Effect of Interplanetary Turbulences Causing Unusual Behaviour in CR Intensity

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Scientific paper

The unusually low as well as enhanced amplitude anisotropic wave train events in cosmic ray intensity have been investigated, using neutron monitoring data for different latitude. The enhanced amplitude events occur dominantly during the declining phase of solar activity, whereas, low amplitude events occur dominantly during minimum solar activity period. The Bz is found to remain +ve for ma jority of the days of the events, which shows that the occurrence of enhanced and low amplitude events is dominant during the positively directed IMF polarity. Further, during the period of events number of Interplanetary Magnetic Clouds have been identified using IMF and SWP parameters. The geomagnetic activity index-Ap is found to remain low during the period of events. The possible phenomenon to cause the enhanced as well as unusually low amplitude daily variation has been proposed to appear on the back side of the Sun.

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