Abstract
Almost a decade has passed since Gul'elmi and Dovbnya (1974) introduced the high latitude class of ultra low frequency (ULF) pulsations known as “Serpentine Emission” (SE). The purpose of this paper is twofold; firstly, to present new morphological results of SE observed at Davis, Antarctica and secondly, to stimulate further experimental and theoretical interest by pulsation researchers. Analyses presented include the first cited amplitude-time structure of SE along with maximum entropy power spectra and digital sonagrams. SE polarizations are investigated and a limited diurnal morphological survey is presented.
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