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- W1571551237 abstract "With ISEE 3 and WIND data, we have studied cases where the solar wind density exceeded 30 cm−3 at two different phases of the solar cycle, and a distinct pattern emerges. Superposed on the broad regions of elevated density in the slow flow are minutes-to-hours-long density peaks of pressure balance structures. Most of the high-density events result from intensification of these pressure balance structures owing to compression over a day-long time scale, usually in the sheaths of ejecta at solar maximum and in corotating interaction regions at solar minimum. The data indicate that the pressure balance structures have a transient source." @default.
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- W1571551237 date "1999-01-01" @default.
- W1571551237 modified "2023-10-16" @default.
- W1571551237 title "Density enhancements in the solar wind" @default.
- W1571551237 doi "https://doi.org/10.1063/1.58703" @default.
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