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Recurrency and the origin of the vertical component of the interplanetary magnetic field
Authors:M I Pudovkin  D I Ponyavin  A D Chertkov
Institution:(1) Institute of Physics, State University, 199164 Leningrad, U.S.S.R.
Abstract:The autocorrelation functions of the solar wind velocity and of the IMF components as well as of the geomagnetic activity indices are studied for two periods: August–December, 1965 and January–May, 1974. The vertical component of the IMF is shown to exhibit a rather definite recurrency relatively independent of the recurrency of the solar wind velocity.The daily mean values of the Z-component of the IMF are shown to correlate (rhov = -0.5) with the intensity of the meridional component of the large scale solar magnetic field with time delay of about 5 days with respect to the latter. This result is interpreted as an evidence for the Z- component of the IMF to be carried away by the solar wind from the Sun.
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