API documentation

1. Data Structures

By default, the MeshArray type is an alias to MeshArrays.gcmarray.

MeshArrays.gcmarrayType
gcmarray{T, N, AT}

gcmarray data structure. Available constructors:

gcmarray{T,N,AT}(grid::gcmgrid,meta::varmeta,f::Array{AT,N},
         fSize::Array{NTuple{N, Int}},fIndex::Array{Int,1},v::String)

gcmarray(grid::gcmgrid,f::Array{Array{T,2},N}) where {T,N}
gcmarray(grid::gcmgrid,f::Array{Array{T,N},1}) where {T,N}

gcmarray(grid::gcmgrid,fSize::Array{NTuple{N, Int}},fIndex::Array{Int,1})
gcmarray(<same as above>,n3::Int)
gcmarray(<same as above>,n3::Int,n4::Int)

gcmarray(grid::gcmgrid)
gcmarray(grid::gcmgrid,::Type{T})
gcmarray(grid::gcmgrid,::Type{T},n3::Int)
gcmarray(grid::gcmgrid,::Type{T},n3::Int,n4::Int)

gcmarray(A::Array{T,N};meta::varmeta=defaultmeta)
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MeshArrays.gcmgridType
gcmgrid

gcmgrid data structure. Available constructors:

gcmgrid(path::String, class::String, nFaces::Int, 
        fSize::Array{NTuple{2, Int},1},
        ioSize::Union{NTuple{2, Int},Array{Int64,2}},
        ioPrec::Type, read::Function, write::Function)

The class can be set to "LatLonCap", "CubeSphere", "PeriodicChannel", "PeriodicDomain".

For example, A periodic channel (periodic in the x direction) of size 360 by 160, can be defined as follows.

pth=MeshArrays.GRID_LL360
class="PeriodicChannel"
ioSize=(360, 160)
ioPrec=Float32

γ=gcmgrid(pth, class, 1, [ioSize], ioSize, ioPrec, read, write)

Γ=GridLoad(γ)    

Please refer to GridSpec and UnitGrid for more info related to gcmgrid options.

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MeshArrays.varmetaType
varmeta

varmeta data structure. By default, unit is missing (non-dimensional), position is fill(0.5,3) (cell center), time is missing, and name / long_name is unknown.

Available constructors:

varmeta(unit::Union{Unitful.Units,Number,Missing},position::Array{Float64,1},
        time::Union{DateTime,Missing,Array{DateTime,1}},name::String,long_name::String)

And:

defaultmeta = varmeta(missing,fill(0.5,3),missing,"unknown","unknown")

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More :

MeshArrays.gcmvectorType
gcmvector{T, N}

gcmvector data structure that can be used for subsetting and indexing into a gcmarray.

gcmvector{T,N}(grid::gcmgrid,f::Array{Array{T,1},N},
         fSize::Array{NTuple{N, Int}},fIndex::Array{Int,1})
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MeshArrays.gcmfacesType
gcmfaces{T, N}

gcmfaces data structure. Available constructors:

gcmfaces{T,N}(grid::gcmgrid,f::Array{Array{T,N},1},
         fSize::Array{NTuple{N, Int}}, aSize::NTuple{N,Int})

gcmfaces(grid::gcmgrid,v1::Array{Array{T,N},1}) where {T,N}
gcmfaces(grid::gcmgrid,::Type{T},
         fSize::Array{NTuple{N, Int}}, aSize::NTuple{N,Int}) where {T,N}

gcmfaces(grid::gcmgrid)
gcmfaces(grid::gcmgrid,::Type{T})
gcmfaces(grid::gcmgrid,::Type{T},n3::Int)
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2. Grids And I/O

MeshArrays.UnitGridFunction
UnitGrid(γ::gcmgrid;option="minimal")

Generate a unit grid, where every grid spacing and area is 1, according to γ.

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UnitGrid(ioSize, tileSize; option="minimal")

Generate a unit grid, where every grid spacing and area is 1, according to ioSize, tileSize.

Since ioSize, tileSize defines a one to one mapping from global to tiled array, here we use read_tiles, write_tiles instead of the default read, write. And we overwrite local XC,YC etc accordingly with global XC,YC etc .

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MeshArrays.simple_periodic_domainFunction
simple_periodic_domain(np::Integer,nq=missing)

Set up a simple periodic domain of size np x nq

using MeshArrays
np=16 #domain size is np x np
Γ=simple_periodic_domain(np)
isa(Γ.XC,MeshArray)
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MeshArrays.GridSpecFunction
GridSpec(GridName,GridParentDir="./")

Select one of the pre-defined grids (by GridName) and return the corresponding gcmgrid – a global grid specification which contains the grid files location (GridParentDir).

Possible choices for GridName:

  • "PeriodicDomain"
  • "PeriodicChannel"
  • "CubeSphere"
  • "LatLonCap"`
using MeshArrays
g = GridSpec()
g = GridSpec("PeriodicChannel",MeshArrays.GRID_LL360)
g = GridSpec("CubeSphere",MeshArrays.GRID_CS32)
g = GridSpec("LatLonCap",MeshArrays.GRID_LLC90)
isa(g,gcmgrid)
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MeshArrays.GridLoadFunction
GridLoad(γ::gcmgrid;option="minimal")

Return a NamedTuple of grid variables read from files located in γ.path (see ?GridSpec).

By default, option="minimal" means that only grid cell center positions (XC, YC) are loaded.

The "full" option provides a complete set of grid variables.

Based on the MITgcm naming convention, grid variables are:

  • XC, XG, YC, YG, AngleCS, AngleSN, hFacC, hFacS, hFacW, Depth.
  • RAC, RAW, RAS, RAZ, DXC, DXG, DYC, DYG.
  • DRC, DRF, RC, RF (one-dimensional)
using MeshArrays

γ = GridSpec("CubeSphere",MeshArrays.GRID_CS32)
#γ = GridSpec("LatLonCap",MeshArrays.GRID_LLC90)
#γ = GridSpec("PeriodicChannel",MeshArrays.GRID_LL360)

Γ = GridLoad(γ;option="full")

isa(Γ.XC,MeshArray)
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MeshArrays.GridLoadVarFunction
GridLoadVar(nam::String,γ::gcmgrid)

Return a grid variable read from files located in γ.path (see ?GridSpec, ?GridLoad).

Based on the MITgcm naming convention, grid variables are:

  • XC, XG, YC, YG, AngleCS, AngleSN, hFacC, hFacS, hFacW, Depth.
  • RAC, RAW, RAS, RAZ, DXC, DXG, DYC, DYG.
  • DRC, DRF, RC, RF (one-dimensional)
using MeshArrays

γ = GridSpec("CubeSphere",MeshArrays.GRID_CS32)
XC = GridLoadVar("XC",γ)

isa(XC,MeshArray)
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More :

MeshArrays.TilesFunction
Tiles(γ::gcmgrid,ni::Int,nj::Int)

Define sudomain tiles of size ni,nj. Each tile is defined by a Dict where tile,face,i,j correspond to tile ID, face ID, index ranges.

using MeshArrays
γ=GridSpec("LatLonCap",MeshArrays.GRID_LLC90)
τ=Tiles(γ,30,30)

isa(τ[1],NamedTuple)
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Tiles(τ::Array{Dict},x::MeshArray)

Return an Array of tiles which cover x according to tile partition τ.

using MeshArrays
γ=GridSpec("LatLonCap",MeshArrays.GRID_LLC90)
d=γ.read(γ.path*"Depth.data",MeshArray(γ,γ.ioPrec))
τ=Tiles(γ,30,30)
td=Tiles(τ,d)

D=similar(d)
Tiles!(τ,td,D)

isa(td[1],Array)
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MeshArrays.Tiles!Function
Tiles!(τ::Array,tx::Array,x::MeshArrays)

Map tiles in tx according to tile partition τ into x.

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MeshArrays.exchangeFunction
exchange(fld::MeshArray)

Exchange / transfer data between neighboring arrays. Other methods are

exchange(fld::MeshArray,N::Integer)
exchange(u::MeshArray,v::MeshArray)
exchange(u::MeshArray,v::MeshArray,N::Integer)
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Base.readFunction
read(fil::String,x::MeshArray)

Read array from file and return as a MeshArray.

The second argument (MeshArray or gcmgrid) provides the grid specifications (x.grid.ioSize). ```

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Base.read!Function
read!(xx::Array,x::MeshArray)

Reformat array into MeshArray and write into x.

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Base.writeFunction
write(fil::String,x::MeshArray)

Write MeshArray to binary file. Other methods:

write(xx::Array,x::MeshArray) #to Array
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3. Interpolation

MeshArrays.interpolation_setupFunction
interpolation_setup(fil::String)

Read e.g. interp_coeffs_halfdeg.jld2

fil=joinpath(tempdir(),"interp_coeffs_halfdeg.jld2")
λ=MeshArrays.interpolation_setup(fil)
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interpolation_setup(;Γ,lon,lat,path,url)

Download or recompute interpolation coefficients (e.g. interp_coeffs_halfdeg.jld2).

  • λ=interpolation_setup() to download from url to path
  • λ=interpolation_setup(Γ=Γ) to recompute at lon,lat
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MeshArrays.InterpolateFunction
Interpolate(z_in::MeshArray,f,i,j,w)
using MeshArrays

γ=GridSpec("LatLonCap",MeshArrays.GRID_LLC90)
Γ=GridLoad(γ; option="full")

lon=[i for i=-179.5:1.0:179.5, j=-89.5:1.0:89.5]
lat=[j for i=-179.5:1.0:179.5, j=-89.5:1.0:89.5]
(f,i,j,w,j_f,j_x,j_y)=InterpolationFactors(Γ,vec(lon),vec(lat))
DD=Interpolate(Γ.Depth,f,i,j,w)

using CairoMakie
heatmap(vec(lon[:,1]),vec(lat[1,:]),DD,colorrange=(0.,6000.))
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Interpolate(z_in::MeshArray,f,i,j,w)
using MeshArrays

γ=GridSpec("LatLonCap",MeshArrays.GRID_LLC90)
Γ=GridLoad(γ; option="full")

lon=[i for i=-179.5:1.0:179.5, j=-89.5:1.0:89.5]
lat=[j for i=-179.5:1.0:179.5, j=-89.5:1.0:89.5]
(f,i,j,w,j_f,j_x,j_y)=InterpolationFactors(Γ,vec(lon),vec(lat))
L=(lon=lon, lat=lat, f=f, i=i, j=j, w=w)

using CairoMakie
heatmap(Interpolate(Γ.Depth,L)...,colorrange=(0.,6000.))

or

heatmap(Γ.Depth,interpolation=L,colorrange=(0.,6000.))
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MeshArrays.InterpolationFactorsFunction
InterpolationFactors(Γ,lon::Array{T,1},lat::Array{T,1})

Compute interpolation coefficients etc from grid Γ to lon,lat

using MeshArrays
γ=GridSpec("CubeSphere",MeshArrays.GRID_CS32)
Γ=GridLoad(γ; option="full")
lon=collect(45.:0.1:46.); lat=collect(60.:0.1:61.)
(f,i,j,w,j_f,j_x,j_y)=InterpolationFactors(Γ,lon,lat)
YC=Interpolate(Γ.YC,f,i,j,w)
extrema(i)==(9,10)
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MeshArrays.StereographicProjectionFunction
StereographicProjection(XC0,YC0,XC,YC)

Apply stereographic projection that puts XC0,YC0 at 0.0,0.0 to target point(s) XC,YC

lon=collect(45.:0.1:46.); lat=collect(60.:0.1:61.)
x,y=StereographicProjection(45.,60.,lon,lat)
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NearestNeighbors.knnFunction
knn(xgrid,ygrid::MeshArray,x,y::Array{T,1},k::Int)

Find k nearest neighbors to each point in x,y on xgrid,ygrid

lon=collect(0.1:0.5:2.1); lat=collect(0.1:0.5:2.1);
(f,i,j,c)=knn(Γ.XC,Γ.YC,lon,lat)
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4. Vector Fields

MeshArrays.curlFunction
curl(u::MeshArray,v::MeshArray,Γ::NamedTuple)

Compute curl of a velocity field.

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MeshArrays.gradientFunction
gradient(inFLD::MeshArray,Γ::NamedTuple)

Compute spatial derivatives. Other methods:

gradient(inFLD::MeshArray,Γ::NamedTuple,doDIV::Bool)
gradient(inFLD::MeshArray,iDXC::MeshArray,iDYC::MeshArray)
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MeshArrays.UVtoTransportFunction
UVtoTransport(U,V,G::NamedTuple)

Convert e.g. velocity (m/s) to transport (m^3/s) by multiplying by DRF and DXG,DYG.

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MeshArrays.UVtoUEVNFunction
UVtoUEVN(u,v,G::NamedTuple)
  1. Interpolate to grid cell centers (uC,vC)
  2. Convert to Eastward/Northward components (uE,vN)

Note: land masking u,v with NaNs preemptively can be adequate.

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5. Other

MeshArrays.TransectFunction
Transect(name,lons,lats,Γ)

Compute integration paths that follow a great circle between two geolocations give by lons, lats.

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