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- W4243704024 abstract "Following each of three geomagnetic sudden commencements, ionospheric disturbances (ionospheric storms) are found to propagate from two isolated locations in high-latitude regions of the Earth. These two positions are conjugate points (magnetically), and are in different locations for each magnetic storm. Speeds of travel are 361 m/sec and 722 m/sec. Disturbances with the slower speed produce detectable effects on the ionosphere after encircling the Earth. I.G.Y. data (hourly values of h′F) from a world-wide station network were used and a superposed-epoch method employed. A study of ionograms from Australian stations during these and other magnetic storms supports the superposed-epoch results. It is shown that red arcs, certain auroral forms and v.l.f. electromagnetic emissions may be associated with these travelling disturbances." @default.
- W4243704024 created "2022-05-12" @default.
- W4243704024 date "1960-10-01" @default.
- W4243704024 modified "2023-09-26" @default.
- W4243704024 title "The sun's polar magnetic field" @default.
- W4243704024 doi "https://doi.org/10.1016/0038-092x(60)90023-2" @default.
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