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EARTHQUAKES (2): WAVEFORM MODELING, MOMENT TENSORS, & SOURCE PARAMETERS

EARTHQUAKES (2): WAVEFORM MODELING, MOMENT TENSORS, & SOURCE PARAMETERS

EARTHQUAKES (2): WAVEFORM MODELING, MOMENT TENSORS, & SOURCE PARAMETERS. Kikuchi and Kanamori, 1991. SOMETIMES FIRST MOTIONS DON’T CONSTRAIN FOCAL MECHANISM Especially likely when Few nearby stations, as in the oceans, so arrivals are near center of focal sphere

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764 views • 42 slides
Description of selected broadband ground motion simulation methods Paul Somerville, URS

Description of selected broadband ground motion simulation methods Paul Somerville, URS

Description of selected broadband ground motion simulation methods Paul Somerville, URS Yuehua Zeng, USGS Golden. Simulation Methods Described: 1. URS 2. Zeng 3. UCSB 4. SDSU. URS Hybrid Approach to Broadband Ground Motion Simulations ( Graves and Pitarka , 2004).

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531 views • 39 slides
Description of selected broadband ground motion simulation methods Paul Somerville, URS

Description of selected broadband ground motion simulation methods Paul Somerville, URS

Description of selected broadband ground motion simulation methods Paul Somerville, URS Yuehua Zeng, USGS Golden. Simulation Methods Described: 1. URS 2. Zeng 3. UCSB 4. SDSU. URS Hybrid Approach to Broadband Ground Motion Simulations ( Graves and Pitarka , 2004).

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391 views • 39 slides
Permitting Streamline Initiatives

Permitting Streamline Initiatives

Permitting Streamline Initiatives. Dianne Anderson Kate Brown. Review internal processes for improvements. Streamlining Approaches. Provide applicant tools (Direct Assistance Guidance) Increase application consistency/accuracy Create predictability for permitting expectations.

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356 views • 35 slides
Some statistics for high-energy astrophysics Andy Pollock European Space Agency

Some statistics for high-energy astrophysics Andy Pollock European Space Agency

Some statistics for high-energy astrophysics Andy Pollock European Space Agency XMM-Newton RGS Calibration Scientist Urbino Workshop in High-Energy Astrophysics 2008 July 31. with illustrations from XSPEC. Make every photon count. Account for every photon.

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320 views • 32 slides
P. Chung Nuclear Chemistry, SUNY, Stony Brook

P. Chung Nuclear Chemistry, SUNY, Stony Brook

Evidence for a long-range pion emission source in Au+Au Collisions at. P. Chung Nuclear Chemistry, SUNY, Stony Brook. Outline Motivation Brief Review of Correlation analysis methods Data Analysis & Results Correlation functions Source functions

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374 views • 28 slides
Massive Black Hole Mergers: As Sources and Simulations

Massive Black Hole Mergers: As Sources and Simulations

Massive Black Hole Mergers: As Sources and Simulations. John Baker Gravitational Astrophysics Laboratory NASA/GSFC. CGWP Sources & Simulations February 03, 2005. Massive Black Hole Mergers. MBHs are believed to lurk at centers of all galaxies with bulges

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307 views • 21 slides
Bulk Properties in Au+Au Collisions at ?s NN = 9.2 GeV in STAR Experiment at RHIC

Bulk Properties in Au+Au Collisions at ?s NN = 9.2 GeV in STAR Experiment at RHIC

Bulk Properties in Au+Au Collisions at ?s NN = 9.2 GeV in STAR Experiment at RHIC. Lokesh Kumar (for the STAR Collaboration) Panjab University, Chandigarh - India. Outline:. Motivation STAR Experiment and Collisions at ?s NN = 9.2 GeV

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371 views • 19 slides
Andrea Manconi , T.R. Walter M. Motagh, J. Ruch, M. Shirzaei, R. Wang & J. Zschau

Andrea Manconi , T.R. Walter M. Motagh, J. Ruch, M. Shirzaei, R. Wang & J. Zschau

Deformation sources derived from InSAR analysis at volcanoes: How realistic are the models?. Andrea Manconi , T.R. Walter M. Motagh, J. Ruch, M. Shirzaei, R. Wang & J. Zschau Helmholtz Centre GFZ Potsdam, Telegrafenberg, 14473 Potsdam (Germany). Volcanic unrest:

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281 views • 18 slides
Zadonina E.O. (1) , Caldeira B. (1,2) , Bezzeghoud M. (1,2), Borges J.F. (1,2)

Zadonina E.O. (1) , Caldeira B. (1,2) , Bezzeghoud M. (1,2), Borges J.F. (1,2)

I. Slip distribution, co-seismic deformation and Coulomb stress change for the 12 May 2008 Wenchuan (China, M w 7.9 ) earthquake II. Influence of model parameters on synthesized high-frequency strong-motion waveforms.

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263 views • 18 slides
Project S5 High resolution multi-disciplinary monitoring of active fault test-sites areas in Italy

Project S5 High resolution multi-disciplinary monitoring of active fault test-sites areas in Italy

WP 4.3 Estimates of earthquakes source parameters and structure characteristics from massive seismic waveform analysis. Project S5 High resolution multi-disciplinary monitoring of active fault test-sites areas in Italy.

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278 views • 17 slides
An Introduction to Simulink

An Introduction to Simulink

An Introduction to Simulink. Marios S. Pattichis. Configuration Parameters. Simulink is designed to be a front-end tool for integrating ordinary differential equations (ODEs). So, you need to keep sampling issues in mind:

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The unknowns are: xo = source location d = source depth

The unknowns are: xo = source location d = source depth

Werner deconvolution, like Euler deconvolution, is more properly thought of as an inverse method: we analyze the observed magnetic field and solve for source parameters.

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Event selection at lower incident energies

Event selection at lower incident energies

Exists a strong correlation between all impact parameter dependent observables. Possible to exclude peripheral collisions by gates on N c or E t. Event selection at lower incident energies. NPA A548 (1992) 489. QMD+SMM:Two-step hybrid model comparisons. E * /A the : Charge distribution

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131 views • 4 slides
UNIVERSITY OF ATHENS Faculty of Geology and Geoenvironment

UNIVERSITY OF ATHENS Faculty of Geology and Geoenvironment

UNIVERSITY OF ATHENS Faculty of Geology and Geoenvironment Department of Geophysics and Geothermics. ABSTRACT

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90 views • 1 slides

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