On the cause of geomagnetic activity at Hale sector boundary |
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Authors: | SRPrabhakaran Nayar P Revathy |
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Institution: | Physics Department, Kerala University, Kariavattom, Trivandrum, India 695 581;Indian Institute of Geomagnetism, Magnetic Observatory, Beach, Trivandrum, India |
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Abstract: | The solar wind velocity and density have been studied around the interplanetary magnetic field sector boundaries (+ to ? and ? to +) during 1965–1974, separating the data into autumnal and vernal periods. It is noticed that the solar wind velocity shows a sharp increase around the Hale type of sector boundary in both northern and southern heliosphere indicating a more favourable condition for the high speed stream after Hale type of sector boundary crossing than non-Hale boundary. |
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