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
