Low/High Amplitude Anisotropic Wave Train Events in Cosmic Ray Intensity as an Effect of Interplanatery Turbulances

Physics

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Scientific paper

Using the ground based neutron monitor data of Deep River we have studied the low and high amplitude anisotropic wave train events (LAE/HAE) in cosmic ray intensity for different latitudes. The investigation has been made for both LAE and HAE during the period 1981-94. It has been observed that the phase of diurnal anisotropy for ma jority of HAE/LAE cases remains in the same co-rotational direction while phase of diurnal anisotropy shifted to later hours for some of the HAE cases, whereas shifted to early hours for some of the LAE cases. Further, for ma jority of HAE/LAE cases the amplitude of semi-diurnal anisotropy remains statistically the same, while phase of semi-diurnal anisotropy for all HAE cases shifted to later hours. The HAE appears dominant during the declining phase of solar activity whereas LAE appears dominant during minimum solar activity.

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