Interplanetary magnetic field polarity and low-latitude geomagnetic field

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Geomagnetism, Interplanetary Magnetic Fields, Magnetic Field Configurations, Satellite Observation, Solar Activity Effects, Tropical Regions, Magnetic Effects, Magnetic Flux, Polar Regions, Polarity, Ring Currents, Statistical Correlation, Time Dependence

Scientific paper

The relationship between the low-latitude magnetic field and the polarity of the interplanetary magnetic field is determined and discussed for low and high solar activity conditions. It is found that the field reacts differently during the passage of poleward (A) and equatorward (C) sectors, and that a change of sector from A to C is associated with a large depression in the field. The response is substantially different during the passage of sector boundary, depending on the nature of the change (A to C or C to A). The observed effects are roughly similar in day, nighttime and mean daily field and occur with an enhanced magnitude during periods of high solar activity. The results computed from Alibag observations are confirmed by an analysis of the data from Hermanus and San Juan.

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