Solar wind structure dynamics by multipoint observations
Physics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science（2000）
Correspondence to G.N. Zastenker
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.
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Key words
solar wind,structural dynamics
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