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- W2024066095 abstract "It has been generally accepted up to now that giant pulsations (Pg) are auroral zone phenomena but here we present observations of a sequence of three Pg events on successive days at three stations well within the plasmasphere. Field line resonance behaviour is exhibited with one of the events clearly resonating at L ≅ 2.8. From the resonant frequency (10.4 mHz) equatorial mass densities are calculated and from these, and the measured azimuthai polarization at resonance, the inference is drawn that Pgs are oscillations in the fundamental guided poloidal mode. We suggest that the drift wave instability of the compressional Alfvén wave may be the source mechanism for Pgs and speculate how conditions for the instability may have arisen." @default.
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- W2024066095 date "1985-10-01" @default.
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- W2024066095 title "Giant pulsations in the plasmasphere" @default.
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- W2024066095 doi "https://doi.org/10.1016/0032-0633(85)90073-x" @default.
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