Volume 236 -
The 34th International Cosmic Ray Conference (ICRC2015) -
Solar and Heliospheric Physics: Theory, Models and Simulations
Three-dimensional MHD simulation of the solar wind from the solar surface to 400 solar radius using REPPU (REProduce Plasma Universe) code
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Published on:
August 18, 2016
DOI: https://doi.org/10.22323/1.236.0184
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-ShareAlike.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-ShareAlike.