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SPICE workshop Venice 2004

SPICESeismic wave Propagation and Imaging in Complex media: a European network

Welcome to Venice!Welcome to Venice!

First Research and Training workshop

Sep 25 – Oct 2, 2004

First Research and Training workshop

Sep 25 – Oct 2, 2004

SPICE workshop Venice 2004

SPICESeismic wave Propagation and Imaging in Complex media: a European network

Thanks to

The local organizers: Geza Seriani, Angela Marchetto and son, Sergio Persoglia , Erika Vye, and many others!

The lecturers: Raul Madariaga, Jose Carcione, Jean-Pierre Vilotte, Peter Moczo, Geza Seriani, Ekkehart Tessmer, Dan Givoli, Roberto Gori, Giovanni Erbacci

SPICE workshop Venice 2004

SPICESeismic wave Propagation and Imaging in Complex

media: a European network

• Why SPICE?• Wave propagation across spatial scales• The role of numerical methods• Parallelization and supercomputers

• What is SPICE?• The Network• The Task Groups• Workshops and Meetings• The Digital Library• Involvement

• Why SPICE?• Wave propagation across spatial scales• The role of numerical methods• Parallelization and supercomputers

• What is SPICE?• The Network• The Task Groups• Workshops and Meetings• The Digital Library• Involvement

SPICE workshop Venice 2004

Motivation

• There is a wide gap between theoretical/numerical and observational seismology

• Computational power is now such that 3D numerical approaches to wave propagation will enter routine data fitting procedures (e.g. source or structural imaging) or monitoring

• The scientific value of 3D simulation data is continuously increasing (e.g. earthquake scenario simulations, global wave propagation)

• There is little or no infrastructure supporting software development and large data volume handling in the Earth science community

• The community in computational seismology is fragmented

• There is a wide gap between theoretical/numerical and observational seismology

• Computational power is now such that 3D numerical approaches to wave propagation will enter routine data fitting procedures (e.g. source or structural imaging) or monitoring

• The scientific value of 3D simulation data is continuously increasing (e.g. earthquake scenario simulations, global wave propagation)

• There is little or no infrastructure supporting software development and large data volume handling in the Earth science community

• The community in computational seismology is fragmented

Why SPICE?

SPICE workshop Venice 2004

Observations: diffractions at the CMBObservations: diffractions at the CMB

Data compilation by Ed Garnero, Arizona State University.

Data compilation by Ed Garnero, Arizona State University.

SPICE workshop Venice 2004

Computational seismology on all scales

• Lab scale (e.g. modelling high-frequency seismograms from fracturing experiments)

• Volcano seismology, Reservoir wave propagation

• Dynamic rupture propagation, earthquake scenario simulation

• Continental and planetary scale, global wave propagation

• Lab scale (e.g. modelling high-frequency seismograms from fracturing experiments)

• Volcano seismology, Reservoir wave propagation

• Dynamic rupture propagation, earthquake scenario simulation

• Continental and planetary scale, global wave propagation

0.1m

10km

100-1000km

>1000km

Methodology used is converging!

Why SPICE?

SPICE workshop Venice 2004

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Elastic wave equations

Parallelisation

Grid

3D Model

SimulationSynthetic seismograms

Numerical simulation of seismic wave propagationNumerical simulation of seismic wave propagation

Why SPICE?

SPICE workshop Venice 2004

Computers and waves Computers and waves

Computational power has reached a state wherewe can expect to numerically simulate 3D wave fields in the observed frequency bands.

Local seismology: 5x5x5km 10 Hz

Regional seismology: 150x150x80km 2 Hz

Global seismology (sections): 1 sGlobal seismology (whole): 5 s

Computational power has reached a state wherewe can expect to numerically simulate 3D wave fields in the observed frequency bands.

Local seismology: 5x5x5km 10 Hz

Regional seismology: 150x150x80km 2 Hz

Global seismology (sections): 1 sGlobal seismology (whole): 5 s

Cut-off frequencySimulations like this require O(10-100)

GB RAM and parallel programming

Simulations like this require O(10-100) GB RAM and parallel programming

Why SPICE?

SPICE workshop Venice 2004

What is (was) missing? What is (was) missing?

- Earth Sciences curriculae usually do not provide training in numerical methods and/or parallel programming.

- There is little interaction between the more applied side of wave propagation (exploration) and the more general seismology (even though methodologies are very similar)

- We envisage substantial increase in the use of 3D methods in all fields of wave propagation

- Seismologists need a toolbox with verified open-source codes for 3D wave propagation

- Earth Sciences curriculae usually do not provide training in numerical methods and/or parallel programming.

- There is little interaction between the more applied side of wave propagation (exploration) and the more general seismology (even though methodologies are very similar)

- We envisage substantial increase in the use of 3D methods in all fields of wave propagation

- Seismologists need a toolbox with verified open-source codes for 3D wave propagation

Why SPICE?

SPICE workshop Venice 2004

What is SPICE?The partners

What is SPICE?The partners

What is SPICE?

SPICE workshop Venice 2004

SPICE Task GroupsSPICE Task Groups

What is SPICE?

• TG: Electronic library• Standards for synthetic data storage• Digital library with codes, training material• Connecting to GRID projects• www-pages

• TG: Research and Training Workshops • Workshop organization

• TG: Planetary and continental scale• Forward modelling tools• Imaging benchmark

• TG: Local scale• Dynamic rupture modelling• Toolbox for rupture problems

• TG: Small scale • Understanding seismic sources in volcanoes• Wave propagation through mushy layers (sea floor)

• TG: Electronic library• Standards for synthetic data storage• Digital library with codes, training material• Connecting to GRID projects• www-pages

• TG: Research and Training Workshops • Workshop organization

• TG: Planetary and continental scale• Forward modelling tools• Imaging benchmark

• TG: Local scale• Dynamic rupture modelling• Toolbox for rupture problems

• TG: Small scale • Understanding seismic sources in volcanoes• Wave propagation through mushy layers (sea floor)

SPICE workshop Venice 2004

SPICE WorkshopsSPICE Workshops

What is SPICE?

2004: Venice International University, Sep 25 – Oct 2• Numerical methods applied to wave

propagation• Lectures and training

2005: Smolenice Castle, Czech Republic, Sep 4 – 10• Large scale simulations, parallelization,

applications• Lectures, training, and presentations

2006: Ireland, time and place to be announced• Inverse problems in seismology• Lectures, training, and presentations

2007: Cargese, Corsica, time to be announced• Multidisciplinary research meeting

2004: Venice International University, Sep 25 – Oct 2• Numerical methods applied to wave

propagation• Lectures and training

2005: Smolenice Castle, Czech Republic, Sep 4 – 10• Large scale simulations, parallelization,

applications• Lectures, training, and presentations

2006: Ireland, time and place to be announced• Inverse problems in seismology• Lectures, training, and presentations

2007: Cargese, Corsica, time to be announced• Multidisciplinary research meeting

SPICE workshop Venice 2004

SPICE Special sessionscomputational seismology

SPICE Special sessionscomputational seismology

What is SPICE?

2004: EGU Meeting, Nice

2005: EGU Meeting, Venice

2007: EGU/EAGE Meeting

2004: EGU Meeting, Nice

2005: EGU Meeting, Venice

2007: EGU/EAGE Meeting

SPICE workshop Venice 2004

SPICE Digital LibrarySPICE Digital Library

What is SPICE?

• Open-source codes for wave propagation problems

• Related training material for various methodologies (material from workshops)

• Facilities for synthetic data storage and recovery (e.g. format converters)

• Synthetic data base (e.g. earthquake scenarios, synthetics for large earthquakes)

• Open-source codes for wave propagation problems

• Related training material for various methodologies (material from workshops)

• Facilities for synthetic data storage and recovery (e.g. format converters)

• Synthetic data base (e.g. earthquake scenarios, synthetics for large earthquakes)

SPICE workshop Venice 2004

Involvement in SPICEInvolvement in SPICE

What is SPICE?

• Workshops and special sessions

• Participation in task groups, collaboration with SPICE partners

• Research visits to SPICE partners (can be funded)

• Use of code library and training material

• Sign up to SPICE newsletter

• Participate in SPICE Newsgroup (to be installed)

• Feedback on workshops, training, www pages, etc.

• Workshops and special sessions

• Participation in task groups, collaboration with SPICE partners

• Research visits to SPICE partners (can be funded)

• Use of code library and training material

• Sign up to SPICE newsletter

• Participate in SPICE Newsgroup (to be installed)

• Feedback on workshops, training, www pages, etc.

SPICE workshop Venice 2004

Seismic wave Propagation and Imaging in Complex media: a European network

Enjoy the workshop!Enjoy the workshop!

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