Comparative study of the phase of diurnal anisotropy on quiet and disturbed days on a long term basis up to recent period

Details Comparative study of the phase of diurnal anisotropy on quiet and disturbed days on a long term basis up to recent period Comparative study of the phase of diurnal anisotropy on quiet and disturbed days on a long term basis up to recent period

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..124k&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 124 (SEE N85-34991 23-93)

Computer Science

Anisotropy, Atmospheric Pressure, Cosmic Rays, Diurnal Variations, Latitude, Geomagnetism, Interplanetary Magnetic Fields, Radiant Flux Density

Scientific paper

The data from the world wide grid of neutron monitoring stations was analyzed for a comparative study of the phase of diurnal anisotropy on quiet and disturbed days on a long term basis up to recent period. It has been observed that the phase of the diurnal anisotropy on disturbed days where the value of the Ap-index is higher, is found to shift towards earlier hours in comparison to the phase of the diurnal anisotropy on quiet days where the value of Ap-index is lower on all the stations from 1965 to 71. Such a trend is not observable for the later period. This affect is found to be more pronounced on equatorial stations, in particular, in comparison to high latitude stations. It was derived from these observational facts that the relationship between Ap-index and the phase of the diurnal anisotropy is not invariant throughout the period of consideration. Furthermore, the exact cause of such a drastic change is not known, but it demonstrates very clearly that the interplanetary conditions which are responsible for both, diurnal anisotropy of cosmic ray intensity and the geomagnetic Ap-index variation, have drastically changed during the period 1971 and onwards.

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