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COSMO - Dynamical Core Rewrite Approach, Rewrite and Status Tobias GysiPowerPoint Presentation

COSMO - Dynamical Core Rewrite Approach, Rewrite and Status Tobias Gysi

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COSMO - Dynamical Core Rewrite Approach, Rewrite and Status Tobias Gysi

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COSMO - Dynamical Core Rewrite

Approach, Rewrite and Status

Tobias Gysi

POMPA Workshop, Manno, 3.5.2011

Supercomputing Systems AGFon +41 43 456 16 00

Technopark 1Fax +41 43 456 16 10

8005 Zürichwww.scs.ch

Challenge

- Assuming that the COSMO code will continue run on commodity processors in the next couple of years, what is the performance improvement we can achieve by rewriting the dynamical core?
Boundary Conditions

- Do not touch the underlying physical model (i.e. equations that are being solved)
- Formulas must remain as they are
- Arbitrary ordering of computations, etc. may change
- Results must remain ‘identical’ to ‘a very high level of accuracy’

- Part of an initiative looking at all parts of the COSMO code.
Support

- Support from & direct interaction with MeteoSwiss, DWD, CSCS, C2SM

Feasibility Study

Lib. Design

Rewrite

Test

Tune

CPU

GPU

t

~2 Years

Feasibility

Library

Test & Tune

You Are Here

- Get to know the code
- Understand performance characteristics
- Find computational motives
- Stencil
- Tri-Diagonal Solver

- Implement a prototype code
- Relevant part of the dynamical core (Fast Wave Solver, ~30% of total runtime)
- Try to optimize for x86
- No MPI parallelization

- Implemented in C++
- Optimize for memory-bandwidth utilization
- Avoid pre-computation, do computation on the fly
- Merge loops accessing the common variables
- Use iterators rather than full index calculation on 3D grid
- Store data contiguous in ‘k-direction’ (vertical columns)

The performance difference is NOT due to programming language but due to code optimizations!

- A performance increase of 2x has been achieved on a representative part of the code
- Main optimizations identified (for scalar processors)
- Avoid pre-calculation whenever possible
- Merge loops
- Change the storage order to k-first

- Performance is all about memory bandwidth

Write a code that

- Delivers the right results
- Dedicated unit-tests & verification framework

- Apply the performance optimization strategies used in the prototype
- Can be developed within a year to run on x86 and GPU platforms
- Mandatory: support three-level parallelism in a very flexible way
- Vector processing units (e.g. SSE)
- Multi-core node (sub-domain)
- Multiple nodes (domain) - not part of the SCS project

- Optional: write one single code that can be compiled to both platforms

- Mandatory: support three-level parallelism in a very flexible way

Write a code that

- Facilitates future improvements in terms of
- New models / algorithms
- Portability to new computer architectures

- Can and will be integrated by the COSMO consortium into the main branch

- It is challenging to develop a stencil library
- There is no big chunk of work that can be hidden behind a API call (e.g. matrix multiplication)
- The actual update function of the stencil is heavily application specific and performance critical
- We use a DSEL like approach (Domain Specific Embedded Language)
- “Stencil language” embedded in C++
- Separate description of loop logic and update function
- During compile time generate optimized C++ code(possible due to C++ meta programming capabilities)

- Parallelization on the node level is done by
- Splitting the calculation domain into blocks (IJ-Plane)
- Parallelize the work over the blocks
- Double buffering avoids concurrency issues

- The library allows the definition of multiple stages per stencil
- Stages are update functions applied consecutively to one block
- As a block is typically much smaller than the complete domain we can leverage the caches of the CPU

- Calculation on the fly is supported using a combination of stages and column buffers
- Column buffers are fields with the size of one block local to every CPU core
- A first stage writes to a buffer while a second stage consumes the pre-calculated values

1. Naive

for k

a(k) := b(k) + c(k)

end

...

for k

d(k) := a(k-1)*e(-1) +

a(k)*e(0) +

a(k+1)*e(+1)

end

...

for k

f(k) := a(k)*g(k) + d(k)

end

1. Naive

for k

a(k) := b(k) + c(k)

end

...

for k

d(k) := a(k-1)*e(-1) +

a(k)*e(0) +

a(k+1)*e(+1)

end

...

for k

f(k) := a(k)*g(k) + d(k)

end

2. No pre-calculation

for k

d(k) := (b(k-1)+c(k-1))*e(-1) + (b(k)+c(k))*e(0) +

(b(k+1)+c(k+1))*e(+1)

f(k) := (b(k)+c(k))*g(k) + d(k)

end

1. Naive

for k

a(k) := b(k) + c(k)

end

...

for k

d(k) := a(k-1)*e(-1) +

a(k)*e(0) +

a(k+1)*e(+1)

end

...

for k

f(k) := a(k)*g(k) + d(k)

end

3. Pre-calculation with temporary variables

for k

z := b(k+1) + c(k+1)

d(k) := x*e(-1) +

y*e(0) +

z*e(+1)

f(k) := y*g(k) + d(k)

x:=y

y:=z

end

4. Pre-calculation with column buffer

for k

a(k) := b(k) + c(k)

end

for k

d(k) := a(k-1)*e(-1) +

a(k)*e(0) +

a(k+1)*e(+1)

f(k) := a(k)*g(k) + d(k)

end

1. Naive

for k

a(k) := b(k) + c(k)

end

...

for k

d(k) := a(k-1)*e(-1) +

a(k)*e(0) +

a(k+1)*e(+1)

end

...

for k

f(k) := a(k)*g(k) + d(k)

end

1. Naive

for k

a(k) := b(k) + c(k)

end

...

for k

d(k) := a(k-1)*e(-1) +

a(k)*e(0) +

a(k+1)*e(+1)

end

...

for k

f(k) := a(k)*g(k) + d(k)

end

5. Pre-calculation with stages & column Buffer

Stencil

Stage 1

a := b + c

Stage 2

d := a*e (k:-1,0,1)

Stage 3

f := a*g + d

Apply Stencil

- So far the following stencils have been implemented:
- Fast wave solver (w bottom boundary initialization missing)
- Advection
- 5th order advection
- Bott 2 advection (cri implementation missing)

- Complete tendencies
- Horizontal Diffusion
- Coriolis

- The next steps are:
- Implicit vertical diffusion
- Put it all together
- Performance optimization

Acknowledgements to all our collaborators at

- C2SM (Center for Climate Systems Modeling)
- MeteoSwiss
- DWD (DeutscherWetterdienst)
- CSCS