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Research Topic : saline solution, hypertonic
Field of Research : Space and Solar Physics
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Numerical Solution of Differential and Integral Equations (2)
Space and Solar Physics (2)
Astronomical and Space Sciences (1)
Atomic and Molecular Physics (1)
Numerical and Computational Mathematics (1)
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  • Funded Activity

    Discovery Projects - Grant ID: DP160100746

    Funder
    Australian Research Council
    Funding Amount
    $403,100.00
    Summary
    Advanced simulation methods for the coupled solar interior and atmosphere. This project aims to develop numerical methods for complex magnetohydrodynamic simulations able to handle sharp and dynamically evolving inhomogeneities, spherical geometries, and dramatic variations in density and wave speed across the simulation domain. The project plans to develop these methods within the context of solar wave processes, which are fundamental to the transfer of energy from the sun’s interior to its out .... Advanced simulation methods for the coupled solar interior and atmosphere. This project aims to develop numerical methods for complex magnetohydrodynamic simulations able to handle sharp and dynamically evolving inhomogeneities, spherical geometries, and dramatic variations in density and wave speed across the simulation domain. The project plans to develop these methods within the context of solar wave processes, which are fundamental to the transfer of energy from the sun’s interior to its outer atmosphere, to the acceleration of the solar wind that rushes past the Earth continually, and to solar activity in general. This would provide the best available modelling of how the sun's atmosphere works, with direct implications for how the Earth's space environment is determined by solar storms and eruptions.
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    Funded Activity

    ARC Future Fellowships - Grant ID: FT120100057

    Funder
    Australian Research Council
    Funding Amount
    $571,852.00
    Summary
    Numerical modelling of the solar atmosphere. This project will develop a complete and realistic model of the magnetic solar activity using computer simulations of the interconnected solar interior and atmosphere. The results of this project will provide a deeper insight into the physical processes behind solar activity phenomena and will help in the development of methods of solar activity prediction.
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