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- W2061835880 abstract "It is shown that the 11-yr variation of the galactic cosmic-ray intensity is linearly related to the λ5303 coronal intensity close to the solar equator (± 5° or ± 10°). The available data on the temperature of the inner corona is used to calculate the annual average solar wind velocity at low heliolatitudes (± 5°) for each year during the period 1957–1967. The 11-yr variation of the computed velocity from the solar data is linearly related to the variation of cosmic-ray intensity. In terms of the theory of diffusion-convection, the empirical results are used to estimate the cosmic-ray intensity in the nearby interstellar space and hence the residual modulation at solar minimum. The following are the important conclusions: 1.(1) The size of the modulating region (R) varies with solar cycle such that for a given rigidity P, R − r/K = const. where r = 1 a.u. and K is the isotropic diffusion coefficient.2.(2) The residual modulation of the cosmic-ray intensity is roughly proportional to P−1.3.(3) The modulating parameter η for 1965 is found to be slightly higher than the upper limit of 1 GV set by Gloeckler and Jokipii (1967)." @default.
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- W2061835880 date "1973-11-01" @default.
- W2061835880 modified "2023-09-23" @default.
- W2061835880 title "Comments on “On the magnitude of the 11-year radiocarbon cycle” by P.E. Damon, Austin Long and E.I. Wallick" @default.
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- W2061835880 doi "https://doi.org/10.1016/0012-821x(73)90003-4" @default.
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