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Rev 164: Titan Monitoring Campaign
titanicrivers
post Apr 15 2012, 10:33 PM
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Some Titan images from the Rev 164 TMC sequence of April 8 from 1.8M km. RGB composite fading to a CL1 CB3 image reveals details of the upper atmosphere and surface centered on the Belet region. Images rotated so N is up.
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titanicrivers
post May 1 2012, 07:59 AM
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The second CL1 UV3 image VP mentions above now is in the raw images. Difference blending the two (on the left below) shows essentially no change other than slight apparent diameter difference due to Titan-spacecraft distance difference.
More interesting is the difference blending of the BL1 CL2 (blue light filter) with the UV filtered image (right image below) the latter showing details in a higher haze layer compared to the blue filter. These two images were from the same Titan spacecraft distance. Some artifact related to original image brightness may be present.
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- titanicrivers   Rev 164: Titan Monitoring Campaign   Apr 15 2012, 10:33 PM
- - brellis   Great sequence - easy to see why Mr. Lorenz titled...   Apr 16 2012, 02:50 AM
- - titanicrivers   Lots of upper atmosphere banding visible on the sh...   Apr 18 2012, 02:47 AM
- - titanicrivers   CL1 UV3 views of Titan from April 8 and April 23 a...   Apr 27 2012, 05:23 AM
- - volcanopele   Interesting comparison. Yeah, a lot of the faint ...   Apr 27 2012, 05:50 AM
- - titanicrivers   Thanks VP. The southern haze layers in the BL and...   Apr 27 2012, 07:38 AM
- - titanicrivers   The second CL1 UV3 image VP mentions above now is ...   May 1 2012, 07:59 AM

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