Some approach images from T114 are shown superimposed on the images from the Ciclops looking ahead website http://www.ciclops.org/view/8225/Rev225?js=1 and the new ISS Titan map found in Photojournal here http://photojournal.jpl.nasa.gov/catalog/PIA19658 . From east to west, four of the narrow angle camera images initially centered on Mt Doom and Sotra Patera are shown below. N00250904-9 appears to show the Sotra Patera area and Mt Doom in some detail.
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Edited images N00250904 and N00250909 from T114 worked into the new 2015 ISS map are overlain with a portion of the T25 SAR http://pirlwww.lpl.arizona.edu/~perry/RADA...5_V01_part1.jpg that nicely covered the Doom mons-Sotra patera-Mohini fluctus area. The lobate structure of Mohini shows quite well in the two NAC images. Mohini seems to show some differences in the lobate flow structure (? age related) in the T25 SAR.
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VIMS Titan view from T114 is now posted on the Planetary Photojournal as PIA20016:

Thanks for the img resize whoever did that

Great mosaic, VIMS Jason. Glad you guys got some excellent data from your ride-along observation with us.

For the curious, the ISS HIRES observation was designed as a WAC mosaic as we flew by Cassini (NACs would have been much too blurry). VIMS has a smaller FOV than the WAC, so their best images from this encounter, seen on the left side of their full-disk mosaic, were discontinuous.