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- W2007687517 abstract "Six-hour segments of simultaneous solar wind plasma and interplanetary magnetic field data from RAP 8, WIND and 1NTERBALL-1 are used to compare correlations of the plasma and interplanetary magnetic field for the same solar wind structures. Magnetic field structures are, on average, as well-correlated as plasma structures. The averaged on large statistics cross-correlation coefficient is equal to 0.75 for ion flux and 0.71 for IMF magnitude comparison. But for many individual 6-hour segments the difference between plasma and IMF correlations is rather large. We find that good IMF correlations coincide with good plasma correlations 65% of the time but that good plasma correlations coincide with good IMF correlations only 44% of the time. Also the dependence of ion flux correlations on the IMF cone angle was studied for two sets of data. The plasma correlations increase as the IMF cone angle increases, suggesting plasma structures may be elongated parallel to the IMF." @default.
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- W2007687517 date "2000-01-01" @default.
- W2007687517 modified "2023-10-16" @default.
- W2007687517 title "Solar wind structure dynamics by multipoint observations" @default.
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- W2007687517 doi "https://doi.org/10.1016/s1464-1917(99)00055-0" @default.
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