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- W19853550 abstract "Abstract Using the ground based neutron monitor data of Deep River we have studiedthe low and high amplitude anisotropic wave train events (LAE/HAE) in cosmic ray in-tensity for different latitudes. The investigation has been made for both LAE and HAEduring the period 1981–94. It has been observed that the phase of diurnal anisotropyfor majority of HAE/LAE cases remains in the same co-rotational direction while phaseof diurnal anisotropy shifted to later hours for some of the HAE cases, whereas shiftedto early hours for some of the LAE cases. Further, for majority of HAE/LAE casesthe amplitude of semi-diurnal anisotropy remains statistically the same, while phaseof semi-diurnal anisotropy for all HAE cases shifted to later hours. The HAE appearsdominant during the declining phase of solar activity whereas LAE appears dominantduring minimum solar activity. 1. IntroductionThe average characteristics of cosmic ray diurnal anisotropy are adequatelyexplained by the co-rotational concept. However the observed day-to-day varia-tion both in amplitude and time of maximum and the abnormally large ampli-tudes or abnormally low amplitudes of consecutive days cannot be explained inco-rotational term. The average diurnal anisotropy of cosmic radiation has gen-erally been explained in terms of azimuthal co-rotation" @default.
- W19853550 created "2016-06-24" @default.
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- W19853550 date "2003-07-01" @default.
- W19853550 modified "2023-10-07" @default.
- W19853550 title "LOW/HIGH AMPLITUDE ANISOTROPIC WAVE TRAIN EVENTS IN COSMIC RAY INTENSITY AS AN EFFECT OF INTERPLANATERY TURBULANCES" @default.
- W19853550 hasPublicationYear "2003" @default.
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