Titan weather studies feature large in plans for the November encounter. From the latest 'looking ahead':
Outbound, VIMS will control pointing, mapping Titan's surface and cloud features. ISS will take images during this flyby by riding along with other instruments' observations, so no large mosaics are planned. The ride-along images should be useful for cloud monitoring, and if present, the clouds' motions and development can be tracked. The area will have been covered by the October 29 distant observation for comparison. Follow-up observations on November 13 and 14 will allow researchers to track clouds in the two days following the encounter. These will also cover the area that was under the arrow storm a month and a half earlier. An important goal will be to detect signs of surface changes that resulted from flooding caused by the storm's torrential rains.
Probably conjectured but based on what happened after another large storm in late 2004 in the south polar region of Titan (see discussion and especially the photojournal link) here: http://photojournal.jpl.nasa.gov/catalog/PIA11147
My impression was the 2004 storm was a bit larger and thereafter frequent clouds remained over the s polar region which may have contributed additional precipitation. I would imagine many factors have to be considered (cloud heights, methane relative 'humidity', duration of the main storm cloud over a terrain, tropospheric winds, porosity and dryness of the terrain, state of any methanofers etc.) before predicting what might be seen on the ground in Senkyo (from last month's storm) in this T73 flyby. It will be exciting to see regardless!
One other question is whether any sign of flooding was seen on the ground after the April 2008 storm over S Belet?
Interesting. The clouds over Belet seem to stop pretty sharply at the west 'coast' of Adiri. Do well drained highlands dry out quickly whereas wetted dunes continue to exude cloud-forming vapours after the storm has passed?
Re rain detection: Any indication that they might try to do so?
I'd imagine that radar would be the only possible way to do this; there should be a pronounced attenuation of both the inbound & outbound pulses if they pass through a rainstorm.
It'd be a tough observation to get, though. You'd have to specifically target a suspected storm system, and I don't know if they can reshuffle an encounter timeline rapidly enough to react to storm formation.
Still, might be worth it. We could learn something useful about the composition of the rain; mostly methane, of course, but undoubtedly there would be trapped aerosols & other compounds as well that would modify its radar attenuation properties.
So now you know the source of the loud "http://www.nooooooooooooooo.com/" coming from the direction of Tucson, Arizona yesterday:
http://www.jpl.nasa.gov/news/news.cfm?release=2010-374
Engineers at NASA's Jet Propulsion Laboratory, Pasadena, Calif., are working to understand what caused NASA's Cassini spacecraft to put itself into "safe mode," a precautionary standby mode. Cassini entered safe mode around 4 p.m. PDT (7 p.m. EDT) on Tuesday, Nov. 2.
Since going into safe mode, the spacecraft has performed as expected, suspending the flow of science data and sending back only data about engineering and spacecraft health. Cassini is programmed to put itself into safe mode automatically any time it detects a condition on the spacecraft that requires action from mission controllers on the ground.
Engineers say it is not likely that Cassini will be able to resume full operations before a planned Nov. 11 flyby of Saturn's moon Titan. But Cassini has 53 more Titan flybys planned in its extended mission, which lasts until 2017.
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I had just started to get REALLY excited about T73.
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