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- | ====== Geo/Planetary Dynamo Model Wish List ====== | ||
- | __Must Haves__ | ||
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- | - **As realistic parameter values as possible** | ||
- | - Boundary conditions: | ||
- | - Temperature: Dirichlet, Neumann or Robin conditions at either boundary | ||
- | - Tangential Velocity: No slip or viscous stress-free or drag laws, e.g. general Rayleigh friction, Ekman friction | ||
- | - Magnetic Field: Finitely or perfectly conducting or insulating at both boundaries, CMB: specify conductance of layer instead of conductivity for a weakly conducting layer | ||
- | - Radial velocity: impermeable, drag laws, prescribable | ||
- | - Initial Conditions on B,v,T: | ||
- | - present day B field | ||
- | - weak or strong B field | ||
- | - benchmark case | ||
- | - dipolar or multipolar B field | ||
- | - gravity fields? | ||
- | - ability to change resolution in initial file | ||
- | - Geometry: | ||
- | - Prescription of inner core size, including no inner core | ||
- | - Topography on boundaries using small slope approximation | ||
- | - External Influences: | ||
- | - Mantle thermal heterogeneities as a thermal boundary condition | ||
- | - External magnetic field sources | ||
- | - Driving Mechanisms: | ||
- | - Internal heating | ||
- | - Compositional driving independent of thermal driving | ||
- | - Stratification: | ||
- | - Allowing radial stratification through background temperature profiles (i.e. fake heat sources in Boussinesq models) | ||
- | - Prescribed radial variations of internal heat sources, secular cooling, and compositional change (note: this is a generalization of item 5a). | ||
- | - Temperature/pressure dependent physical parameters | ||
- | - Different equations of state | ||
- | - Radial variations (e.g. density, conductivity, viscosity…) | ||
- | - Freely Rotating Inner core that can respond to torques from: | ||
- | - Inner-core / Mantle gravitational coupling | ||
- | - EM torques | ||
- | - Viscous torques | ||
- | - Explicit treatment of Coriolis force | ||
- | |||
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- | __"Easy" Additions__ | ||
- | |||
- | - Driving Mechanisms: | ||
- | - Precession, Tides, Mechanical torques | ||
- | - Stratification: | ||
- | - Internal interfaces through continuity conditions | ||
- | - Implicit treatment of Coriolis force | ||
- | - Subgrid-scale turbulence | ||
- | - Gravity field solver (including mantle density anomalies) | ||
- | - Radiative regions in gas giant atmospheres | ||
- | |||
- | __Dream of having__ | ||
- | |||
- | - **Even more realistic parameter values than currently possible** | ||
- | - Real geochemistry in the core | ||
- | - snow zones | ||
- | - helium rain | ||
- | - other odd features due to chemistry in multi-component fluids | ||
- | - geochemical reactions with the mantle at the CMB | ||
- | - solid/fluid mixtures | ||
- | - Inner core physics | ||
- | - convection in the inner core | ||
- | - inner core translation | ||
- | - phase equilibrium at inner core boundary | ||
- | - inner core ellipticity – respond to gravitational torques in mantle | ||
- | - Real geochemistry in the core | ||
- | - snow zones | ||
- | - helium rain | ||
- | - other odd features due to chemistry in multi-component fluids | ||
- | - Mushy layer physics at ICB | ||
- | - Solid/fluid mixtures | ||
- | - Boundary conditions: | ||
- | - tangential velocity field: magnetoviscous friction | ||
- | - radial velocity: permeable | ||
- | - time-varying inner core radius | ||
- | - Laterally variable temperature/pressure dependent physical parameters (e.g relating conductivity directly to temperature in Hot Jupiter atmospheres) |