Cosmic-Ray Diffusion Coefficients throughout the Inner Heliosphere from a Global Solar Wind Simulation

We use a three-dimensional magnetohydrodynamic simulation of the solar wind to calculate cosmic-ray diffusion coefficients throughout the inner heliosphere (2 R⊙ - 3 au). The simulation resolves large-scale solar wind flow, which is coupled to small-scale fluctuations through a turbulence model. Sim...

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Bibliographic Details
Main Authors: R. Chhiber, P. Subedi, A. V. Usmanov, W. H. Matthaeus, D. Ruffolo, M. L. Goldstein, T. N. Parashar
Other Authors: Bartol Research Institute
Format: Article
Published: 2018
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Online Access:https://repository.li.mahidol.ac.th/handle/123456789/42442
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Institution: Mahidol University

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