Difference between even and odd 11-year cycles in cosmic ray intensity

Details Difference between even and odd 11-year cycles in cosmic ray intensity Difference between even and odd 11-year cycles in cosmic ray intensity

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..493o&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 493-496 (SEE N85-34729 23-92)

Computer Science

Convective Flow, Current Sheets, Diffusion Coefficient, Galactic Cosmic Rays, Neutral Sheets, Solar Cycles, Sunspot Cycle, Cosmic Ray Showers, Low Pass Filters, Solar Activity

Scientific paper

Cosmic ray data for the period 1946 - 1984 are used to determine the run of the comic ray intensity over three complete solar cycles. The analysis shows a tendency towards a regular alternation of cosmic ray intensity cycles with double and single maxima. Whereas a saddle-like shape is characteristic of even cycles, odd cycles are characterized by a peak-like shape. The importance of this behaviour is discussed in terms of different processes influencing cosmic ray transport in the heliosphere.

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