Titlebook: Cosmic Rays in the Heliosphere; Volume Resulting fro L. A. Fisk,J. R. Jokipii,K.-P. Wenzel Book 1998 Springer Science+Business Media Dordre

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https://doi.org/10.1007/978-3-319-94367-1 rays over a period of time that now exceeds 25 years and extends to heliocentric distances beyond 65 AU. These data, when compared over consecutive 11 year solar cycles, clearly establishes the existence of a 22-year cosmic ray modulation cycle that is dominated by the 11-year solar activity cycle

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Conducting a Competency Analysisdinal and radial gradients of these particles exhibit a 22-year periodicity in concert with the reversal of the Sun’s magnetic field. The power-law index of the low energy portion of the energy spectrum of ACRs at the shock in 1996 appears to be ≤ −1.3, suggesting that the strength of the solar wind

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Structured On-the-Job Training Modulesmission to the many low latitude inner heliosphere missions that preceded it. The two major omissions are the high latitude solar wind at solar maximum, which will he measured during the second Ulysses polar passages. and the solar wind near the Sun. which could he analyzed by a Solar Probe mission.