Abstract
Spectra of complex Jovian S-storms can be interpreted as groups of tilted-V variants. In such an approach the basic components (wide-range S-bursts, narrow-range S-trains, emissions of type N, and shadow events) are arranged in a predictable sequence. It seems that the application of tilted-V variants offers some order for the chaos evident in many S-storm spectra.
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Riihimaa, J.J. Variants of tilted-V events in Jupiter's decametric radio spectra. Earth Moon Planet 48, 49–54 (1990). https://doi.org/10.1007/BF00115068
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DOI: https://doi.org/10.1007/BF00115068