Twenty years of interplanetary magnetofluid variations with periods between 10 days and 3 years

Details Twenty years of interplanetary magnetofluid variations with periods between 10 days and 3 years Twenty years of interplanetary magnetofluid variations with periods between 10 days and 3 years

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382..399s&link_type=abstract

Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 399

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Solar Wind Plasma, Sources Of Solar Wind, Particle Emission, Solar Wind, Interplanetary Magnetic Fields

Scientific paper

A new dynamic periodogram technique has been developed to study variations in the solar wind plasma and magnetic field parameters collected primarily by IMP-8 during its more then twenty years of mission life. The long data set and the new technique allows the determination of changes in the various periodicities as a function of time. For example, a 1-year oscillation is shown to be most pronounced during solar minima, while during solar maxima half-year and 2-year periodicities are dominant. Many other periodicities (~36, 50, 73, ~154 days, ~9 months, and 1.3-years) are identified and their time dependencies investigated.

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