EBS 506: Special Topics Estuarine Turbidity maximum Instructor: António Baptista.

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EBS 506: Special Topics Estuarine Turbidity maximum Instructor: António Baptista

Transcript of EBS 506: Special Topics Estuarine Turbidity maximum Instructor: António Baptista.

Page 1: EBS 506: Special Topics Estuarine Turbidity maximum Instructor: António Baptista.

EBS 506: Special Topics

Estuarine Turbidity maximum

Instructor: António Baptista

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“CMOP: Transforming Ocean Exploration”

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Key questions

• What is an Estuarine Turbidity Maximum (ETM) ?

• Which estuaries does it occur on?

• What causes it?

• Why is it important?

• How can it be: observed? modeled ?

• How does it vary in space and time ?

• How does it affect: estuarine productivity ? microbial communities ?

• How is it affected by: climate? human activities?

• What does it look like in the Columbia River estuary?

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SATURN-01SATURN-03

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CR open benchmark

Goals Enable continuous enhancement of multiple models and exploration of diverse

modeling strategies

Design requirements Maximize value-added expertise of model developers/expert users, while minimizing

their time investment Dynamic timeframes (blending controlled hindcasts with continuous blind forecasts) Focus on unstructured grid models

Implementation phases– CMOP-driven SELFE pilot (on-going)– CMOP-assisted pilots for other lead models with by-invitation participation of the

respective developers / expert users (a ~12 month effort)– Open to community (early 2010) and consider exporting to other coastal margins

(2011)

Enablers– CMOP’s SATURN modeling system & Rapid Deployment Forecasting System– OpenDAP-CF standards for unstructured grid models (synergistic effort led by Rich

Signell, with participation of at least the FVCOM, ADCIRC, SELFE, ELCIRC communities)

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Open Columbia River benchmark

Goals

Enablers

Phases

Concept

Color Key

Goals Enable continuous enhancement of multiple models and exploration of diverse modeling strategies Maximize value-added expertise of model developers/expert users, while minimizing their time investment

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Code registration

• Open to open-source community unstructured-grid codes, allowing for realistic ocean/atmospheric/river forcing– Version(s) supported by the code developers– Opendap-CF compliant grids, outputs, and atmospheric/ocean inputs– Liaison person to the SATURN team by the developers/expert users;

liaison should be available to support the registration process and to create a default

• Preferences– MPI version available

• Code/version specific parameter interface

What to do with old versions?• Kkkk

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Registration & refinement of modeling strategy

• All registered codes go through this step• Static benchmark

– Ideally 4 weeks (with two warm-up weeks) representing a Q transition

• Modeling strategy (CR.nnn.mmm.ggg.ppp.qqqq)

– nnn: Code (001: SELFE; 002. FVCOM; 003. ADCIRC)– mmm: code version– ggg: Grid (001: DB14; 002: DB16; 003: hires)– ppp: Turbulence closure (001: k-kl)– qqq: Other elements

• Skill and performance assessment– SA metrics – Feature representation– CPU , memory

• What to save after a simulation– Input files (as necessary to recreate simulation)– Skill and performance assessment metrics

• Rankings (per objective?)– Overall; by model; by grid

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“CMOP: Transforming Ocean Exploration”

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