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		<id>http://ed560.ipgp.fr/index.php?title=Descriptif_ED1819-SU11_Surfaces&amp;diff=15980&amp;oldid=prev</id>
		<title>Ridel le 17 septembre 2018 à 12:18</title>
		<link rel="alternate" type="text/html" href="http://ed560.ipgp.fr/index.php?title=Descriptif_ED1819-SU11_Surfaces&amp;diff=15980&amp;oldid=prev"/>
				<updated>2018-09-17T12:18:09Z</updated>
		
		<summary type="html">&lt;p&gt;&lt;/p&gt;

		&lt;table style=&quot;background-color: white; color:black;&quot;&gt;
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		&lt;td colspan='2' style=&quot;background-color: white; color:black;&quot;&gt;← Version précédente&lt;/td&gt;
		&lt;td colspan='2' style=&quot;background-color: white; color:black;&quot;&gt;Version du 17 septembre 2018 à 12:18&lt;/td&gt;
		&lt;/tr&gt;
		&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Ligne 5 :&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Ligne 5 :&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background: #eee; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;- salle à venir&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background: #eee; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;- salle à venir&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: #eee; color:black; font-size: smaller;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background: #eee; color:black; font-size: smaller;&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: #ffa; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;Characterizing natural surfaces: remote observations, modeling and inversion&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;background: #cfc; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;&amp;lt;SPAN STYLE=&amp;quot;background-color: #ffffcc;font-weight:bold&amp;quot;&amp;gt; &lt;/ins&gt;Characterizing natural surfaces: remote observations, modeling and inversion&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;&amp;lt;/span&amp;gt;&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: #eee; color:black; font-size: smaller;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background: #eee; color:black; font-size: smaller;&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: #eee; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;Remote sensing of planetary surfaces by satellites or spacecraft provides important clues on their properties, at global scale or/and high spatial resolution. They help following their structural and temporal evolution over days or years which may impact human activities and conditions of living or provide unique knowledge on unexplored extraterrestrial surfaces. Radiances originating from various depths in the near surface and measured over a large range of wavelengths, directions and timescales are modulated by its structure and composition. Heat and radiative transfer models have been developed to infer these properties from radiances. &amp;nbsp;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background: #eee; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;Remote sensing of planetary surfaces by satellites or spacecraft provides important clues on their properties, at global scale or/and high spatial resolution. They help following their structural and temporal evolution over days or years which may impact human activities and conditions of living or provide unique knowledge on unexplored extraterrestrial surfaces. Radiances originating from various depths in the near surface and measured over a large range of wavelengths, directions and timescales are modulated by its structure and composition. Heat and radiative transfer models have been developed to infer these properties from radiances. &amp;nbsp;&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: #eee; color:black; font-size: smaller;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background: #eee; color:black; font-size: smaller;&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: #eee; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;This course aims at delivering skills in multi-wavelengths remote sensing and modeling of natural surfaces and at training participants in data inversion of satellite/spacecraft data from visible to the thermal/microwave infrared domain. It will be delivered in the form of 10h (5 x 2h) of main lessons, merged with a training session (15h=5*3h). This will consist of characterizing the properties of a specific surface among various solar system bodies such as the Moon, icy satellites of Saturn, etc, using databases from NASA missions mainly. This training includes data manipulation, model study (sensitivity analysis,...) and data inversion based on Bayesian inference under Python environment.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background: #eee; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;This course aims at delivering skills in multi-wavelengths remote sensing and modeling of natural surfaces and at training participants in data inversion of satellite/spacecraft data from visible to the thermal/microwave infrared domain. It will be delivered in the form of 10h (5 x 2h) of main lessons, merged with a training session (15h=5*3h). This will consist of characterizing the properties of a specific surface among various solar system bodies such as the Moon, icy satellites of Saturn, etc, using databases from NASA missions mainly. This training includes data manipulation, model study (sensitivity analysis,...) and data inversion based on Bayesian inference under Python environment.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;!-- diff generator: internal 2026-05-04 06:15:16 --&gt;
&lt;/table&gt;</summary>
		<author><name>Ridel</name></author>	</entry>

	<entry>
		<id>http://ed560.ipgp.fr/index.php?title=Descriptif_ED1819-SU11_Surfaces&amp;diff=15978&amp;oldid=prev</id>
		<title>Ridel le 17 septembre 2018 à 12:16</title>
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				<updated>2018-09-17T12:16:46Z</updated>
		
		<summary type="html">&lt;p&gt;&lt;/p&gt;

		&lt;table style=&quot;background-color: white; color:black;&quot;&gt;
		&lt;col class='diff-marker' /&gt;
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		&lt;col class='diff-content' /&gt;
		&lt;tr valign='top'&gt;
		&lt;td colspan='2' style=&quot;background-color: white; color:black;&quot;&gt;← Version précédente&lt;/td&gt;
		&lt;td colspan='2' style=&quot;background-color: white; color:black;&quot;&gt;Version du 17 septembre 2018 à 12:16&lt;/td&gt;
		&lt;/tr&gt;
		&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Ligne 1 :&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Ligne 1 :&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;-&lt;/td&gt;&lt;td style=&quot;background: #ffa; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;- durée total des cours : &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;30 &lt;/del&gt;h&amp;lt;BR&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;background: #cfc; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;- durée total des cours : &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;25 &lt;/ins&gt;h&amp;lt;BR&amp;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: #ffa; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;- &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;5 matinées (9h30&lt;/del&gt;-&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;12h30) &lt;/del&gt;et &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;5 après-midis (14h&lt;/del&gt;-&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;17h) du 7 au 11 janvier 2018 au laboratoire &lt;/del&gt;[http://www.apc.univ-paris7.fr/APC_CS/fr/acces-contact &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;APC&lt;/del&gt;]&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;,&amp;lt;BR&amp;gt; salles 302A.&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;background: #cfc; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;- &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;avril ou juin 2019, mise à jour à venir rapidement&amp;lt;BR&amp;gt;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;nbsp;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;background: #cfc; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;- &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;15h de travaux pratiques en salle informatique &lt;/ins&gt;et &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;10h de cours magistral&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;nbsp;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;background: #cfc; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;- &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;batiment &lt;/ins&gt;[http://www.apc.univ-paris7.fr/APC_CS/fr/acces-contact &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Condorcet&lt;/ins&gt;] &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;de l'Université Paris Diderot&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;nbsp;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;background: #cfc; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;- salle à venir&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: #eee; color:black; font-size: smaller;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background: #eee; color:black; font-size: smaller;&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: #eee; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;Characterizing natural surfaces: remote observations, modeling and inversion&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background: #eee; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;Characterizing natural surfaces: remote observations, modeling and inversion&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: #eee; color:black; font-size: smaller;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background: #eee; color:black; font-size: smaller;&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: #ffa; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;Remote sensing of planetary surfaces by satellites or spacecraft provides important clues on their properties, at global scale or/and high spatial resolution. They help following their structural and temporal evolution over days or years which may impact human activities and conditions of living or provide unique knowledge on unexplored extraterrestrial surfaces. Radiances originating from various depths in the near surface and measured over a large range of wavelengths, directions and timescales are modulated by its structure and composition. Heat and radiative transfer models have been developed to infer these properties from radiances. This course aims at delivering skills in multi-wavelengths remote sensing and modeling of natural surfaces and at training participants in data inversion of satellite/spacecraft data from visible to the thermal/microwave infrared domain. It will be delivered in the form of &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;12h &lt;/del&gt;(&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;4 &lt;/del&gt;x &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;3h&lt;/del&gt;) of main lessons, merged with a training session (15h=5*3h). This will consist of characterizing the properties of a specific surface among various solar system bodies such as the Moon, icy satellites of Saturn, etc, using databases from NASA missions mainly. This training includes data manipulation, model study (sensitivity analysis,...) and data inversion based on Bayesian inference under Python environment.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;background: #cfc; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;Remote sensing of planetary surfaces by satellites or spacecraft provides important clues on their properties, at global scale or/and high spatial resolution. They help following their structural and temporal evolution over days or years which may impact human activities and conditions of living or provide unique knowledge on unexplored extraterrestrial surfaces. Radiances originating from various depths in the near surface and measured over a large range of wavelengths, directions and timescales are modulated by its structure and composition. Heat and radiative transfer models have been developed to infer these properties from radiances. &amp;nbsp;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;nbsp;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;background: #cfc; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;&amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;nbsp;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;background: #cfc; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;This course aims at delivering skills in multi-wavelengths remote sensing and modeling of natural surfaces and at training participants in data inversion of satellite/spacecraft data from visible to the thermal/microwave infrared domain. It will be delivered in the form of &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;10h &lt;/ins&gt;(&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;5 &lt;/ins&gt;x &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;2h&lt;/ins&gt;) of main lessons, merged with a training session (15h=5*3h). This will consist of characterizing the properties of a specific surface among various solar system bodies such as the Moon, icy satellites of Saturn, etc, using databases from NASA missions mainly. This training includes data manipulation, model study (sensitivity analysis,...) and data inversion based on Bayesian inference under Python environment.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;!-- diff generator: internal 2026-05-04 06:15:16 --&gt;
&lt;/table&gt;</summary>
		<author><name>Ridel</name></author>	</entry>

	<entry>
		<id>http://ed560.ipgp.fr/index.php?title=Descriptif_ED1819-SU11_Surfaces&amp;diff=15977&amp;oldid=prev</id>
		<title>Ridel le 17 septembre 2018 à 12:11</title>
		<link rel="alternate" type="text/html" href="http://ed560.ipgp.fr/index.php?title=Descriptif_ED1819-SU11_Surfaces&amp;diff=15977&amp;oldid=prev"/>
				<updated>2018-09-17T12:11:12Z</updated>
		
		<summary type="html">&lt;p&gt;&lt;/p&gt;

		&lt;table style=&quot;background-color: white; color:black;&quot;&gt;
		&lt;col class='diff-marker' /&gt;
		&lt;col class='diff-content' /&gt;
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		&lt;col class='diff-content' /&gt;
		&lt;tr valign='top'&gt;
		&lt;td colspan='2' style=&quot;background-color: white; color:black;&quot;&gt;← Version précédente&lt;/td&gt;
		&lt;td colspan='2' style=&quot;background-color: white; color:black;&quot;&gt;Version du 17 septembre 2018 à 12:11&lt;/td&gt;
		&lt;/tr&gt;
		&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Ligne 1 :&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Ligne 1 :&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;nbsp;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;background: #cfc; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;color: red; font-weight: bold; text-decoration: none;&quot;&gt;- durée total des cours : 30 h&amp;lt;BR&amp;gt;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;nbsp;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;background: #cfc; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;color: red; font-weight: bold; text-decoration: none;&quot;&gt;- 5 matinées (9h30-12h30) et 5 après-midis (14h-17h) du 7 au 11 janvier 2018 au laboratoire [http://www.apc.univ-paris7.fr/APC_CS/fr/acces-contact APC],&amp;lt;BR&amp;gt; salles 302A.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;nbsp;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;background: #cfc; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;color: red; font-weight: bold; text-decoration: none;&quot;&gt;&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: #eee; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;Characterizing natural surfaces: remote observations, modeling and inversion&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background: #eee; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;Characterizing natural surfaces: remote observations, modeling and inversion&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: #eee; color:black; font-size: smaller;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background: #eee; color:black; font-size: smaller;&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: #eee; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;Remote sensing of planetary surfaces by satellites or spacecraft provides important clues on their properties, at global scale or/and high spatial resolution. They help following their structural and temporal evolution over days or years which may impact human activities and conditions of living or provide unique knowledge on unexplored extraterrestrial surfaces. Radiances originating from various depths in the near surface and measured over a large range of wavelengths, directions and timescales are modulated by its structure and composition. Heat and radiative transfer models have been developed to infer these properties from radiances. This course aims at delivering skills in multi-wavelengths remote sensing and modeling of natural surfaces and at training participants in data inversion of satellite/spacecraft data from visible to the thermal/microwave infrared domain. It will be delivered in the form of 12h (4 x 3h) of main lessons, merged with a training session (15h=5*3h). This will consist of characterizing the properties of a specific surface among various solar system bodies such as the Moon, icy satellites of Saturn, etc, using databases from NASA missions mainly. This training includes data manipulation, model study (sensitivity analysis,...) and data inversion based on Bayesian inference under Python environment.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background: #eee; color:black; font-size: smaller;&quot;&gt;&lt;div&gt;Remote sensing of planetary surfaces by satellites or spacecraft provides important clues on their properties, at global scale or/and high spatial resolution. They help following their structural and temporal evolution over days or years which may impact human activities and conditions of living or provide unique knowledge on unexplored extraterrestrial surfaces. Radiances originating from various depths in the near surface and measured over a large range of wavelengths, directions and timescales are modulated by its structure and composition. Heat and radiative transfer models have been developed to infer these properties from radiances. This course aims at delivering skills in multi-wavelengths remote sensing and modeling of natural surfaces and at training participants in data inversion of satellite/spacecraft data from visible to the thermal/microwave infrared domain. It will be delivered in the form of 12h (4 x 3h) of main lessons, merged with a training session (15h=5*3h). This will consist of characterizing the properties of a specific surface among various solar system bodies such as the Moon, icy satellites of Saturn, etc, using databases from NASA missions mainly. This training includes data manipulation, model study (sensitivity analysis,...) and data inversion based on Bayesian inference under Python environment.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;!-- diff generator: internal 2026-05-04 06:15:16 --&gt;
&lt;/table&gt;</summary>
		<author><name>Ridel</name></author>	</entry>

	<entry>
		<id>http://ed560.ipgp.fr/index.php?title=Descriptif_ED1819-SU11_Surfaces&amp;diff=15976&amp;oldid=prev</id>
		<title>Ridel&amp;nbsp;:&amp;#32;Page créée avec « Characterizing natural surfaces: remote observations, modeling and inversion  Remote sensing of planetary surfaces by satellites or spacecraft provides important clues on the… »</title>
		<link rel="alternate" type="text/html" href="http://ed560.ipgp.fr/index.php?title=Descriptif_ED1819-SU11_Surfaces&amp;diff=15976&amp;oldid=prev"/>
				<updated>2018-09-17T12:02:35Z</updated>
		
		<summary type="html">&lt;p&gt;Page créée avec « Characterizing natural surfaces: remote observations, modeling and inversion  Remote sensing of planetary surfaces by satellites or spacecraft provides important clues on the… »&lt;/p&gt;
&lt;p&gt;&lt;b&gt;Nouvelle page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;Characterizing natural surfaces: remote observations, modeling and inversion&lt;br /&gt;
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Remote sensing of planetary surfaces by satellites or spacecraft provides important clues on their properties, at global scale or/and high spatial resolution. They help following their structural and temporal evolution over days or years which may impact human activities and conditions of living or provide unique knowledge on unexplored extraterrestrial surfaces. Radiances originating from various depths in the near surface and measured over a large range of wavelengths, directions and timescales are modulated by its structure and composition. Heat and radiative transfer models have been developed to infer these properties from radiances. This course aims at delivering skills in multi-wavelengths remote sensing and modeling of natural surfaces and at training participants in data inversion of satellite/spacecraft data from visible to the thermal/microwave infrared domain. It will be delivered in the form of 12h (4 x 3h) of main lessons, merged with a training session (15h=5*3h). This will consist of characterizing the properties of a specific surface among various solar system bodies such as the Moon, icy satellites of Saturn, etc, using databases from NASA missions mainly. This training includes data manipulation, model study (sensitivity analysis,...) and data inversion based on Bayesian inference under Python environment.&lt;/div&gt;</summary>
		<author><name>Ridel</name></author>	</entry>

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