Difference between revisions of "May 25, 2005"

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=An IR Strip Across a Kipuka=
 
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    <tr><td><div align="center" class="main_sm">Image Credit: [mailto:pjstooke@uwo.ca Phil Stooke]</p>
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<tr><td><div align="center" class="main_sm">Image Credit: [mailto:pjstooke@uwo.ca Phil Stooke]</p>
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<p align="center"><b>An IR Strip Across a Kipuka</b></p>
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<p align="center"><b>An IR Strip Across a Kipuka</b></p>
<p align="left">What can you do when the Moon is hidden by clouds? Explore it with Clementine images! This image shows the kipuka (old surface surrounded by younger lavas) north of Menelaus, illustrated in LPOD on May 14. The vertical image strip is a mosaic of eleven Clementine long wavelength infrared (LWIR) images downloaded from NASA's Planetary Image Atlas.  The original images are impossible to recognize, all useful details are lost in a sea of noise. But by averaging and subtracting the noise, the moon's surface is revealed. Because this is thermal infrared, warm surfaces (darker or facing the sun) are bright and cool surfaces (brighter or facing away from the sun) are dark. Small craters with dark surroundings are in reality fresh bright-ejecta craters. At the bottom we see the rough ejecta of Menelaus crater, and north of it the kipuka, split by a rille, rising above the surrounding plains. In most areas, these LWIR images are the highest resolution views from Clementine.</p>
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<p align="left">What can you do when the Moon is hidden by clouds? Explore it with Clementine images! This image shows the kipuka (old surface surrounded by younger lavas) north of Menelaus, illustrated in LPOD on May 14. The vertical image strip is a mosaic of eleven Clementine long wavelength infrared (LWIR) images downloaded from NASA's Planetary Image Atlas.  The original images are impossible to recognize, all useful details are lost in a sea of noise. But by averaging and subtracting the noise, the moon's surface is revealed. Because this is thermal infrared, warm surfaces (darker or facing the sun) are bright and cool surfaces (brighter or facing away from the sun) are dark. Small craters with dark surroundings are in reality fresh bright-ejecta craters. At the bottom we see the rough ejecta of Menelaus crater, and north of it the kipuka, split by a rille, rising above the surrounding plains. In most areas, these LWIR images are the highest resolution views from Clementine.</p>
<blockquote><p align="right">&#8212; [mailto:pjstooke@uwo.ca Phil Stooke]</blockquote>
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<blockquote><p align="right">&#8212; [mailto:pjstooke@uwo.ca Phil Stooke]</blockquote>
 
<p align="left"><p><b>Technical Details:</b><br>
 
<p align="left"><p><b>Technical Details:</b><br>
 
All processing done in Photoshop. Each frame is filtered to remove noise.  The frames are stacked and averaged, and the average frame is then subtracted from each individual image. The result is very bland, but with contrast enhancement and more noise removal this is the result. In the mosaic, overlapping areas are also merged to further reduce noise.</p>
 
All processing done in Photoshop. Each frame is filtered to remove noise.  The frames are stacked and averaged, and the average frame is then subtracted from each individual image. The result is very bland, but with contrast enhancement and more noise removal this is the result. In the mosaic, overlapping areas are also merged to further reduce noise.</p>
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[http://publish.uwo.ca/~pjstooke/ Phil Stooke's Website]
 
[http://publish.uwo.ca/~pjstooke/ Phil Stooke's Website]
 
<p align="left"><b>Tomorrow's LPOD: </b> A New Kind of DHC</p>
 
<p align="left"><b>Tomorrow's LPOD: </b> A New Kind of DHC</p>
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<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>  
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<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>  
[mailto:chuck@observingthesky.org Charles A. Wood]</p>
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[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
<p align="center" class="main_titles"><b>Technical Consultant:</b><br>
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<p align="center" class="main_titles"><b>Technical Consultant:</b><br>
[mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
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[mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
<p align="center" class="main_titles"><b>Contact Translator:</b><br>
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<p align="center" class="main_titles"><b>Contact Translator:</b><br>
[mailto:pablolonnie@yahoo.com.mx" class="one Pablo Lonnie Pacheco Railey]  (Es)<br>
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[mailto:pablolonnie@yahoo.com.mx" class="one Pablo Lonnie Pacheco Railey]  (Es)<br>
[mailto:chlegrand@free.fr" class="one Christian Legrand] (Fr)</p>
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[mailto:chlegrand@free.fr" class="one Christian Legrand] (Fr)</p>
<p align="center" class="main_titles"><b>[mailto:webuser@observingthesky.org Contact Webmaster]</b></p>
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<p align="center" class="main_titles"><b>[mailto:webuser@observingthesky.org Contact Webmaster]</b></p>
<p align="center" class="main_titles"><b>A service of:</b><br>
+
<p align="center" class="main_titles"><b>A service of:</b><br>
[http://www.observingthesky.org/" class="one ObservingTheSky.Org]</p>
+
[http://www.observingthesky.org/" class="one ObservingTheSky.Org]</p>
<p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
+
<p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
[http://antwrp.gsfc.nasa.gov/apod/astropix.html" class="one Astronomy] | [http://www.msss.com/" class="one Mars] | [http://epod.usra.edu/" class="one Earth]</p>
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[http://antwrp.gsfc.nasa.gov/apod/astropix.html" class="one Astronomy] | [http://www.msss.com/" class="one Mars] | [http://epod.usra.edu/" class="one Earth]</p>
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<p>&nbsp;</p>
 
<p>&nbsp;</p>
 
 
 
 
 
----
 
----
 
===COMMENTS?===  
 
===COMMENTS?===  
 
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.
 
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.

Revision as of 18:32, 4 January 2015

An IR Strip Across a Kipuka

<nobr>An IR Strip Across a Kipuka</nobr>

<img src="archive/2005/05/images/LPOD-2005-05-25.jpeg" border="0">

Image Credit: Phil Stooke


An IR Strip Across a Kipuka

What can you do when the Moon is hidden by clouds? Explore it with Clementine images! This image shows the kipuka (old surface surrounded by younger lavas) north of Menelaus, illustrated in LPOD on May 14. The vertical image strip is a mosaic of eleven Clementine long wavelength infrared (LWIR) images downloaded from NASA's Planetary Image Atlas. The original images are impossible to recognize, all useful details are lost in a sea of noise. But by averaging and subtracting the noise, the moon's surface is revealed. Because this is thermal infrared, warm surfaces (darker or facing the sun) are bright and cool surfaces (brighter or facing away from the sun) are dark. Small craters with dark surroundings are in reality fresh bright-ejecta craters. At the bottom we see the rough ejecta of Menelaus crater, and north of it the kipuka, split by a rille, rising above the surrounding plains. In most areas, these LWIR images are the highest resolution views from Clementine.

Phil Stooke

Technical Details:
All processing done in Photoshop. Each frame is filtered to remove noise. The frames are stacked and averaged, and the average frame is then subtracted from each individual image. The result is very bland, but with contrast enhancement and more noise removal this is the result. In the mosaic, overlapping areas are also merged to further reduce noise.

Related Links:
Phil Stooke's Website

Tomorrow's LPOD: A New Kind of DHC



Author & Editor:
Charles A. Wood

Technical Consultant:
Anthony Ayiomamitis

Contact Translator:
" class="one Pablo Lonnie Pacheco Railey (Es)
" class="one Christian Legrand (Fr)

Contact Webmaster

A service of:
" class="one ObservingTheSky.Org

Visit these other PODs:
" class="one Astronomy | " class="one Mars | " class="one Earth

 


COMMENTS?

Click on this icon File:PostIcon.jpg at the upper right to post a comment.