Rising Thermal Bubble
In this example, we demonstrate the usage of the ClimateMachine
AtmosModel machinery to solve the fluid dynamics of a thermal perturbation in a neutrally stratified background state defined by its uniform potential temperature. We solve a flow in a box configuration - this is representative of a large-eddy simulation. Several versions of the problem setup may be found in literature, but the general idea is to examine the vertical ascent of a thermal bubble (we can interpret these as simple representation of convective updrafts).
Description of experiment
- Dry Rising Bubble (circular potential temperature perturbation)
- Boundaries Top and Bottom boundaries:
Impenetrable(FreeSlip())
- Top and bottom: no momentum flux, no mass flux through walls.Impermeable()
- non-porous walls, i.e. no diffusive fluxes through walls.
- Laterally periodic
- Domain - 2500m (horizontal) x 2500m (horizontal) x 2500m (vertical)
- Resolution - 50m effective resolution
- Total simulation time - 1000s
- Mesh Aspect Ratio (Effective resolution) 1:1
- Overrides defaults for
- CPU Initialisation
- Time integrator
- Sources
- Smagorinsky Coefficient
This experiment setup assumes that you have installed the ClimateMachine
according to the instructions on the landing page. We assume the users' familiarity with the conservative form of the equations of motion for a compressible fluid (see the AtmosModel page).
The following topics are covered in this example
- Package requirements
- Defining a
model
subtype for the set of conservation equations - Defining the initial conditions
- Applying source terms
- Choosing a turbulence model
- Adding tracers to the model
- Choosing a time-integrator
- Choosing diagnostics (output) configurations
The following topics are not covered in this example
- Defining new boundary conditions
- Defining new turbulence models
- Building new time-integrators
- Adding diagnostic variables (beyond a standard pre-defined list of variables)
Loading code
Before setting up our experiment, we recognize that we need to import some pre-defined functions from other packages. Julia allows us to use existing modules (variable workspaces), or write our own to do so. Complete documentation for the Julia module system can be found here.
We need to use the ClimateMachine
module! This imports all functions specific to atmospheric and ocean flow modeling.
using ClimateMachine
ClimateMachine.init()
using ClimateMachine.Atmos
using ClimateMachine.Orientations
using ClimateMachine.ConfigTypes
using ClimateMachine.Diagnostics
using ClimateMachine.GenericCallbacks
using ClimateMachine.ODESolvers
using Thermodynamics.TemperatureProfiles
using Thermodynamics
using ClimateMachine.TurbulenceClosures
using ClimateMachine.VariableTemplates
[1638959891.085061] [hpc-92-37:26680:0] ib_verbs.h:84 UCX ERROR ibv_exp_query_device(mlx5_0) returned 38: No space left on device
In ClimateMachine we use StaticArrays
for our variable arrays. We also use the Test
package to help with unit tests and continuous integration systems to design sensible tests for our experiment to ensure new / modified blocks of code don't damage the fidelity of the physics. The test defined within this experiment is not a unit test for a specific subcomponent, but ensures time-integration of the defined problem conditions within a reasonable tolerance. Immediately useful macros and functions from this include @test
and @testset
which will allow us to define the testing parameter sets.
using StaticArrays
using Test
using CLIMAParameters
using CLIMAParameters.Atmos.SubgridScale: C_smag
using CLIMAParameters.Planet: R_d, cp_d, cv_d, MSLP, grav
struct EarthParameterSet <: AbstractEarthParameterSet end
const param_set = EarthParameterSet();
Initial Conditions
This example demonstrates the use of functions defined in the Thermodynamics
package to generate the appropriate initial state for our problem.
The following variables are assigned in the initial condition
state.ρ
= Scalar quantity for initial density profilestate.ρu
= 3-component vector for initial momentum profilestate.energy.ρe
= Scalar quantity for initial total-energy profile humiditystate.tracers.ρχ
= Vector of four tracers (here, for demonstration only; we can interpret these as dye injections for visualization purposes)
function init_risingbubble!(problem, bl, state, aux, localgeo, t)
(x, y, z) = localgeo.coord
# Problem float-type
FT = eltype(state)
param_set = parameter_set(bl)
# Unpack constant parameters
R_gas::FT = R_d(param_set)
c_p::FT = cp_d(param_set)
c_v::FT = cv_d(param_set)
p0::FT = MSLP(param_set)
_grav::FT = grav(param_set)
γ::FT = c_p / c_v
# Define bubble center and background potential temperature
xc::FT = 5000
yc::FT = 1000
zc::FT = 2000
r = sqrt((x - xc)^2 + (z - zc)^2)
rc::FT = 2000
θamplitude::FT = 2
# This is configured in the reference hydrostatic state
ref_state = reference_state(bl)
θ_ref::FT = ref_state.virtual_temperature_profile.T_surface
# Add the thermal perturbation:
Δθ::FT = 0
if r <= rc
Δθ = θamplitude * (1.0 - r / rc)
end
# Compute perturbed thermodynamic state:
θ = θ_ref + Δθ ## potential temperature
π_exner = FT(1) - _grav / (c_p * θ) * z ## exner pressure
ρ = p0 / (R_gas * θ) * (π_exner)^(c_v / R_gas) ## density
T = θ * π_exner
e_int = internal_energy(param_set, T)
ts = PhaseDry(param_set, e_int, ρ)
ρu = SVector(FT(0), FT(0), FT(0)) ## momentum
# State (prognostic) variable assignment
e_kin = FT(0) ## kinetic energy
e_pot = gravitational_potential(bl, aux) ## potential energy
ρe_tot = ρ * total_energy(e_kin, e_pot, ts) ## total energy
ρχ = FT(0) ## tracer
# We inject tracers at the initial condition at some specified z coordinates
if 500 < z <= 550
ρχ += FT(0.05)
end
# We want 4 tracers
ntracers = 4
# Define 4 tracers, (arbitrary scaling for this demo problem)
ρχ = SVector{ntracers, FT}(ρχ, ρχ / 2, ρχ / 3, ρχ / 4)
# Assign State Variables
state.ρ = ρ
state.ρu = ρu
state.energy.ρe = ρe_tot
state.tracers.ρχ = ρχ
end
init_risingbubble! (generic function with 1 method)
Model Configuration
We define a configuration function to assist in prescribing the physical model. The purpose of this is to populate the ClimateMachine.AtmosLESConfiguration
with arguments appropriate to the problem being considered.
function config_risingbubble(
::Type{FT},
N,
resolution,
xmax,
ymax,
zmax,
) where {FT}
# Since we want four tracers, we specify this and include the appropriate
# diffusivity scaling coefficients (normally these would be physically
# informed but for this demonstration we use integers corresponding to the
# tracer index identifier)
ntracers = 4
δ_χ = SVector{ntracers, FT}(1, 2, 3, 4)
# To assemble `AtmosModel` with no tracers, set `tracers = NoTracers()`.
# The model coefficient for the turbulence closure is defined via the
# [CLIMAParameters
# package](https://CliMA.github.io/CLIMAParameters.jl/latest/) A reference
# state for the linearisation step is also defined.
T_surface = FT(300)
T_min_ref = FT(0)
T_profile = DryAdiabaticProfile{FT}(param_set, T_surface, T_min_ref)
ref_state = HydrostaticState(T_profile)
# Here we assemble the `AtmosModel`.
_C_smag = FT(C_smag(param_set))
physics = AtmosPhysics{FT}(
param_set; ## Parameter set corresponding to earth parameters
ref_state = ref_state, ## Reference state
turbulence = SmagorinskyLilly(_C_smag), ## Turbulence closure model
moisture = DryModel(), ## Exclude moisture variables
tracers = NTracers{ntracers, FT}(δ_χ), ## Tracer model with diffusivity coefficients
)
model = AtmosModel{FT}(
AtmosLESConfigType, ## Flow in a box, requires the AtmosLESConfigType
physics; ## Atmos physics
init_state_prognostic = init_risingbubble!, ## Apply the initial condition
source = (Gravity(),), ## Gravity is the only source term here
)
# Finally, we pass a `Problem Name` string, the mesh information, and the
# model type to the [`AtmosLESConfiguration`] object.
config = ClimateMachine.AtmosLESConfiguration(
"DryRisingBubble", ## Problem title [String]
N, ## Polynomial order [Int]
resolution, ## (Δx, Δy, Δz) effective resolution [m]
xmax, ## Domain maximum size [m]
ymax, ## Domain maximum size [m]
zmax, ## Domain maximum size [m]
param_set, ## Parameter set.
init_risingbubble!, ## Function specifying initial condition
model = model, ## Model type
)
return config
end
config_risingbubble (generic function with 1 method)
Keywords
are used to specify some arguments (see appropriate source files).
Diagnostics
Here we define the diagnostic configuration specific to this problem.
function config_diagnostics(driver_config)
interval = "10000steps"
dgngrp = setup_atmos_default_diagnostics(
AtmosLESConfigType(),
interval,
driver_config.name,
)
return ClimateMachine.DiagnosticsConfiguration([dgngrp])
end
function main()
# These are essentially arguments passed to the
# [`config_risingbubble`](@ref config-helper) function. For type
# consistency we explicitly define the problem floating-precision.
FT = Float64
# We need to specify the polynomial order for the DG discretization,
# effective resolution, simulation end-time, the domain bounds, and the
# courant-number for the time-integrator. Note how the time-integration
# components `solver_config` are distinct from the spatial / model
# components in `driver_config`. `init_on_cpu` is a helper keyword argument
# that forces problem initialization on CPU (thereby allowing the use of
# random seeds, spline interpolants and other special functions at the
# initialization step.)
N = 4
Δh = FT(125)
Δv = FT(125)
resolution = (Δh, Δh, Δv)
xmax = FT(10000)
ymax = FT(500)
zmax = FT(10000)
t0 = FT(0)
timeend = FT(100)
# For full simulation set `timeend = 1000`
# Use up to 1.7 if ode_solver is the single rate LSRK144.
CFL = FT(1.7)
# Assign configurations so they can be passed to the `invoke!` function
driver_config = config_risingbubble(FT, N, resolution, xmax, ymax, zmax)
# Choose an Explicit Single-rate Solver from the existing [`ODESolvers`](@ref ClimateMachine.ODESolvers) options.
# Apply the outer constructor to define the `ode_solver`.
# The 1D-IMEX method is less appropriate for the problem given the current
# mesh aspect ratio (1:1).
ode_solver_type = ClimateMachine.ExplicitSolverType(
solver_method = LSRK144NiegemannDiehlBusch,
)
# If the user prefers a multi-rate explicit time integrator,
# the ode_solver above can be replaced with
#
# `ode_solver = ClimateMachine.MultirateSolverType(
# fast_model = AtmosAcousticGravityLinearModel,
# slow_method = LSRK144NiegemannDiehlBusch,
# fast_method = LSRK144NiegemannDiehlBusch,
# timestep_ratio = 10,
# )`
# See [ODESolvers](@ref ODESolvers-docs) for all of the available solvers.
solver_config = ClimateMachine.SolverConfiguration(
t0,
timeend,
driver_config,
ode_solver_type = ode_solver_type,
init_on_cpu = true,
Courant_number = CFL,
)
dgn_config = config_diagnostics(driver_config)
# Invoke solver (calls `solve!` function for time-integrator), pass the driver,
# solver and diagnostic config information.
result = ClimateMachine.invoke!(
solver_config;
diagnostics_config = dgn_config,
user_callbacks = (),
check_euclidean_distance = true,
)
# Check that the solution norm is reasonable.
@test isapprox(result, FT(1); atol = 1.5e-3)
end
main (generic function with 1 method)
The experiment definition is now complete. Time to run it.
Running the file
julia --project tutorials/Atmos/risingbubble.jl
will run the experiment from the main ClimateMachine.jl directory, with diagnostics output at the intervals specified in config_diagnostics
. You can also prescribe command line arguments for simulation update and output specifications. For rapid turnaround, we recommend that you run this experiment on a GPU.
VTK output can be controlled via command line by setting parse_clargs=true
in the ClimateMachine.init
arguments, and then using --vtk=<interval>
.
Output Visualisation
See the ClimateMachine
API interface documentation for generating output.
are two commonly used programs for .vtu
files.
For NetCDF or JLD2 diagnostics you may use any of the following tools: Julia's NCDatasets
and JLD2
packages with a suitable
or the known and quick NCDF visualization tool: ncview
plotting program.
main()
Test Passed
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