Variation of diurnal anisotropy during minimum of solar activity cycles 20 and 21.

Details Variation of diurnal anisotropy during minimum of solar activity cycles 20 and 21. Variation of diurnal anisotropy during minimum of solar activity cycles 20 and 21.

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996injpb..70..271s&link_type=abstract

Indian J. Phys., Part B, Vol. 70B, No. 4, p. 271 - 276

Physics

Cosmic Rays: Solar Modulation

Scientific paper

A harmonic analysis technique was employed to study the variation of the amplitude and phase of the diurnal anisotropy during the period 1964 - 87 including two reversals of total solar magnetic field and three solar minimum: 1964 - 65 (±), 1976 (±) and 1986 - 87 (±). The authors observed that during the minimum of 1976 (±) when the north polar magnetic field was positive, the phase of the diurnal anisotropy shifted to earlier hours from the 1800 hrs corotation direction as reported by the convection-diffusion model.

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