The Cassini spacecraft began detecting these radio emissions in April 2002, when Cassini was 374 million kilometers (234 million miles) from the planet, using the Cassini radio and plasma wave science instrument. The radio and plasma wave instrument has now provided the first high resolution observations of these emissions, showing an amazing array of variations in frequency and time. The complex radio spectrum with rising and falling tones, is very similar to Earth's auroral radio emissions. These structures indicate that there are numerous small radio sources moving along magnetic field lines threading the auroral region.
Time on this recording has been compressed, so that 73 seconds corresponds to 27 minutes. Since the frequencies of these emissions are well above the audio frequency range, we have shifted them downward by a factor of 44.
Link : http://www.nasa.gov/mission_pages/cassini/multimedia/pia07966.html
Sound file link : http://www.nasa.gov/wav/123163main_cas-skr1-112203.wav
Sound file link : http://www.nasa.gov/wav/123163main_cas-skr1-112203.wav
Great find, Joe!
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