Difference between revisions of "October 25, 2009"

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<em>image by [mailto:revans_01420@yahoo.com Rick Evans]</em><br />
 
<em>image by [mailto:revans_01420@yahoo.com Rick Evans]</em><br />
 
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I created this image of [http://www.lpod.org/archive/2004/03/LPOD-2004-03-02.htm Mons Hansteen], a lunar [http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1975LPICo.234..189W&amp;amp;data_type=PDF_HIGH&amp;amp;whole_paper=YES&amp;amp;type=PRINTER&amp;amp;filetype=.pdf red spot], by performing principal component image analysis (PCA) on the five Clementine UVVIS multispectral band images (i.e. 415, 750, 900, 950 and 1000 nm).  PCA is a tool sometimes used in multispectral geology [http://rst.gsfc.nasa.gov/Sect5/Sect5_3.html studies] to reveal variations in mineral composition. Using <em>Photoshop</em> the Clementine images were loaded respectively into five alpha channels of a color image with the R, G and B channels deleted.  With all alpha channels selected, [http://reindeergraphics.com/index.php?option=com_content&amp;task=view&amp;id=24&amp;Itemid=47 FoveaPro 4.0] software was used to create a PCA transform and then to transform the alpha channel images into their respective principal component images.  The first three resulting PCA images were then loaded respectively into the R, G and B channels of a color image producing the final image shown above.  Mons Hansteen and all other lunar red spot features show up with a very distinctive reddish hue in such images. Lunar red spots seem to absorb preferentially in the ultraviolet region of the spectrum compared to the visible; other lunar mafic features including the central peaks of Tycho are fascinating to observe with this technique as well.  <br />
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I created this image of [[March_2,_2004|Mons Hansteen]], a lunar [http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1975LPICo.234..189W&amp;amp;data_type=PDF_HIGH&amp;amp;whole_paper=YES&amp;amp;type=PRINTER&amp;amp;filetype=.pdf red spot], by performing principal component image analysis (PCA) on the five Clementine UVVIS multispectral band images (i.e. 415, 750, 900, 950 and 1000 nm).  PCA is a tool sometimes used in multispectral geology [http://rst.gsfc.nasa.gov/Sect5/Sect5_3.html studies] to reveal variations in mineral composition. Using <em>Photoshop</em> the Clementine images were loaded respectively into five alpha channels of a color image with the R, G and B channels deleted.  With all alpha channels selected, [http://reindeergraphics.com/index.php?option=com_content&amp;task=view&amp;id=24&amp;Itemid=47 FoveaPro 4.0] software was used to create a PCA transform and then to transform the alpha channel images into their respective principal component images.  The first three resulting PCA images were then loaded respectively into the R, G and B channels of a color image producing the final image shown above.  Mons Hansteen and all other lunar red spot features show up with a very distinctive reddish hue in such images. Lunar red spots seem to absorb preferentially in the ultraviolet region of the spectrum compared to the visible; other lunar mafic features including the central peaks of Tycho are fascinating to observe with this technique as well.  <br />
 
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<em>[mailto:revans_01420@yahoo.com Rick Evans]</em><br />
 
<em>[mailto:revans_01420@yahoo.com Rick Evans]</em><br />
 
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<strong>Lunar History Note:</strong> Today is the  184th birthday of <em>perhaps</em> the greatest selenographer of the 19th century -[http://lpod.wikispaces.com/September+14,+2009 J.F. Julius Schmidt] (1825-1884). Thanks to [http://todayinastronomy.blogspot.com/2009/02/february-7-johann-friedrich-julius.html Mark Tillotson] for the reminder!<br />
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<strong>Lunar History Note:</strong> Today is the  184th birthday of <em>perhaps</em> the greatest selenographer of the 19th century -[http://www2.lpod.org/wiki/September_14,_2009 J.F. Julius Schmidt] (1825-1884). Thanks to [http://todayinastronomy.blogspot.com/2009/02/february-7-johann-friedrich-julius.html Mark Tillotson] for the reminder!<br />
 
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<strong>Related Links</strong><br />
 
<strong>Related Links</strong><br />
Rükl plate [http://the-moon.wikispaces.com/R%C3%BCkl+40 40]<br />
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Rükl plate [https://the-moon.us/wiki/R%C3%BCkl_40 40]<br />
 
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<p><b>Yesterday's LPOD:</b> [[October 24, 2009|Das Mystery]] </p>
 
<p><b>Yesterday's LPOD:</b> [[October 24, 2009|Das Mystery]] </p>

Latest revision as of 08:35, 28 October 2018

Red Arrowhead

LPOD-Oct25-09.jpg
image by Rick Evans

I created this image of Mons Hansteen, a lunar red spot, by performing principal component image analysis (PCA) on the five Clementine UVVIS multispectral band images (i.e. 415, 750, 900, 950 and 1000 nm). PCA is a tool sometimes used in multispectral geology studies to reveal variations in mineral composition. Using Photoshop the Clementine images were loaded respectively into five alpha channels of a color image with the R, G and B channels deleted. With all alpha channels selected, FoveaPro 4.0 software was used to create a PCA transform and then to transform the alpha channel images into their respective principal component images. The first three resulting PCA images were then loaded respectively into the R, G and B channels of a color image producing the final image shown above. Mons Hansteen and all other lunar red spot features show up with a very distinctive reddish hue in such images. Lunar red spots seem to absorb preferentially in the ultraviolet region of the spectrum compared to the visible; other lunar mafic features including the central peaks of Tycho are fascinating to observe with this technique as well.

Rick Evans

Lunar History Note: Today is the 184th birthday of perhaps the greatest selenographer of the 19th century -J.F. Julius Schmidt (1825-1884). Thanks to Mark Tillotson for the reminder!

Related Links
Rükl plate 40

Yesterday's LPOD: Das Mystery

Tomorrow's LPOD: Wonder Rille



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