Recurrency and the origin of the vertical component of the interplanetary magnetic field

Details Recurrency and the origin of the vertical component of the interplanetary magnetic field Recurrency and the origin of the vertical component of the interplanetary magnetic field

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...66..411p&link_type=abstract

Solar Physics, vol. 66, June 1980, p. 411-416.

Physics

1

Autocorrelation, Geomagnetism, Interplanetary Magnetic Fields, Solar Magnetic Field, Solar Wind Velocity, Vertical Distribution, Correlation Coefficients, Magnetoactivity

Scientific paper

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 (rho = -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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