Dynamic Magnetosphere Ionosphere Thermosphere coupling
DynaMIT aims to revolutionize our understanding of space-atmosphere coupling in the polar ionosphere by integrating 3D modeling with innovative data assimilation techniques to enhance space weather predictions.
Projectdetails
Introduction
DynaMIT addresses a fundamental misunderstanding of how Earth is coupled to space in the polar ionosphere. Here, the neutral atmosphere collides with charged particles influenced by electromagnetic fields, profoundly impacting the dynamics of the atmosphere and its surroundings.
Current Understanding
Despite being the best instrumented region of space, our understanding of Earth's ionosphere is severely limited. The current paradigm contains two crippling assumptions:
- The ionosphere is only 2D.
- The ionosphere is in a steady state.
This conceptualization obscures the complex interplay of forces that change the fluids and electromagnetic fields in both regions.
Implications of Misunderstanding
This misunderstanding prevents us from accurately understanding phenomena, such as the aurora polaris, that have been observed and studied from the ground for centuries.
Project Goals
To advance beyond the state of the art, we must transition to a dynamic view of space-atmosphere coupling. This project will apply first principles to model how the neutral atmosphere, plasma, and electromagnetic fields interact.
Methodology
To do this, we will build and combine the DynaMIT model with novel measurements using an innovative data assimilation technique developed in-house. This ground-breaking combination of multi-instrument data with full 3D numerical simulations will create a radical new platform from which we will interrogate fundamental outstanding issues in space physics:
- How ionospheric dynamics disturb Earth's magnetic field.
- How energy flows between regions, and how it dissipates in the atmosphere.
- How space-atmosphere coupling shapes near-Earth space.
Importance of the Research
These questions are critical for understanding how Earth interacts with space, and the influence on technology, climate, and circulation in the lower atmosphere.
Conclusion
If successful, DynaMIT will be a paradigm change that transforms our conceptual understanding of how the atmosphere is coupled with space, provides language to explain ionospheric observations, and paves the way for improvements in space weather predictions.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 2.000.000 |
Totale projectbegroting | € 2.000.000 |
Tijdlijn
Startdatum | 1-10-2023 |
Einddatum | 30-9-2028 |
Subsidiejaar | 2023 |
Partners & Locaties
Projectpartners
- UNIVERSITETET I BERGENpenvoerder
Land(en)
Vergelijkbare projecten binnen European Research Council
Project | Regeling | Bedrag | Jaar | Actie |
---|---|---|---|---|
Open Superior Efficient Solar Atmosphere Model ExtensionDevelop a high-order GPU-enabled 3D time-evolving multi-fluid model of the solar atmosphere to enhance understanding of solar wind, flares, and CMEs for improved Earth impact predictions. | ERC Advanced... | € 2.498.230 | 2024 | Details |
Waves in the Inner Magnetosphere and their Effects on Radiation Belt ElectronsThis 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. | ERC Consolid... | € 1.999.415 | 2024 | Details |
Waves for energy in magnetized plasmasSMARTWAVES 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. | ERC Advanced... | € 2.511.038 | 2024 | Details |
MAGHEAT: understanding energy deposition in the solar chromosphereMAGHEAT aims to identify and characterize the heating mechanisms of the solar chromosphere using advanced observational data and novel simulation methods. | ERC Consolid... | € 1.994.937 | 2023 | Details |
Core dynamics on millennial timescalesPALEOCORE aims to develop an integrated core-field core-flow model to understand Earth's core dynamics over millennial timescales and forecast future magnetic field changes. | ERC Consolid... | € 1.999.854 | 2024 | Details |
Open Superior Efficient Solar Atmosphere Model Extension
Develop a high-order GPU-enabled 3D time-evolving multi-fluid model of the solar atmosphere to enhance understanding of solar wind, flares, and CMEs for improved Earth impact predictions.
Waves in the Inner Magnetosphere and their Effects on Radiation Belt Electrons
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.
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.
MAGHEAT: understanding energy deposition in the solar chromosphere
MAGHEAT aims to identify and characterize the heating mechanisms of the solar chromosphere using advanced observational data and novel simulation methods.
Core dynamics on millennial timescales
PALEOCORE aims to develop an integrated core-field core-flow model to understand Earth's core dynamics over millennial timescales and forecast future magnetic field changes.