=&amp;quot;RE1&amp;quot;&amp;gt;John Cook, Hayden Washington. (May 8, 2015). &amp;#039;&amp;#039;Climate Change Denial: Heads in the Sand&amp;#039;&amp;#039;, 1st Edition. Washington, DC, Earthscan 2011.&amp;lt;/ref&amp;gt; Understanding the Earth&amp;#039;s energy budget can help to predict future effects of [[global warming]], as well as helping to understand [[Earth&amp;#039;s energy flows|flows of energy on the Earth]]. Additionally, knowing how Earth&amp;#039;s energy budget balances can provide insight into how the [[Solar energy to the Earth|energy from the Sun]] interacts with the [[atmosphere]] - specifically with the [[greenhouse gases]] in the atmosphere - to create conditions that make the Earth habitable. For the energy budget to balance, all that needs to occur is:&lt;br /&gt;
&amp;lt;center&amp;gt;&amp;lt;m&amp;gt;Energy\;in=Energy\;out&amp;lt;/m&amp;gt;&amp;lt;/center&amp;gt;&lt;br /&gt;
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==Earth&amp;#039;s Energy Balance==&lt;br /&gt;
The two major components that must be investigated to determine if the Earth&amp;#039;s energy budget balances is the incoming energy from the Sun and the outgoing infrared [[radiation]] from the Earth and its atmosphere. Looking more closely at the interactions that occur in the atmosphere and on the surface of the Earth can help to understand more of &amp;#039;&amp;#039;how&amp;#039;&amp;#039; the Earth&amp;#039;s energy budget balances by investigating the energy flows. Figure 1 shows the current understanding of how energy flows on the Earth look in broad terms.&lt;br /&gt;
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[[File:EnergyBudget3.png|400px|framed|center|Figure 1. Detailed diagram showing incoming and outgoing energy in a balanced example of Earth&amp;#039;s energy budget, with incoming and outgoing values of 341 W/m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;. General flows of energy on the surface and in the atmosphere are shown as well.&amp;lt;ref&amp;gt;&amp;#039;&amp;#039;Created internally by a member of the Energy Education team.&amp;#039;&amp;#039; Adapted from: R. Wolfson, Figure 12.5 in &amp;#039;&amp;#039;Energy, Environment and Climate&amp;#039;&amp;#039;, 2nd ed. New York, U.S.A.: Norton, 2012, pp. 331&amp;lt;/ref&amp;gt;]]&lt;br /&gt;
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Earth&amp;#039;s energy budget is vital in establishing the Earth&amp;#039;s climate. When the energy budget balances, the [[temperature]] on the Earth stays relatively constant, with no overall increase or decrease in average temperature. The energy coming in to the Earth comes from the Sun, and over the surface of the planet this incoming radiation has a rate of transport of &amp;lt;m&amp;gt;341 \frac{W}{m^2}&amp;lt;/m&amp;gt;. A thorough explanation of how this value is determined can be found [[Solar energy to the Earth#Calculating Solar Energy to Surface|here]]. &lt;br /&gt;
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Not all of this energy reaches the Earths atmosphere or surface however, as some is reflected by [[cloud]]s or the atmosphere. The energy that does pass through is absorbed by the atmosphere or the surface, and then moves around through [[convection]], [[evaporation]], or in the form of [[latent heat]].&amp;lt;ref name=&amp;quot;RE2&amp;quot;&amp;gt;NASA Earth Observatory. (May 8, 2015). &amp;#039;&amp;#039;Climate and Earth&amp;#039;s Energy Budget&amp;#039;&amp;#039; [Online]. Available: http://earthobservatory.nasa.gov/Features/EnergyBalance&amp;lt;/ref&amp;gt; Finally, when the energy exits the Earth it can do so by emission from the surface of the Earth, by clouds, or by the atmosphere. Some of the energy that is radiated by the surface of the Earth is absorbed by clouds and greenhouse gases in the atmosphere and then re-emitted downwards, which is how the surface of the Earth is heated and kept at a habitable temperature. This process of heating is known as the [[The greenhouse effect and Earth&amp;#039;s energy budget|greenhouse effect]]. Overall, the energy that exits the Earth in different forms, when added together is equal to the energy that is absorbed by different parts of the Earth.&lt;br /&gt;
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==Earth&amp;#039;s Energy Imbalance==&lt;br /&gt;
The incoming energy to the Earth and the outgoing energy from the Earth do not actually balance. This imbalance is partially caused by the incoming energy from the Sun - which varies with the seasons - but due also to changes in the composition of the Earth&amp;#039;s atmosphere.&amp;lt;ref name=&amp;quot;wolfson&amp;quot;&amp;gt;R. Wolfson, (May 8, 2015). &amp;#039;&amp;#039;Energy, Environment and Climate&amp;#039;&amp;#039;, 2nd ed. New York, U.S.A.: Norton, 2012.&amp;lt;/ref&amp;gt; Changes in the composition of Earth&amp;#039;s atmosphere changes the values of energy absorbed and reflected by the atmosphere, shown in Figure 1. Changing factors such as these result in a very small, but significant energy imbalance on the Earth. &lt;br /&gt;
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As human activities increase the amount of [[carbon dioxide]] in the atmosphere, the energy imbalance continues to grow. Today, the energy imbalance amounts to approximately &amp;lt;m&amp;gt;0.9 \frac{W}{m^2}&amp;lt;/m&amp;gt; more energy incoming than is leaving the Earth.&amp;lt;ref name=&amp;quot;wolfson&amp;quot;/&amp;gt; Compared to flow values in the hundreds of [[watt]]s per [[meter]] squared, this imbalance seems negligible. However, to account for this imbalance, the Earth&amp;#039;s temperature will increase in response. As well, since the amounts of carbon dioxide and other greenhouse gases in our atmosphere are increasing, this value is projected to increase at a rate of &amp;lt;m&amp;gt;0.3 \frac{W}{m^2}&amp;lt;/m&amp;gt; per decade, contributing even more to increasing temperatures.&amp;lt;ref&amp;gt;M. Balmaseda, J.Fasullo, and E. Trenberth. (May 8, 2015). &amp;#039;&amp;#039;Earth&amp;#039;s Energy Imbalance&amp;#039;&amp;#039; [Online]. Available: http://www.cgd.ucar.edu/staff/trenbert/trenberth.papers/T_F_B_energyImb_JCLI_14.pdf&amp;lt;/ref&amp;gt; It is this imbalance in the energy budget that results in increasing temperatures on the Earth, one of the most significant effects of [[climate change]]. &lt;br /&gt;
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==References==&lt;br /&gt;
{{reflist}}&lt;br /&gt;
[[Category:Uploaded]]&lt;/div&gt;</summary>
		<author><name>J.williams</name></author>
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