Innovating Works

TerraVirtualE

Financiado
Planetary space simulations based on the particle description for electrons and...
The question about how solar storms impact a planet has both fundamental scientific importance and great social impacts for protecting our infrastructure from the most powerful solar storms. At present, models rely on a fluid desc... The question about how solar storms impact a planet has both fundamental scientific importance and great social impacts for protecting our infrastructure from the most powerful solar storms. At present, models rely on a fluid description of the electrons due to algorithmic and computational challenges. Our goal is to develop a model of the space environment around a planet based on a particle description of both ions and electrons. We plan to use the particle in cell (PIC) model where both ions and electrons retain their nature as particles. This PIC model will allow us to investigate the critical role of energetic electrons participating in the energy and matter transfer from the solar wind to the planet inner space. What makes this goal now possible is the Energy Conserving semi implicit method (ECsim), developed by the PI. The ECsim conserves energy exactly, a critical element in the investigation of energy flow from the solar wind. In addition, the energy conservation leads to enhanced numerical stability, which in turn greatly augment ECsim’s capability to simulate very large systems such as planet atmospheres while treating electrons as particles rather than fluid. We will start from this new development and introduce two critical innovations. First, we will implement adaptive spatial and temporal resolution for finer resolution closer to the planet and in selected areas of interest. Second, we will implement CPU-GPU algorithms for the new heterogeneous supercomputers developed by EuroHPC. These innovations will increase the capability of ECsim by more than an order of magnitude making it possible to model a region as big as the Earth space environment with the computers available within the next 3-5 years. If successful, we will have the first PIC model to describe a planetary space environment where the correct particle nature of the electrons is considered with all its implication for the energy and matter transport. ver más
31/08/2028
2M€
Duración del proyecto: 63 meses Fecha Inicio: 2023-05-24
Fecha Fin: 2028-08-31

Línea de financiación: concedida

El organismo HORIZON EUROPE notifico la concesión del proyecto el día 2023-05-24
Línea de financiación objetivo El proyecto se financió a través de la siguiente ayuda:
ERC-2022-ADG: ERC ADVANCED GRANTS
Cerrada hace 2 años
Presupuesto El presupuesto total del proyecto asciende a 2M€
Líder del proyecto
KATHOLIEKE UNIVERSITEIT LEUVEN No se ha especificado una descripción o un objeto social para esta compañía.
Perfil tecnológico TRL 4-5