Abstract. Temporal characteristics of irregular magnetic pulsations and intervals of pulsations of diminishing periods (IPDP) plasma wave events observed in association with low-latitude auroras are reported. The two most significant issues are the particle spectrum associated with low-latitude auroras and convective growth rate modeling for the IPDP plasma wave events. In particular, it is shown that the growth rate is sensitive to variations in oxygen-ion kinetic energy in addition to movements of the source region. The frequency increase in the dynamic spectrum of a low-latitude IPDP plasma wave event can be explained in terms of the variation of the kinetic energy of the precipitating oxygen-ion stream during low-latitude auroras.
IntroductionAuroras commonly occur only in high latitudes, but at special times they become visible from places far beyond their usual limits. At these times, they are seen from middle and low latitudes, sometimes even from the tropics [Chapman, 1957]. In spite of the fact that Japan is not favorably situated to observe auroras, auroral displays have occasionally been seen in periods of high solar activity. Matsushita [1956] Although a number of optical observations of low-latitude auroras have been reported in the literature, none have as of yet given sufficient detail on the magnetic pulsation aspects of low-latitude auroras. In particular, it is necessary to investigate the irregular magnetic pulsations occurring during these auroras. In this paper, we refine and expand two previous papers,