Lecture 9

Agenda
📚 Multi-xPU thermal porous convection 3D
💻 Automatic documentation an CI
🚧 Project:

  • Multi-xPU thermal porous convection 3D

  • Automatic documentation and CI


Content

👉 get started with exercises


Projects - 3D thermal porous convection on multi-xPU

The goal of this lecture 9:

Using ImplicitGlobalGrid.jl (continued)

In previous Lecture 8, we introduced ImplicitGlobalGrid.jl, which renders distributed parallelisation with GPU and CPU for HPC a very simple task.

Also, ImplicitGlobalGrid.jl elegantly combines with ParallelStencil.jl to, e.g., hide communication behind computation.

Let's have a rapid tour of ImplicitGlobalGrid.jl's' documentation before using it to turn the 3D thermal porous diffusion solver into a multi-xPU solver.

Multi-xPU 3D thermal porous convection

Let's step through the following content:

👉 You'll find a version of the PorousConvection_3D_xpu.jl code in the solutions folder on Moodle after exercises deadline if needed to get you started.

Enable multi-xPU support

Only a few changes are required to enable multi-xPU support, namely:

  1. Copy your working PorousConvection_3D_xpu.jl code developed for the exercises in Lecture 7 and rename it PorousConvection_3D_multixpu.jl.

  2. Add at the beginning of the code

using ImplicitGlobalGrid
import MPI
  1. Further, add global maximum computation using MPI reduction function to be used instead of maximum()

max_g(A) = (max_l = maximum(A); MPI.Allreduce(max_l, MPI.MAX, MPI.COMM_WORLD))
  1. In the # numerics section, initialise the global grid right after defining nx,ny,nz and use now global grid nx_g(),ny_g() and nz_g() for defining maxiter and ncheck, as well as in any other places when needed.

nx,ny       = 2 * (nz + 1) - 1, nz
me, dims    = init_global_grid(nx, ny, nz)  # init global grid and more
b_width     = (8, 8, 4)                     # for comm / comp overlap
  1. Modify the temperature initialisation using ImplicitGlobalGrid's global coordinate helpers (x_g, etc...), including one internal boundary condition update (update halo):

T  = @zeros(nx, ny, nz)
T .= Data.Array([ΔT * exp(-(x_g(ix, dx, T) + dx / 2 - lx / 2)^2
                          -(y_g(iy, dy, T) + dy / 2 - ly / 2)^2
                          -(z_g(iz, dz, T) + dz / 2 - lz / 2)^2) for ix = 1:size(T, 1), iy = 1:size(T, 2), iz = 1:size(T, 3)])
T[:, :, 1  ] .=  ΔT / 2
T[:, :, end] .= -ΔT / 2
update_halo!(T)
T_old = copy(T)
  1. Prepare for visualisation, making sure only me==0 creates the output directory. Also, prepare an array for storing inner points only (no halo) T_inn as well as global array to gather subdomains T_v

if do_viz
    ENV["GKSwstype"]="nul"
    if (me==0) if isdir("viz3Dmpi_out")==false mkdir("viz3Dmpi_out") end; loadpath="viz3Dmpi_out/"; anim=Animation(loadpath,String[]); println("Animation directory: $(anim.dir)") end
    nx_v, ny_v, nz_v = (nx - 2) * dims[1], (ny - 2) * dims[2], (nz - 2) * dims[3]
    (nx_v * ny_v * nz_v * sizeof(Data.Number) > 0.8 * Sys.free_memory()) && error("Not enough memory for visualization.")
    T_v   = zeros(nx_v, ny_v, nz_v) # global array for visu
    T_inn = zeros(nx - 2, ny - 2, nz - 2) # no halo local array for visu
    xi_g, zi_g = LinRange(-lx / 2 + dx + dx / 2, lx / 2 - dx - dx / 2, nx_v), LinRange(-lz + dz + dz / 2, -dz - dz / 2, nz_v) # inner points only
    iframe = 0
end
  1. Moving to the time loop, add halo update function update_halo! after the kernel that computes the fluid fluxes. You can additionally wrap it in the @hide_communication block to enable communication/computation overlap (using b_width defined above)

@hide_communication b_width begin
    @parallel compute_Dflux!(qDx, qDy, qDz, Pf, T, k_ηf, _dx, _dy, _dz, αρg, _1_θ_dτ_D)
    update_halo!(qDx, qDy, qDz)
end
  1. Apply a similar step to the temperature update, where you can also include boundary condition computation as following (⚠️ no other construct is currently allowed)

@hide_communication b_width begin
    @parallel update_T!(T, qTx, qTy, qTz, dTdt, _dx, _dy, _dz, _1_dt_β_dτ_T)
    @parallel (1:size(T, 2), 1:size(T, 3)) bc_x!(T)
    @parallel (1:size(T, 1), 1:size(T, 3)) bc_y!(T)
    update_halo!(T)
end
  1. Use now the max_g function instead of maximum to collect the global maximum among all local arrays spanning all MPI processes. Use it in the timestep dt definition and in the error calculation (instead of maximum).

# time step
dt = if it == 1
    0.1 * min(dx, dy, dz) / (αρg * ΔT * k_ηf)
else
    min(5.0 * min(dx, dy, dz) / (αρg * ΔT * k_ηf), ϕ * min(dx / max_g(abs.(qDx)), dy / max_g(abs.(qDy)), dz / max_g(abs.(qDz))) / 3.1)
end
  1. Make sure all printing statements are only executed by me==0 in order to avoid each MPI process to print to screen, and use nx_g() instead of local nx in the printed statements when assessing the iteration per number of grid points.

  2. Update the visualisation and output saving part

# visualisation
if do_viz && (it % nvis == 0)
    T_inn .= Array(T)[2:end-1, 2:end-1, 2:end-1]; gather!(T_inn, T_v)
    if me == 0
        p1 = heatmap(xi_g, zi_g, T_v[:, ceil(Int, ny_g() / 2), :]'; xlims=(xi_g[1], xi_g[end]), ylims=(zi_g[1], zi_g[end]), aspect_ratio=1, c=:turbo)
        # display(p1)
        png(p1, @sprintf("viz3Dmpi_out/%04d.png", iframe += 1))
        save_array(@sprintf("viz3Dmpi_out/out_T_%04d", iframe), convert.(Float32, T_v))
    end
end
  1. Finalise the global grid before returning from the main function

finalize_global_grid()
return

If you made it up to here, you should now be able to launch your PorousConvection_3D_multixpu.jl code on multiple GPUs. Let's give it a try 🔥

Make sure to have set following parameters:

lx,ly,lz    = 40.0, 20.0, 20.0
Ra          = 1000
nz          = 63
nx,ny       = 2 * (nz + 1) - 1, nz
b_width     = (8, 8, 4) # for comm / comp overlap
nt          = 500
nvis        = 50

Benchmark run

Then, launch the script on Piz Daint on 8 GPU nodes upon adapting the the runme_mpi_daint.sh or sbatch sbatch_mpi_daint.sh scripts (see here) 🚀

The final 2D slice (at ny_g()/2) produced should look as following and the code takes about 25min to run:

3D porous convection MPI

3D calculation

Running the code at higher resolution (508x252x252 grid points) and for 6000 timesteps produces the following result

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Documenting your code

This lecture we will learn:

comic

Why should I document my code?

Why should I write code comments?

Why should I write documentation?

Documentation easily rots...

Worse than no documentation/code comments is documentation which is outdated.

I find the best way to keep documentation up to date is:

Documentation tools: doc-strings

A Julia doc-string (Julia manual):

"Typical size of a beer crate"
const BEERBOX = 12
?BEERBOX

Documentation tools: doc-strings with examples

One can add examples to doc-strings (they can even be part of testing: doc-tests).

(Run it in the REPL and copy paste to the docstring.)

"""
    transform(r, θ)

Transform polar `(r,θ)` to cartesian coordinates `(x,y)`.

# Example
```jldoctest
julia> transform(4.5, pi/5)
(3.6405764746872635, 2.6450336353161292)
```
"""
transform(r, θ) = (r*cos(θ), r*sin(θ))
?transform

Documentation tools: GitHub markdown rendering

The easiest way to write long-form documentation is to just use GitHub's markdown rendering.

A nice example is this short course by Ludovic (incidentally about solving PDEs on GPUs 🙂).

👉 this is a good and low-overhead way to produce pretty nice documentation

Documentation tools: Literate.jl

There are several tools which render .jl files (with special formatting) into markdown files. These files can then be added to GitHub and will be rendered there.

Example

Literate.markdown("car_travels.jl", directory_of_this_file, execute=true, documenter=false, credit=false)

But this is not automatic! Manual steps: run Literate, add files, commit and push...

or use GitHub Actions...

Documentation tools: Automating Literate.jl

Demonstrated in the repo course-101-0250-00-L8Documentation.jl

name: Run Literate.jl
# adapted from https://lannonbr.com/blog/2019-12-09-git-commit-in-actions

on: push

jobs:
  lit:
    runs-on: ubuntu-latest
    steps:
      # Checkout the branch
      - uses: actions/checkout@v2

      - uses: julia-actions/setup-julia@v1
        with:
          version: '1.9'
          arch: x64

      - uses: julia-actions/cache@v1
      - uses: julia-actions/julia-buildpkg@latest

      - name: run Literate
        run: QT_QPA_PLATFORM=offscreen julia --color=yes --project -e 'cd("scripts"); include("literate-script.jl")'

      - name: setup git config
        run: |
          # setup the username and email. I tend to use 'GitHub Actions Bot' with no email by default
          git config user.name "GitHub Actions Bot"
          git config user.email "<>"

      - name: commit
        run: |
          # Stage the file, commit and push
          git add scripts/md/*
          git commit -m "Commit markdown files fom Literate"
          git push origin master

Documentation tools: Documenter.jl

If you want to have full-blown documentation, including, e.g., automatic API documentation generation, versioning, then use Documenter.jl.

Examples:

Notes:

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Exercises - lecture 9

⚠️ Warning!
Exercise 1 is the final step of your project - scripts and results should be added to the PorousConvection subfolder in your private GitHub repo. The git commit hash (or SHA) of the final push needs to be uploaded on Moodle (more).
From your homework-7 branch, create a new git branch named homework-9 in order to build upon work performed for homework 7.
The exercises from Lecture 9 are include the last steps towards the completion of the project. Hand-in information can be found in Logistics.

Exercise 1 — Multi-xPU computing projects

👉 See Logistics for submission details.

The goal of this exercise is to:

In this exercise, you will:

👉 You'll find a version of the PorousConvection_3D_xpu.jl code on Moodle after exercises deadline if needed to get you started.

  1. Copy the PorousConvection_3D_xpu.jl code from exercises in Lecture 7 and rename it PorousConvection_3D_multixpu.jl.

  2. Refer to the steps outlined in the Multi-xPU 3D thermal porous convection section from Lecture 9 to implement the changes needed to port the 3D single xPU code (from Lecture 7) to multi-xPU.

  3. Upon completion, verify the script converges and produces expected output for following parameters:

lx,ly,lz    = 40.0, 20.0, 20.0
Ra          = 1000
nz          = 63
nx,ny       = 2 * (nz + 1) - 1, nz
b_width     = (8, 8, 4) # for comm / comp overlap
nt          = 500
nvis        = 50

Use 8 GPUs on Piz Daint adapting the runme_mpi_daint.sh or sbatch sbatch_mpi_daint.sh scripts (see here) to use CUDA-aware MPI 🚀

The final 2D slice (at ny_g()/2) produced should look similar as the figure depicted in Lecture 9.

Task

Now that you made sure the code runs as expected, launch PorousConvection_3D_multixpu.jl for 2000 steps on 8 GPUs at higher resolution (global grid of 508x252x252) setting:

nz          = 127
nx,ny       = 2 * (nz + 1) - 1, nz
nt          = 2000
nvis        = 100

and keeping other parameters unchanged.

Use sbtach command to launch a non-interactive job which may take about 5h30-6h to execute.

Produce a figure or animation showing the final stage of temperature distribution in 3D and add it to a new section titled ## Porous convection 3D MPI in the PorousConvection project subfolder's README.md. You can use the Makie visualisation helper script from Lecture 7 for this purpose (making sure to adapt the resolution and other input params if needed).

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Exercise 2 — Automatic documentation in Julia

👉 See Logistics for submission details.

The goal of this exercise is to:

One task you've already done, namely to update the README.md of this set of exercises!

Tasks:

  1. Add doc-string to the functions of following scripts:

    • PorousConvection_3D_xpu.jl

    • PorousConvection_3D_multixpu.jl

  2. Add to the PorousConvection folder a Literate.jl script called bin_io_script.jl that contains and documents following save_array and load_array functions you may have used in your 3D script

"""
Some docstring
"""
function save_array(Aname,A)
    fname = string(Aname,".bin")
    out = open(fname,"w"); write(out,A); close(out)
end

"""
Some docstring
"""
function load_array(Aname,A)
    fname = string(Aname,".bin")
    fid=open(fname,"r"); read!(fid,A); close(fid)
end

Add to the bin_io_script.jl a main() function that will:

B = main()
heatmap(B)
  1. Make the Literate-based workflow to automatically build on GitHub using GitHub Actions. For this, you need to add to the .github/workflow folder (the one containing your CI.yml for testing) the Literate.yml script which we saw in this lecture's section Documentation tools: Automating Literate.jl.

  2. That's all! Head to the Project section in Logistics for a check-list about what you should hand in for this first project.

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