Hale sector boundary and geomagnetic activity

Physics

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Geomagnetism, Interplanetary Magnetic Fields, Magnetic Disturbances, Solar Activity Effects, Indexes (Ratios), Solar Cycles, Solar Magnetic Field

Scientific paper

The variation of the geomagnetic activity index around the interplanetary magnetic field sector boundary has been analyzed for three solar cycles, 1947-1954, 1955-1964 and 1965-1975. The data were divided into vernal and autumnal equinoxes, and the variation around the Hale and non-Hale boundaries was determined. The geomagnetic activity at the interplanetary magnetic field sector boundary crossing was found to be influenced by a variety of factors, including the type of boundary, the season, solar wind parameters, Rozenberg-Coleman effects and geomagnetic dipole orientation. The geomagnetic activity index displays a sharp modulation at the Hale boundary and a sharp minimum prior to the non-Hale boundary, possibly due to the enhancement of the photospheric magnetic field intensity at the Hale sector boundary.

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