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Article Images
Titan’s mysterious radio wave
 
1 June 2007

Titan’s full disk
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 HI-RES JPG (Size: 268 kb)  HI-RES TIFF (Size: 3555 kb)
Composite view of Titan built thanks to Cassini's images taken on 9 October and 25 October 2006.

Credits: NASA/JPL/University of Arizona
 
 
Sketch of radio wave detected during Huygens' descent
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 HI-RES JPEG (Size: 596 kb)
The Permittivity, Waves and Altimetry (PWA) sensor on the Huygens Atmosphere Structure Instrument (HASI) detected an extremely low frequency (ELF) radio wave during the descent. It was oscillating very slowly for a radio wave, just 36 times a second, and increased slightly in frequency as the probe reached lower altitudes.

This sketch illustrates how the radio wave, (if the PWA team confirms that the signal is a natural phenomenon and not an artefact of the way the instrument worked) could provide a powerful new way to probe not just the atmosphere of Titan but its subsurface as well. In fact, the wave could have been reflected by a liquid-ice boundary of a subsurface ocean of water and ammonia predicted by theoretical models.

Credits: ESA/Obs. De Paris Meudon/CETP-IPSL

 
 
Graph of electron density in Titan's atmosphere
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This graph plots the density of electrons in Titan’s atmosphere versus altitude, as obtained from the HASI instrument on board Huygens. The density of electrons is related to the electrical conductivity in the atmosphere.

Credits: ESA/Obs. De Paris Meudon/CETP-IPSL
 


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