Diurnal anisotropy during solar activity cycle twenty and diffusion-convection model

Details Diurnal anisotropy during solar activity cycle twenty and diffusion-convection model Diurnal anisotropy during solar activity cycle twenty and diffusion-convection model

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..116a&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 116-119 (SEE N85-34991 23-93)

Other

Anisotropy, Convection, Diffusion, Diurnal Variations, Models, Solar Activity, Solar Cycles, Cosmic Rays, Coupling, Neutron Counters, Neutrons, Predictions, Solar Wind Velocity

Scientific paper

Underground muon telescope data obtained at Embudo and neutron monitor data obtained at Deep River are divided into two sets; one covers the ascending phase of the cycle (1965 - 70) and the other covers the descending phase (1971 - 76). The amplitude of diurnal anisotropy calculated from the data does not agree with the value predicted by the simplified version of the diffusion-convection model; the discrepancy is worse for neutron data.

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