Waves for energy in magnetized plasmas
SMARTWAVES aims to develop a novel plasma regime for fusion devices by enhancing wave-particle interaction understanding, improving diagnostics, and bridging fusion, space, and astrophysical research.
Projectdetails
Introduction
The interplay between energetic particles and magnetohydrodynamics (MHD) fluctuations plays a paramount role in a modern society with growing energy demands and active interaction with space weather. The prediction of space weather and the viability of fusion as a virtually unlimited source of energy rely on a good understanding of fundamental wave-particle interactions.
Challenges in Wave-Particle Interactions
Although the sources of energetic particles are quite different for space, astrophysical, and laboratory plasmas, the main challenges remain the same:
- 3D multi-scale physics
- Non-linear wave-particle interactions
SMARTWAVES Framework
In the framework of SMARTWAVES, a potentially revolutionary plasma regime for future burning fusion plasma devices with tailored MHD activity will be developed.
Diagnostic Techniques
Novel diagnostic techniques to monitor the temporal evolution of the energetic ion distribution in phase-space will allow the identification of the fundamental wave-particle resonances responsible for the experimental observations.
Next Generation Diagnostics
Combined with the next generation of electron fluctuations diagnostics, I will provide a complete physics basis of currently inaccessible wave phenomena. This will pave the way towards a high-confinement plasma regime that closes the burning plasma performance and exhaust gap, simultaneously maximizing the fusion gain and minimizing the plasma-wall interaction.
Application of Advanced Codes
Advanced 3D non-linear codes validated in tokamak plasmas will be applied to relevant solar events, paving the way to a space weather forecast station.
Knowledge Transfer and Development
I will apply the basic knowledge gained in tokamaks with advanced in-situ diagnostics to test and further develop hybrid models and numerical tools shared by the fusion, space, and astrophysical communities.
Conclusion
This project will represent a gateway between the space, astrophysical, and fusion communities, opening new horizons for a common ground science.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 2.511.038 |
Totale projectbegroting | € 3.034.433 |
Tijdlijn
Startdatum | 1-9-2024 |
Einddatum | 31-8-2029 |
Subsidiejaar | 2024 |
Partners & Locaties
Projectpartners
- UNIVERSIDAD DE SEVILLApenvoerder
Land(en)
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This project aims to develop comprehensive wave models using multi-satellite data to understand the dynamics of Earth's radiation belts and their response to geomagnetic storms.
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Illuminating neutron stars with radiative plasma physics
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