By Scott Bachmeier •
The launch of a SpaceX Falcon Heavy rocket from the NASA Kennedy Space Center in Florida occurred at 2235 UTC on 11 April 2019. Warm thermal signatures of pockets of air (which had been superheated by the booster rocket exhaust) were seen northeast of the launch site in GOES-16 (GOES-East) Low-level Water Vapor (7.3 µm), Mid-level Water Vapor (6.9 µm), Upper-level Water Vapor (6.2 µm) and Shortwave Infrared (3.9 µm) images (above). In addition, closer to the launch site a (thermally-cooler) signature of the lower-altitude rocket exhaust condensation plume was evident — for example, see an annotated comparison of the 2236 UTC images below (GOES-16 was scanning that exact location at 22:37:22 UTC, a little more than 2 minutes after launch). Two portions of the lower-altitude rocket condensation plume — one moving northeastward, and one moving westward — were seen in higher-resolution GOES-16 “Red” Visible (0.64 µm) images (below). The different directions of rocket condensation plume motion were due to directional shear of wind within the lowest 2 km or 6500 feet of the atmosphere, as shown in a plot of 00 UTC rawinsonde data from Cape Canaveral, Florida (below). Similar signatures of other rocket launches have been seen using GOES-16 and GOES-17.Categories: GOES-16, Rocket signatures