|Earth Proton Whistlers|
A proton whistler can only be detected in spacecraft measurements above Earth's ionosphere. The proton whistler will occur immediately after an upward-propagating whistler has been generated by a lightning discharge. It is distinct from the more common, lightning-generated whistler both in tone and spectral characteristics.
Unlike the lightning-generated whistler, the proton whistler consists of a long, slowly rising tone that begins at a low frequency and levels off in a monotone at a frequency just below the proton cyclotron frequency, a characteristic frequency of the ambient plasma. The tone will typically last several seconds.
This example is from the University of Iowa Injun 3 spacecraft.
You can also view an AVI version of the video.
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The Radio and Plasma Wave Group, Department of Physics & Astronomy, College of Liberal Arts & Sciences.