Turbulence plays an important role in Earth’s weather system, and can be more than an inconvenience - hundreds of injuries have occurred on commercial flights due to turbulence. It is studied both in Earth's atmosphere and in that of Saturn's moon, Titan, aided by data from ESA’s Huygens probe. The study of one is helping the other.
Giles Harrison, atmospheric physicist at the University of Reading in the UK, devised an inexpensive way to measure the effects of turbulence using weather balloons. The instrument package contains a magnetic field sensor which measures fluctuations in Earth’s magnetic field due to turbulence. As Earth's magnetic field is very stable, the measurements of magnetic changes taken with the weather balloon showed the effects of turbulence on the sensor, since the balloon itself was moving very violently.
All bodies, planets and moons, are subject to the same principles of physics. So by working together, researchers looking at Earth and those looking at our planetary neighbours can really test their models of the processes taking place and gain new insights into both.
Planetary scientist Ralph Lorenz, at the Johns Hopkins University Applied Physics Laboratory in the USA, found Harrison's results key to making sense of data from Huygens, which descended by parachute through Titan's atmosphere in January 2005.
The Surface Science Package (SSP) on board Huygens included a set of tilt sensors which measured motions of the probe during its descent. These tilt sensors act much like a drink in a glass, using a small slug of liquid to measure the tilt angle.
As the probe plummeted under the parachute through Titan’s atmosphere, there was a lot of buffeting, even though the air itself was fairly still. Knowing the signature of cloud-induced turbulence in Harrison's balloon data from Earth inspired Lorenz to look for a similar effect in the Huygens data using the tilt sensor.
“Huygens’ tilt history was just this long, squiggly, complex mess, but seeing the fingerprint of cloud turbulence in Harrison's work showed me what to look for,” said Lorenz.
Armed with that information, Lorenz found that a 20-minute period of Huygens' 2.5-hour descent, around an altitude of 20 km, was affected by this kind of in-cloud turbulence. Having experimented with instrumentation on small models, even frisbees, to understand the dynamics of aerospace vehicles like the probe, Lorenz was familiar with the sensors used by Harrison.
Lorenz’s analysis helped identify a turbulent cloud layer in Titan’s atmosphere - a significant result for the investigation of Titan’s meteorology. In the process, he also found a way to improve Harrison's magnetic sensor arrangement on the weather balloon, simply by changing its orientation.
Mark Leese, Project Manager for the SSP on Huygens at The Open University said “We knew Huygens had a bumpy ride down to Titan’s surface. Now we can separate out twenty minutes of air turbulence – probably due to a cloud layer - from other effects such as cross winds or air buffeting due to the irregular shape of the probe.”
Article: ‘Descent motions of the Huygens probe as measured by the Surface Science Package (SSP): turbulent evidence for a cloud layer’, by R. Lorenz, J. Zarnecki, M. Towner, M. Leese, A. Ball, B. Hathi, A. Hagermann and N. Ghafoor, Planetary and Space Science journal.