Main Image
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
M. Den
Full text: pdf
Published on: 2016 August 18
DOI: https://doi.org/10.22323/1.236.0184
Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-ShareAlike.