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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 Apr 27 2012, 05:23 AM
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CL1 UV3 views of Titan from April 8 and April 23 are blink compared below. The banding high in the atmosphere shows no striking changes in these images from about 1.8M km. Slight changes reflect spacecraft movement, Titan rotation, sun angle to camera and imaging processing differences I would think.
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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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