xylar asay-davis matthew hecht, philip jones, mathew maltrud, christopher newman, mark petersen,...

17
Model for Prediction Across Scales (MPAS): Ocean Component Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere 2010 August 2010

Upload: mervin-bradley

Post on 13-Dec-2015

214 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

Model for Prediction Across Scales (MPAS): Ocean Component

Xylar Asay-DavisMatthew Hecht, Philip

Jones, Mathew Maltrud,

Christopher Newman, Mark Petersen, Todd

Ringler

Los Alamos National LabPDEs on the Sphere 2010

August 2010

Page 2: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

2X. Asay-Davis, et al.

ContributorsLANL: Xylar Asay-Davis, Matthew Hecht, Phil

Jones, Mark Petersen, Mat Maltrud, Chris Newman, Todd Ringler

NCAR: Michael Duda, Joe Klemp, Bill Skamarock

LLNL: Dan Bergmann, Art Mirin

USC: Lili Ju

FSU: Max Gunzburger, Doug Jacobsen

Page 3: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

3X. Asay-Davis, et al.

What is MPAS?1. MPAS is an unstructured-grid approach to

climate system modeling.

2. MPAS supports both quasi-uniform and variable resolution meshing of the sphere using quadrilaterals, triangles or Voronoi tessellations.

3. MPAS is a software framework for the rapid prototyping of single-components of climate system models (atmosphere, ocean, land ice, etc.)

4. MPAS offers the potential to explore regional-scale climate change within the context of global climate system

After testing, models will be distributed through SourceForge at http://mpas.sourceforge.net/.

Page 4: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

4X. Asay-Davis, et al.

MPAS is built on top of a finite-volume technique.

The finite-volume approach is a generalization of the Arakawa and Lamb (1981) energy and potential enstrophy conserving scheme.

In the shallow-water system, our approach conserves energy and potential vorticity while dissipating potential enstrophy (without dissipating energy).

Page 5: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

5X. Asay-Davis, et al.

MPAS will have access to several different high-order tracer transport algorithms, each with their appropriate flux-limiter.

Page 6: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

6X. Asay-Davis, et al.

Results from one high-order transport scheme.Snapshot at Day 5.Limiter turned off.

Conservative Transport Schemes for Spherical Geodesic Grid.

See Bill Skamarock’s talk tomorrow.

2nd-order

3rd-order 4th-order

Initial Condition

Page 7: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

7X. Asay-Davis, et al.

MPAS will have access to a high-order extension of Prather’s method-of-moments transport algorithm.The Characteristic Discontinuous Galerkin (CGD) method takes advantage of the Lagrangian nature of transport while maintaining a static mesh. (Lowrie, 2010)

The method has been extended to arbitrary convex polygons and to arbitrary order of accuracy. (Buonoi, Lowrie and Ringler 2010).

The method has also illuminated the connection between CDG and Prather’s Method-of-Moments.

Page 8: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

8X. Asay-Davis, et al.

MPAS Project Status: Ocean Summary1. Running MPAS with stretched lat-lon meshes with real-world

topography with a z-level vertical coordinate.

2. We have started the (2nd) evaluation of the barotropic-baroclinic splitting.

3. Code runs on 1 to 4096+ processors on a variety of platforms (MacBook Air, Lobo, Coyote, Ranger, Jaguar)

4. Ocean model can run in pure isopycnal mode as well as z-level mode.

5. We have tested and are implementing a high-order advection scheme (Skamarock)

6. Running ocean model with quasi-uniform and variable resolution Voronoi tessellations

Page 9: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

9X. Asay-Davis, et al.

POP to MPAS comparisonSubtropical gyres are weaker in MPAS by 30%.

We are checking parameter settings in each model to determine the source of this difference.

MPAS will not have checker-boarding.

POP MPAS

day

15

0ye

ar

6

Page 10: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

10X. Asay-Davis, et al.

MPAS: Ocean Voronoi TessellationsUniform and variable resolution Voronoi tessellations have been created at resolutions between 120 and 15 km.

Right: Global 15km mesh, PV shown, single-layer, flat bottom.

The meshes use nearest-neighbor search from ETOPO2 to define land/sea mask and ocean depth.

Page 11: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

11X. Asay-Davis, et al.

Movie

Variable Resolution Voronoi Tessellations

Page 12: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

12X. Asay-Davis, et al.

Variable Resolution Voronoi Tessellations

Mesh grid spacing varies by a factor of 8, ranging from 25 km to 200 km. This mesh has about 1/10 the number of nodes as the globally uniform 15 km mesh.

Page 13: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

13X. Asay-Davis, et al.

Variable Resolution Voronoi Tessellations

uniform mesh1,800,000 nodes

variable resolution mesh120,000 nodes

Page 14: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

14X. Asay-Davis, et al.

My Work: Immersed Boundary MethodIce Shelf/Ocean interface, coast lines and bathymetry

Used to represent complex and/or moving boundaries

Boundaries can intersect computational grid cells

Requires minimal modification of ocean model

Ocean

Ice Shelf

Page 15: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

15X. Asay-Davis, et al.

Radial Basis Functions (RBFs)Reconstruction of scalar and vector fields

Vector reconstruction:Based on Baudisch et

al. (2006).Only from normal

components at edgesExactly reproduces a

constant vector field

Page 16: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

16X. Asay-Davis, et al.

MPAS Ocean: Challenges Looking Forward1. Porting POP physics to MPAS

2. Obtaining quality simulations

3. Implementing barotropic-baroclinic splitting

4. Implementing high-order vertical remapping

5. Designing computationally efficient kernels

Page 17: Xylar Asay-Davis Matthew Hecht, Philip Jones, Mathew Maltrud, Christopher Newman, Mark Petersen, Todd Ringler Los Alamos National Lab PDEs on the Sphere

17X. Asay-Davis, et al.

Thanks!