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	<title>HiBlog: HiRISE Team Blog &#187; TDI</title>
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	<link>http://hirise.lpl.arizona.edu/HiBlog</link>
	<description>High Resolution Imaging Science Experiment</description>
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		<title>Time-Delayed Identification</title>
		<link>http://hirise.lpl.arizona.edu/HiBlog/2008/07/10/time-delayed-identification/</link>
		<comments>http://hirise.lpl.arizona.edu/HiBlog/2008/07/10/time-delayed-identification/#comments</comments>
		<pubDate>Thu, 10 Jul 2008 23:13:20 +0000</pubDate>
		<dc:creator>Ingrid Daubar</dc:creator>
				<category><![CDATA[Camera specs]]></category>
		<category><![CDATA[HiRISE]]></category>
		<category><![CDATA[Phoenix]]></category>
		<category><![CDATA[Special Images]]></category>
		<category><![CDATA[Technical]]></category>
		<category><![CDATA[CCD]]></category>
		<category><![CDATA[descent]]></category>
		<category><![CDATA[EDL]]></category>
		<category><![CDATA[heat shield]]></category>
		<category><![CDATA[parachute]]></category>
		<category><![CDATA[TDI]]></category>

		<guid isPermaLink="false">http://hirise.lpl.arizona.edu/HiBlog/?p=196</guid>
		<description><![CDATA[ Our latest release includes more products from the original Phoenix descent observation, which include the color CCDs hand-mosaicked over the red filter CCDs.  We&#8217;ve also been working with the Phoenix and MRO engineering teams to identify the location of the heat shield in the image (left).  It&#8217;s pretty incredible that we caught [...]]]></description>
			<content:encoded><![CDATA[<p><a href="http://hirise.lpl.arizona.edu/images/2008/details/cut/PSP_008579_9020-B_cut_a.jpg"><img src="http://hirise.lpl.arizona.edu/images/2008/details/cut/PSP_008579_9020-B_cut_a.jpg" alt="Phoenix heat shield" height=150 ALIGN="left" /></a> Our latest release includes <a href="http://hirise.lpl.arizona.edu/phoenix-descent-color.php">more products</a> from the original Phoenix <a href="http://hirise.lpl.arizona.edu/phoenix-descent.php">descent observation</a>, which include the color CCDs hand-mosaicked over the red filter CCDs.  We&#8217;ve also been working with the Phoenix and MRO engineering teams to identify the location of the heat shield in the image (left).  It&#8217;s pretty incredible that we caught the lander just after releasing the heat shield &#8211; a few more seconds, and it would have been out of the scene.</p>
<p>Emily Lakdawalla continues her excellent <a href="http://www.planetary.org/blog/">blog</a> coverage in <a href="http://www.planetary.org/blog/article/00001547/">this article</a>, which does a great job of explaining some of the reasons why this image was especially difficult to take.  Along the way, she includes a tutorial on TDI (Time-Delay-Integration), written by one of the engineers that helped build the instrument.  TDI is the method HiRISE uses to gather lots of light into its CCDs, and it&#8217;s one of the reasons we get such high <a href="http://en.wikipedia.org/wiki/Signal-to-noise_ratio">signal-to-noise</a> in our images.  It&#8217;s a complicated concept, but it&#8217;s an important one for understanding HiRISE&#8217;s incredible imaging abilities, as well as its limitations.  </p>
<p>From her blog post:</p>
<blockquote><p>
This is a fascinating story showing how necessary it sometimes is to have a deep understanding of an instrument in order to understand the data that comes from it. &#8230;It can be dangerous to read too much into space images until you have studied how the cameras really work.
</p></blockquote>
<p>It&#8217;s a great post &#8211; <i>she</i> deserves a cookie!  <img src='http://hirise.lpl.arizona.edu/HiBlog/wp-includes/images/smilies/icon_smile.gif' alt=':)' class='wp-smiley' /> </p>
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		<item>
		<title>Image Fest #3</title>
		<link>http://hirise.lpl.arizona.edu/HiBlog/2008/03/18/image-fest-3/</link>
		<comments>http://hirise.lpl.arizona.edu/HiBlog/2008/03/18/image-fest-3/#comments</comments>
		<pubDate>Tue, 18 Mar 2008 17:29:42 +0000</pubDate>
		<dc:creator>GuyMac</dc:creator>
				<category><![CDATA[Color]]></category>
		<category><![CDATA[HiRISE]]></category>
		<category><![CDATA[Images & Science]]></category>
		<category><![CDATA[Interesting images]]></category>
		<category><![CDATA[1500]]></category>
		<category><![CDATA[CCD]]></category>
		<category><![CDATA[dune field]]></category>
		<category><![CDATA[dune fields]]></category>
		<category><![CDATA[geometry]]></category>
		<category><![CDATA[Glow]]></category>
		<category><![CDATA[off-nadir]]></category>
		<category><![CDATA[polygons]]></category>
		<category><![CDATA[projection]]></category>
		<category><![CDATA[PSP]]></category>
		<category><![CDATA[roll angle]]></category>
		<category><![CDATA[TDI]]></category>
		<category><![CDATA[Viking]]></category>
		<category><![CDATA[Viking Lander]]></category>
		<category><![CDATA[Viking Lander 1]]></category>
		<category><![CDATA[Viking Lander 2]]></category>
		<category><![CDATA[VL1]]></category>
		<category><![CDATA[VL2]]></category>

		<guid isPermaLink="false">http://hirise.lpl.arizona.edu/HiBlog/?p=162</guid>
		<description><![CDATA[Here are 40 RGB color images from the 1500 &#8211; 1600 orbit range of MRO.
View Images
There are, as always, many magnificent images here. Some of the noteworthy observations are:
PSP_001521_2025 and PSP_001501_2280: On the HiRISE web site you can see diagrams made by Tim Parker show the locations of various parts (lander, backshell, heatshield or parachute) [...]]]></description>
			<content:encoded><![CDATA[<p>Here are 40 RGB color images from the 1500 &#8211; 1600 orbit range of MRO.</p>
<p><a href="/HiBlog/wp-content/uploads/psp_0015.html">View Images</a></p>
<p>There are, as always, many magnificent images here. Some of the noteworthy observations are:</p>
<p><a href="/HiBlog/wp-content/uploads/psp_0015.html#PSP_001521_2025">PSP_001521_2025</a> and <a href="/HiBlog/wp-content/uploads/psp_0015.html#PSP_001501_2280">PSP_001501_2280</a>: On the HiRISE web site you can see diagrams made by Tim Parker show the locations of various parts (lander, backshell, heatshield or parachute) for <a href="/PSP_001521_2025">Viking Lander 1</a> and <a href="/PSP_001501_2280">Viking Lander 2</a>. It&#8217;s possible they aren&#8217;t in the color strip (I haven&#8217;t found them)!</p>
<p><a href="/HiBlog/wp-content/uploads/psp_0015.html#PSP_001508_1245">PSP_001508_1245</a> and <a href="/HiBlog/wp-content/uploads/psp_0015.html#PSP_001510_2195">PSP_001510_2195</a>: These two exhibit a &#8220;glow&#8221; pattern of saturated pixels due to high TDI (Time Delay Integration) settings on the blue-green CCDs. (All of the exposure settings are chosen for each observation based on a photometric model of the scene).</p>
<p><a href="/HiBlog/wp-content/uploads/psp_0015.html#PSP_001538_2035">PSP_001538_2035</a>: This is a rim-to-rim section across a crater called Tooting that is about 30 kilometers in diameter. It&#8217;s also interesting to note how the altitude of the rims, when combined with the large off-nadir roll angle (23 degrees), leads to an <a href="http://hirise-pds.lpl.arizona.edu/PDS/EXTRAS/RDR/PSP/ORB_001500_001599/PSP_001538_2035/PSP_001538_2035_COLOR.abrowse.jpg">oddly bowed geometric projection</a>. But it is correct; as the terrain rose, fell, and rose again from HiRISE&#8217;s angled point of view, the center of the ground track deviated slightly east or west from a true great-circle line.</p>
<p><a href="/HiBlog/wp-content/uploads/psp_0015.html#PSP_001558_1325">PSP_001558_1325</a> and <a href="/HiBlog/wp-content/uploads/psp_0015.html#PSP_001593_2635">PSP_001593_2635</a>: These dune fields are striking, forming incredible patterns.</p>
<p><a href="/HiBlog/wp-content/uploads/psp_0015.html#PSP_001582_2245">PSP_001582_2245</a>: Looking like a super-sized area of dried mud, the polygonal cracks in this image are amazing.</p>
<p><strong>Updated (2008-Apr-10)</strong></p>
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