Twenty-two year cycle in the cosmic ray quasi-quinquennnial variation.

Details Twenty-two year cycle in the cosmic ray quasi-quinquennnial variation. Twenty-two year cycle in the cosmic ray quasi-quinquennnial variation.

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc...10...51e&link_type=abstract

18th International Cosmic Ray Conference, Vol. 10, p. 51 - 54

Computer Science

Cosmic Rays:Solar Modulation

Scientific paper

It is shown, from the data obtained during two complete sunspot cycles, that a 22 yr variation in the phase of the cosmic ray quasi-quinquennial wave exists. The changes of this variation in cosmic ray intensity as a function of a corresponding solar activity variation show that the phase lag between these two waves is changing over the solar activity cycle. The results are interpreted in terms of the solar magnetic field inversion.

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