Modeling Solar Atmosphere
Title: Modeling Solar Atmosphere
DNr: NAISS 2024/22-702
Project Type: NAISS Small Compute
Principal Investigator: Sanja Danilovic <>
Affiliation: Stockholms universitet
Duration: 2024-05-31 – 2024-09-01
Classification: 10305


Magnetism underlies much of the activity and dynamics of the solar atmosphere. The physics of the solar atmosphere is complex, encompassing the interaction of (polarised) radiation and matter, magneto-hydrodynamics and plasma physics. Understanding the observations in terms of physics thus requires intricate theoretic modeling. This project is part of "Physics of the solar atmosphere" (proposal ) The aim of applying for the time before the decision is taken is to use the best of our time with developers of the GPU version of the code which we have not run before and maximize the usage of Dardel in the future.