Abstract
Preliminary information pertaining to the diffusive anisotropy of the galactic cosmic rays (GCR) in the inner heliosphere is derived from the study of the steady state solar diurnal variation (SDV) for the period 1965 to 1994. This time period spans three solar activity cycles. Data obtained with the neutron monitors (NM) at Deep River and Huancayo and the underground vertical muon telescopes (UT) at Embudo, are used in our analysis.
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