aragog.output
output
Output
FloatOrArray = float | npt.NDArray
module-attribute
__version__ = '26.01.06'
module-attribute
logger = logging.getLogger(__name__)
module-attribute
Evaluator(_parameters)
dataclass
Contains classes that evaluate quantities necessary to compute the interior evolution.
Args: _parameters: Parameters
Attributes: boundary_conditions: Boundary conditions initial_condition: Initial condition mesh: Mesh phases: Evaluators for all phases radionuclides: Radionuclides
Output(solver)
Stores inputs and outputs of the models.
Source code in aragog/output.py
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conductive_heat_flux_basic
property
Conductive heat flux
convective_heat_flux_basic
property
Convective heat flux
core_mass
property
Core mass computed with constant density
dTdr
property
dTdr
dTdrs
property
dTdrs
density_basic
property
Density
gravitational_separation_heat_flux_basic
property
Gravitational separation heat flux
heat_capacity_basic
property
Heat capacity
heating
property
Internal heat generation at staggered nodes
heating_dilatation
property
Internal heat generation from dilatation/compression at staggered nodes
heating_radio
property
Internal heat generation from radioactive decay at staggered nodes
heating_tidal
property
Internal heat generation from tidal heat dissipation at staggered nodes
liquidus_K_staggered
property
Liquidus
log10_viscosity_basic
property
Viscosity of the basic mesh
log10_viscosity_staggered
property
Viscosity of the staggered mesh
mantle_mass
property
Mantle mass computed from the AdamsWilliamsonEOS
mass_radii_km_basic
property
Mass radii of the basic mesh in km
mass_radii_km_staggered
property
Mass radii of the staggered mesh in km
mass_staggered
property
Mass of each layer on staggered mesh
melt_fraction_basic
property
Melt fraction on the basic mesh
melt_fraction_global
property
Volume-averaged melt fraction
melt_fraction_staggered
property
Melt fraction on the staggered mesh
mixing_heat_flux_basic
property
Convective mixing heat flux
pressure_GPa_basic
property
Pressure of the basic mesh in GPa
pressure_GPa_staggered
property
Pressure of the staggered mesh in GPa
radii_km_basic
property
Radii of the basic mesh in km
radii_km_staggered
property
Radii of the staggered mesh in km
rheological_front
property
Rheological front at the last solve iteration given user defined threshold. It is defined as a dimensionless distance with respect to the outer radius.
shape_basic
property
Shape of the basic data
shape_staggered
property
Shape of the staggered data
solidus_K_staggered
property
Solidus
solution_top_temperature
property
Solution (last iteration) temperature at the top of the domain (planet surface)
super_adiabatic_temperature_gradient_basic
property
Super adiabatic temperature gradient
temperature_K_basic
property
Temperature of the basic mesh in K
temperature_K_staggered
property
Temperature of the staggered mesh in K
thermal_expansivity_basic
property
Thermal expansivity
times
property
Times in years
total_heat_flux_basic
property
Conductive heat flux
plot(num_lines=11, figsize=(25, 10))
Plots the solution with labelled lines according to time.
Args: num_lines: Number of lines to plot. Defaults to 11. figsize: Size of the figure. Defaults to (25, 10).
Source code in aragog/output.py
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write_at_time(file_path, tidx=-1, compress=False)
Write the state of the model at a particular time to a NetCDF4 file on the disk.
Args: file_path: Path to the output file tidx: Index on the time axis at which to access the data compress: Whether to compress the data
Source code in aragog/output.py
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Parameters(*, boundary_conditions, energy, initial_condition, mesh, phase_solid, phase_liquid, phase_mixed, radionuclides, scalings, solver)
dataclass
Assembles all the parameters.
The parameters in each section are scaled here to ensure that all the parameters are scaled (non-dimensionalised) consistently with each other.
from_file(*filenames)
classmethod
Parses the parameters in a configuration file(s)
Args: *filenames: Filenames of the configuration data
Source code in aragog/parser.py
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radionuclide_sections(parser)
staticmethod
Section names relating to radionuclides
Sections relating to radionuclides must have the prefix radionuclide_
Source code in aragog/parser.py
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Solver(param)
Solves the interior dynamics
Args: filename: Filename of a file with configuration settings root: Root path to the flename
Attributes: filename: Filename of a file with configuration settings root: Root path to the filename. Defaults to empty parameters: Parameters evaluator: Evaluator state: State
Source code in aragog/solver.py
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solution
property
The solution.
temperature_basic
property
Temperature of the basic mesh in K
temperature_staggered
property
Temperature of the staggered mesh in K
dTdt(time, temperature)
dT/dt at the staggered nodes
Args: time: Time temperature: Temperature at the staggered nodes
Returns: dT/dt at the staggered nodes
Source code in aragog/solver.py
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from_file(filename, root=Path())
classmethod
Parses a configuration file
Args: filename: Filename root: Root of the filename
Returns: Parameters
Source code in aragog/solver.py
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initialize()
Initializes the model.
Source code in aragog/solver.py
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make_tsurf_event()
Creates a temperature event function for use with an ODE solver to monitor changes in the surface temperature.The event triggers when the change exceeds the threshold, allowing the solver to stop integration.
Returns: The event has the attributes: - terminal = True: Integration stops when the event is triggered. - direction = -1: Only triggers when the function is decreasing through zero.
Source code in aragog/solver.py
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reset()
This function initializes the model, while keeping the previous state of the PhaseEvaluatorCollection object. This avoids multiple loads of lookup table data when running Aragog multiple times.
Source code in aragog/solver.py
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State(parameters, _evaluator)
dataclass
Stores and updates the state at temperature and pressure.
Args: parameters: Parameters evaluator: Evaluator
Attributes: evaluator: Evaluator critical_reynolds_number: Critical Reynolds number gravitational_separation_flux: Gravitational separation flux at the basic nodes heating: Total internal heat production at the staggered nodes (power per unit mass) heating_radio: Radiogenic heat production at the staggered nodes (power per unit mass) heating_tidal: Tidal heat production at the staggered nodes (power per unit mass) heat_flux: Heat flux at the basic nodes (power per unit area) inviscid_regime: True if the flow is inviscid and otherwise False, at the basic nodes inviscid_velocity: Inviscid velocity at the basic nodes is_convective: True if the flow is convecting and otherwise False, at the basic nodes reynolds_number: Reynolds number at the basic nodes super_adiabatic_temperature_gradient: Super adiabatic temperature gradient at the basic nod temperature_basic: Temperature at the basic nodes temperature_staggered: Temperature at the staggered nodes bottom_temperature: Temperature at the bottom basic node top_temperature: Temperature at the top basic node viscous_regime: True if the flow is viscous and otherwise False, at the basic nodes viscous_velocity: Viscous velocity at the basic nodes
critical_reynolds_number
property
Critical Reynolds number from Abe (1993)
heat_flux
property
The total heat flux according to the fluxes specified in the configuration.
heating
property
The power generation according to the heat sources specified in the configuration.
heating_dilatation
property
The heat source through dilation/compression.
heating_radio
property
The radiogenic power generation.
heating_tidal
property
The tidal power generation.
mass_flux
property
The total melt mass flux according to the fluxes specified in the configuration.
conductive_heat_flux()
Conductive heat flux:
where \(k\) is thermal conductivity, \(T\) is temperature, and \(r\) is radius.
Source code in aragog/solver.py
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convective_heat_flux()
Convective heat flux:
where \(\rho\) is density, \(c_p\) is heat capacity at constant pressure, \(\kappa_h\) is eddy diffusivity, \(T\) is temperature, \(r\) is radius, and \(S\) is entropy.
Source code in aragog/solver.py
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dilatation_heating()
Dilatation/compression heating (power per unit mass)
Returns: Dilatation/compression heating (power per unit mass) at each layer of the staggered mesh, at a given point in time.
Source code in aragog/solver.py
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gravitational_separation_mass_flux()
Gravitational separation mass flux:
where \(\rho\) is density, \(\phi\) is melt fraction, and \(v_{rel}\) is relative velocity.
Source code in aragog/solver.py
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mixing_mass_flux()
Mixing mass flux:
where \(\rho\) is density, \(\kappa_h\) is eddy diffusivity, \(\phi\) is melt mass fraction, and \(r\) is radius.
Source code in aragog/solver.py
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radiogenic_heating(time)
Radiogenic heating (constant with radius)
Args: time: Time
Returns: Radiogenic heating (power per unit mass) at each layer of the staggered mesh, at a given point in time.
Source code in aragog/solver.py
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tidal_heating()
Tidal heating at each layer of the mantle.
Args: time: Time
Returns: Tidal heating (power per unit mass) at each layer of the staggered mesh, at a given point in time.
Source code in aragog/solver.py
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update(temperature, time)
Updates the state.
The evaluation order matters because we want to minimise the number of evaluations.
Args: temperature: Temperature at the staggered nodes pressure: Pressure at the staggered nodes time: Time
Source code in aragog/solver.py
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