Impact of solar magnetic field amplitude and geometry on cosmic rays diffusion coefficients in the inner heliosphere | Journal of Space Weather and Space Climate

Topical Issue - Space climate: The past and future of solar activity

Open Access

Fig. 2

2D (on the left) and 1D (on the right) representation of the Alfvén wave energy density ϵ obtained with our fit. For the left panel, we illustrate the profile of ϵ for the reference case D1 (see Table 2). For the right panel, we show the radial profile taken at the north pole (top) and the latitudinal profile taken in the northern hemisphere at 1 AU. Values are in .

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