Difference between revisions of "December 14, 2011"

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<em>image by [mailto:tosi.philippe@wanadoo.fr Philippe Tosi], Pic du Midi observatory, France</em><br />
 
<em>image by [mailto:tosi.philippe@wanadoo.fr Philippe Tosi], Pic du Midi observatory, France</em><br />
 
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High Dynamic Range (HDR) [http://www.hdrsoft.com/ software]combines multiple exposure [http://lpod.wikispaces.com/April+5%2C+2008 images] to highlight detail across the whole brightness range. Here Philippe applies it to a full Moon view of Tycho and its dark collar. This technique appears to bring out the individual raylets that often get visually fused into a confusing bright nexus. And it shows darker materials underlying the rays on the right side of the image. HDR imaging may be a new approach to detail mapping and ultimately characterizing and classifying lunar ray systems. <br />
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High Dynamic Range (HDR) [http://www.hdrsoft.com/ software]combines multiple exposure [http://www2.lpod.org/wiki/April_5,_2008 images] to highlight detail across the whole brightness range. Here Philippe applies it to a full Moon view of Tycho and its dark collar. This technique appears to bring out the individual raylets that often get visually fused into a confusing bright nexus. And it shows darker materials underlying the rays on the right side of the image. HDR imaging may be a new approach to detail mapping and ultimately characterizing and classifying lunar ray systems. <br />
 
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<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br />
 
<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><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+64 64]<br />
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Rükl plate [https://the-moon.us/wiki/R%C3%BCkl_64 64]<br />
 
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<p><b>Yesterday's LPOD:</b> [[December 13, 2011|Little Dots, Big Story]] </p>
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<p><b>Tomorrow's LPOD:</b> [[December 15, 2011|Tracing Back the Rays]] </p>
 
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Latest revision as of 08:25, 28 October 2018

Sorting Out the Rays

LPOD-Dec14-11.jpg
image by Philippe Tosi, Pic du Midi observatory, France

High Dynamic Range (HDR) softwarecombines multiple exposure images to highlight detail across the whole brightness range. Here Philippe applies it to a full Moon view of Tycho and its dark collar. This technique appears to bring out the individual raylets that often get visually fused into a confusing bright nexus. And it shows darker materials underlying the rays on the right side of the image. HDR imaging may be a new approach to detail mapping and ultimately characterizing and classifying lunar ray systems.

Chuck Wood

Technical Details
October, 2011. C.14 with Skynyx 2.1 M + IR filter 742nm. HDR Soft Photomatix 4 developped by HDRsoft Society, fusion of 3 expositions 0.08; 0.16 and 0.32 sec.

Related Links
Rükl plate 64

Yesterday's LPOD: Little Dots, Big Story

Tomorrow's LPOD: Tracing Back the Rays



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