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[documentation] Add a page about custom workspaces (#927)
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amontoison authored Nov 6, 2024
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1 change: 1 addition & 0 deletions docs/Project.toml
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Expand Up @@ -10,6 +10,7 @@ LDLFactorizations = "40e66cde-538c-5869-a4ad-c39174c6795b"
LinearAlgebra = "37e2e46d-f89d-539d-b4ee-838fcccc9c8e"
LinearOperators = "5c8ed15e-5a4c-59e4-a42b-c7e8811fb125"
MatrixMarket = "4d4711f2-db25-561a-b6b3-d35e7d4047d3"
OffsetArrays = "6fe1bfb0-de20-5000-8ca7-80f57d26f881"
Printf = "de0858da-6303-5e67-8744-51eddeeeb8d7"
SparseArrays = "2f01184e-e22b-5df5-ae63-d93ebab69eaf"
SuiteSparseMatrixCollection = "ac199af8-68bc-55b8-82c4-7abd6f96ed98"
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1 change: 1 addition & 0 deletions docs/make.jl
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Expand Up @@ -29,6 +29,7 @@ makedocs(
"Warm-start" => "warm-start.md",
"Matrix-free operators" => "matrix_free.md",
"Callbacks" => "callbacks.md",
"Custom workspaces" => "custom_workspaces.md",
"Performance tips" => "tips.md",
"Tutorials" => ["CG" => "examples/cg.md",
"CAR" => "examples/car.md",
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303 changes: 303 additions & 0 deletions docs/src/custom_workspaces.md
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## Custom workspaces for the Poisson equation with halo regions

### Introduction

The Poisson equation is a fundamental partial differential equation (PDE) in physics and mathematics, modeling phenomena like temperature distribution and incompressible fluid flow.
In a 2D Cartesian domain, it can be expressed as:

```math
\nabla^2 u(x, y) = f(x, y)
```

Here, $u(x, y)$ is the potential function and $f(x, y)$ represents the source term within the domain.

This page explains how to use a Krylov method to solve the Poisson equation over a rectangular region with specified boundary conditions, detailing the use of a Laplacian operator within a data structure that incorporates **halo regions**.

### Finite difference discretization

We solve the Poisson equation numerically by discretizing the 2D domain using a finite difference method.
For a square domain $[0, L] \times [0, L]$, divided into a grid of points, each point approximates the solution $u$ at that position.

With grid spacings $h_x = \frac{L}{N_x + 1}$ and $h_y = \frac{L}{N_y + 1}$, let $u_{i,j}$ denote the approximation of $u(x_i, y_j)$ at grid point $(x_i, y_j) = (ih, jh)$.
The 2D Laplacian can be approximated at each interior grid point $(i, j)$ by combining the following central difference formulas:

```math
\frac{\partial^2 u}{\partial x^2} \approx \frac{u_{i+1,j} - 2u_{i,j} + u_{i-1,j}}{h^2}
```

```math
\frac{\partial^2 u}{\partial y^2} \approx \frac{u_{i,j+1} - 2u_{i,j} + u_{i,j-1}}{h^2}
```

This yields the discrete Poisson equation:

```math
\frac{u_{i+1,j} - 2u_{i,j} + u_{i-1,j}}{h^2} + \frac{u_{i,j+1} - 2u_{i,j} + u_{i,j-1}}{h^2} = f_{i,j}
```

resulting in a system of linear equations for the $N^2$ unknowns $u_{i,j}$ at each interior grid point.

### Boundary conditions

Boundary conditions complete the system. Common choices are:

- **Dirichlet**: Specifies values of $u$ on the boundary.
- **Neumann**: Specifies the normal derivative (or flux) of $u$ on the boundary.

### Implementing halo regions with HaloVector

In parallel computing, **halo regions** (or ghost cells) around the grid store boundary values from neighboring subdomains, allowing independent stencil computation near boundaries.
This setup streamlines boundary management in distributed environments.

For specialized applications, Krylov.jl’s internal storage expects an `AbstractVector`, which can benefit from a structured data layout.
A **`HaloVector`** provides this structure, using halo regions to enable finite difference stencils without boundary condition checks.
The `OffsetArray` type from [OffsetArrays.jl](https://github.com/JuliaArrays/OffsetArrays.jl) facilitates custom indexing, making it ideal for grids with halo regions.
By embedding an `OffsetArray` within `HaloVector`, we achieve seamless grid alignment, allowing **"if-less"** stencil application.

This setup reduces boundary condition checks in the core loop, yielding clearer and faster code.
The flexible design of `HaloVector` supports 1D, 2D, or 3D configurations, adapting easily to different grid layouts.

### Definition and usage of the HaloVector

`HaloVector` is a specialized vector for grid-based computations, especially finite difference methods with halo regions.
It is parameterized by:

- **`FC`**: The element type of the vector.
- **`D`**: The data array type, which uses `OffsetArray` to enable custom indexing.

```@example halo-regions; continued = true
using OffsetArrays
struct HaloVector{FC, D} <: AbstractVector{FC}
data::D
function HaloVector(data::D) where {D}
FC = eltype(data)
return new{FC, D}(data)
end
end
function HaloVector{FC,D}(::UndefInitializer, l::Int64) where {FC,D}
m = n = sqrt(l) |> Int
data = zeros(FC, m + 2, n + 2)
v = OffsetMatrix(data, 0:m + 1, 0:n + 1)
return HaloVector(v)
end
function Base.length(v::HaloVector)
m, n = size(v.data)
l = (m - 2) * (n - 2)
return l
end
function Base.size(v::HaloVector)
l = length(v)
return (l,)
end
function Base.getindex(v::HaloVector, idx)
m, n = size(v.data)
row = div(idx - 1, n - 2) + 1
col = mod(idx - 1, n - 2) + 1
return v.data[row, col]
end
```

The `size` and `getindex` functions support REPL display, aiding interaction, though they are optional for Krylov.jl’s functionality.

### Efficient stencil implementation

Using `HaloVector` with `OffsetArray`, we can apply the discrete Laplacian operator in a matrix-free approach with a 5-point stencil, managing halo regions effectively.
This layout allows **clean and efficient Laplacian computation** without boundary checks within the core loop.

```@example halo-regions; continued = true
using LinearAlgebra
# Define a matrix-free Laplacian operator
struct LaplacianOperator
Nx::Int # Number of grid points in the x-direction
Ny::Int # Number of grid points in the y-direction
Δx::Float64 # Grid spacing in the x-direction
Δy::Float64 # Grid spacing in the y-direction
end
# Define size and element type for the operator
Base.size(A::LaplacianOperator) = (A.Nx * A.Ny, A.Nx * A.Ny)
Base.eltype(A::LaplacianOperator) = Float64
function LinearAlgebra.mul!(y::HaloVector{Float64}, A::LaplacianOperator, u::HaloVector{Float64})
# Apply the discrete Laplacian in 2D
for i in 1:A.Nx
for j in 1:A.Ny
# Calculate second derivatives using finite differences
dx2 = (u.data[i-1,j] - 2 * u.data[i,j] + u.data[i+1,j]) / (A.Δx)^2
dy2 = (u.data[i,j-1] - 2 * u.data[i,j] + u.data[i,j+1]) / (A.Δy)^2
# Update the output vector with the Laplacian result
y.data[i,j] = dx2 + dy2
end
end
return y
end
```

### Methods to overload for compatibility with Krylov.jl

To integrate `HaloVector` with Krylov.jl, we define essential vector operations, including dot products, norms, scalar multiplication, and element-wise updates.
These implementations allow Krylov.jl to leverage custom vector types, enhancing both solver flexibility and performance.

```@example halo-regions; continued = true
using Krylov
import Krylov.FloatOrComplex
function Krylov.kdot(n::Integer, x::HaloVector{T}, y::HaloVector{T}) where T <: FloatOrComplex
mx, nx = size(x.data)
_x = x.data
_y = y.data
res = zero(T)
for i = 1:mx-1
for j = 1:nx-1
res += _x[i,j] * _y[i,j]
end
end
return res
end
function Krylov.knorm(n::Integer, x::HaloVector{T}) where T <: FloatOrComplex
mx, nx = size(x.data)
_x = x.data
res = zero(T)
for i = 1:mx-1
for j = 1:nx-1
res += _x[i,j]^2
end
end
return sqrt(res)
end
function Krylov.kscal!(n::Integer, s::T, x::HaloVector{T}) where T <: FloatOrComplex
mx, nx = size(x.data)
_x = x.data
for i = 1:mx-1
for j = 1:nx-1
_x[i,j] = s * _x[i,j]
end
end
return x
end
function Krylov.kaxpy!(n::Integer, s::T, x::HaloVector{T}, y::HaloVector{T}) where T <: FloatOrComplex
mx, nx = size(x.data)
_x = x.data
_y = y.data
for i = 1:mx-1
for j = 1:nx-1
_y[i,j] += s * _x[i,j]
end
end
return y
end
function Krylov.kaxpby!(n::Integer, s::T, x::HaloVector{T}, t::T, y::HaloVector{T}) where T <: FloatOrComplex
mx, nx = size(x.data)
_x = x.data
_y = y.data
for i = 1:mx-1
for j = 1:nx-1
_y[i,j] = s * _x[i,j] + t * _y[i,j]
end
end
return y
end
function Krylov.kcopy!(n::Integer, y::HaloVector{T}, x::HaloVector{T}) where T <: FloatOrComplex
mx, nx = size(x.data)
_x = x.data
_y = y.data
for i = 1:mx-1
for j = 1:nx-1
_y[i,j] = _x[i,j]
end
end
return y
end
function Krylov.kfill!(x::HaloVector{T}, val::T) where T <: FloatOrComplex
mx, nx = size(x.data)
_x = x.data
for i = 1:mx-1
for j = 1:nx-1
_x[i,j] = val
end
end
return x
end
function Krylov.kref!(n::Integer, x::HaloVector{T}, y::HaloVector{T}, c::T, s::T) where T <: FloatOrComplex
mx, nx = size(x.data)
_x = x.data
_y = y.data
for i = 1:mx-1
for j = 1:nx-1
x_ij = _x[i,j]
y_ij = _y[i,j]
_x[i,j] = c * x_ij + s * y_ij
_x[i,j] = conj(s) * x_ij - c * y_ij
end
end
return x, y
end
```

Note that `Krylov.kref!` is only required for `minres_qlp`.

### 2D Poisson equation solver with Krylov methods

```@example halo-regions
using Krylov, OffsetArrays
# Parameters
L = 1.0 # Length of the square domain
Nx = 200 # Number of interior grid points in x
Ny = 200 # Number of interior grid points in y
Δx = L / (Nx + 1) # Grid spacing in x
Δy = L / (Ny + 1) # Grid spacing in y
# Define the source term f(x,y)
f(x,y) = -2 * π * π * sin(π * x) * sin(π * y)
# Create the matrix-free Laplacian operator
A = LaplacianOperator(Nx, Ny, Δx, Δy)
# Create the right-hand side
rhs = zeros(Float64, Nx+2, Ny+2)
data = OffsetArray(rhs, 0:Nx+1, 0:Ny+1)
for i in 1:Nx
for j in 1:Ny
xi = i * Δx
yj = j * Δy
data[i,j] = f(xi, yj)
end
end
b = HaloVector(data)
# Solve the system with CG
u_sol, stats = Krylov.cg(A, b, atol=1e-12, rtol=0.0, verbose=1)
```

```@example halo-regions
# The exact solution is u(x,y) = sin(πx) * sin(πy)
u_star = [sin(π * i * Δx) * sin(π * j * Δy) for i=1:Nx, j=1:Ny]
norm(u_sol.data[1:Nx, 1:Ny] - u_star, Inf)
```

### Conclusion

Implementing a 2D Poisson equation solver with `HaloVector` improves code clarity and efficiency.
Custom indexing with `OffsetArray` streamlines halo region management, eliminating boundary checks within the core loop.
This approach reduces branching, yielding faster execution, especially on large grids.
`HaloVector`'s flexibility also makes it easy to extend to 3D grids or more complex stencils.

!!! info
[Oceananigans.jl](https://github.com/CliMA/Oceananigans.jl) uses a similar strategy with its `Field` type, efficiently solving large linear systems with Krylov.jl.
4 changes: 4 additions & 0 deletions docs/src/matrix_free.md
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Expand Up @@ -284,7 +284,9 @@ A = FFTPoissonOperator(n, L, complex)
# Solve the linear system using CG
u_sol, stats = cg(A, f, atol=1e-10, rtol=0.0, verbose=1)
```

```@example fft_poisson
# The exact solution is u(x) = -sin(x)
u_star = -sin.(x)
u_star ≈ u_sol
Expand Down Expand Up @@ -418,7 +420,9 @@ f = vec(F)
# Solve the linear system using MinAres
u_sol, stats = minares(A, f, atol=1e-10, rtol=0.0, verbose=1)
```

```@example helmholtz
# Solution as 3D array
U_sol = reshape(u_sol, Nx, Ny, Nz)
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