Cosmic ray density grandients perpendicular to the solar equatorial plane

Details Cosmic ray density grandients perpendicular to the solar equatorial plane Cosmic ray density grandients perpendicular to the solar equatorial plane

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ijrsp..11..140p&link_type=abstract

Indian Journal of Radio and Space Physics (ISSN 0367-8393), vol. 11, Aug. 1982, p. 140, 141.

Physics

Space Physics

1

Cosmic Rays, Galactic Radiation, Radiant Flux Density, Anisotropy, Sunspots

Scientific paper

It is noted that the existence of cosmic-ray semidiurnal anisotropy of interplanetary origin has generally been attributed to the symmetrically rising density gradients perpendicular to the solar equatorial plane. An increase in the magnitude of the semidiurnal anisotropy of cosmic rays during the years 1973-1975 by a factor of 2 is in theory expected to be associated with larger magnitudes of the heliolatitudinal density gradients. The distribution of cosmic-ray intensity in the heliolatitude range + or - 7.25 deg obtained using the data of the Deep River neutron monitor is shown not to support the density gradient hypothesis. The presence of symmetrical gradients at higher heliolatitudes, however, cannot be ruled out.

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