no code implementations • 22 Feb 2021 • Nicolas Wijsen, Evangelia Samara, Àngels Aran, David Lario, Jens Pomoell, Stefaan Poedts
The simulation reproduces the solar wind configuration and the energetic particle enhancements observed by both spacecraft.
Space Physics Solar and Stellar Astrophysics
no code implementations • 12 Feb 2021 • Evangelia Samara, Rui F. Pinto, Jasmina Magdalenic, Nicolas Wijsen, Veronika Jercic, Camilla Scolini, Immanuel C. Jebaraj, Luciano Rodriguez, Stefaan Poedts
We compared the output of the default coronal model with the output from MULTI-VP at the inner boundary of the heliospheric domain of EUHFORIA in order to understand differences between the two models, before they propagate to Earth.
Solar and Stellar Astrophysics Space Physics
no code implementations • 26 Nov 2020 • Fan Zhang, Stefaan Poedts, Andrea Lani, Błażej Kuźma, Kris Murawski
In the present numerical simulations, the initial density is specified to reach hydrostatic equilibrium, and as a comparison, chemical equilibrium is also taken into account to provide a density profile that differs from typical hydrostatic equilibrium profiles.
Plasma Physics Solar and Stellar Astrophysics
