H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary...

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H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA, 02139. 15 August, 2011 15 August, 2011 TRAVEL TIME CALCULATIONS 1

Transcript of H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary...

Page 1: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi ToksozH. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz

Department of Earth Atmospheric and Planetary Sciences,

Massachusetts Institute of Technology,

Cambridge,MA, 02139.

15 August, 201115 August, 2011

TRAVEL TIME CALCULATIONS

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Page 2: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

Classification of Ray Tracing Methods for TT calculation

1 - Analytic solutions for 1-D models

  --Direct Analytical solution (Snell’s Law)

-- Tau-P method Solutions expressed as integrals over depth (Buland and Chapman,

1983)

3D 2- Shortest (fastest) time methods (Solve: Travel time = minimum) Fermat’s Law

  -- Two -point ray bending ( Um and Thurber, 1987, Zhao et al, 1992; Zhao and Lei,

2004)

-- Finite difference (propagate grid of times from source) (Ferra and Madariaga, 1987,

Moser 1991, Podvin and Lecomte, 1991)

3- Eikonal solvers (Solve: | gradient of travel time | = slowness)

-- Finite difference (grid of times) (Vidale, 1990, Podvin and Lecomte, 1991)

  -- Fast marching (grid of times) (Rawlinson and Sambridge, 2004.)

4- Ray shooters (Solve: ray equations) (differential equations for ray trajectory)

  -- Dynamic ray tracing (Cerveny, Molotkov and Psencik)2

Page 3: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

Direct Analytical Calculation and Microseismic Model

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Depth(m) Distance(m) E1 155 60.96 E2 80 106.68 E3 50 152.40

Page 4: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

Calculate First Arrivals

1 D: Tau- P

3 D: Bending Method

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Page 5: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

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Page 6: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

Bending (Pseudo Bending) ray tracing

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Page 7: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

Three-point perturbationTravel time by summation along the segments of ray path:

Offset direction:

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Page 8: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

Illustration of pseudo-bending algorithm

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Page 9: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

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Page 10: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

Dynamic Ray Tracing

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Calculate ALL (required) Arrivals

Page 11: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

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Page 12: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

Definition of layers and Solution of

Differential Equation System:,

APPROXIMATION OF VELOCITY DISTRIBUTION.

MM=0... BICUBIC SPLINE INTERPOLATION.

MM=1... LINEAR VERTICAL INTERPOLATION BETWEEN ISOVELOCITY INTERFACES.

MM=2... PIECE-WISE BILINEAR INTERPOLATION

THE SHOOTING METHOD IS USED. TO PERFORM ITERATIONS, VARIOUS METHODS CAN BE APPLIED:

METHOD=0... REGULA FALSI.

METHOD=1... COMBINATION OF REGULA FALSI METHOD AND METHOD OF HALVING INTERVALS.

METHOD=2... HALVING OF INTERVALS.

METHOD=3... METHOD BASED ON PARAXIAL RAY APPROXIMATION.

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Page 13: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

Velocity Model

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Page 14: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

3 3

2

1

3

2

1

2

2-1;5; 3,2,2,2,1

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1 ;4; 3,3,2,,1

Page 15: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

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2

1

2

1

2

2 2

1

1;5; 3,2,2,2,1

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1;6; 1,2,2,2,2,1

Page 16: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

Time

MODE: 0, 1, 1

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Page 17: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

MODE: 0, 1, 1 and 1, 2, 1, 1

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Page 18: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

MODE: 0, 1, 1 / 1, 2, 1, 1 /1 4 1 2 2 1

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Page 19: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

MODE: 0 1 1 / 1 2 1 1/ -1 2 1 1/1 4 1 2 2 1/ 1 6 1 2 2 2 2 1

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Page 20: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

Mode:0 1 1/1 2 1 1/-1 2 1 1/1 4 1 2 2 1/1 6 1 2 2 2 2 1/1 4 1 -2 -2 1:

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Page 21: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

Mode:0 1 1/1 2 1 1/-1 2 1 1/1 4 1 2 2 1/1 6 1 2 2 2 2 1/1 4 1 -2 -2

1

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Page 22: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

For Event 1 (E1) Dynamic Ray Tracing TT.

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Page 23: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

For Event E1 Analytical solution, Bending, Tau_P and DRT

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Page 24: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

PROGRAM SEIS88 IS DESIGNED FOR THE COMPUTATION OF RAYS OF SEISMIC WAVES WHICH ARRIVE AT A SYSTEM OF RECEIVERS DISTRIBUTED REGULARLY OR IRREGULARLY ALONG THE EARTH'S SURFACE, ALONG AN INTERFACE,OR ALONG A VERTICAL PROFILE. THE GENERATION OF WAVES IS SEMI-AUTOMATIC. AT RECEIVERS, CORRESPONDING TRAVEL TIMES ARE AUTOMATICALLY DETERMINED. OPTIONALLY, AMPLITUDES AND PHASE SHIFTS MAY BE EVALUATED. EFFECTS OF A SLIGHT ABSORPTION MAY BE ALSO CONSIDERED. ALL THESE QUANTITIES ARE STORED AND MAY BE OPTIONALLY PLOTTED OR USED FOR THE COMPUTATION OF SYNTHETIC SEISMOGRAMS. ALL THE DIRECT AND PRIMARY REFLECTED WAVES P AND S, INCLUDING THE CONVERTED WAVES AT THE POINT OF REFLECTION, CAN BE GENERATED AUTOMATICALLY. MULTIPLE REFLECTIONS OF ARBITRARY TYPE ARE OPTIONALLY GENERATED MANUALLY (BY INPUT DATA).

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THE AMPLITUDES OF P, SV AND SH WAVES ARE EVALUATED BY STANDARD RAY FORMULAE. NO MODIFICATIONS ARE APPLIED IN SINGULAR REGIONS. THE PURE HEAD WAVES GENERALLY DO NOT EXIST IN LATERALLY INHOMOGENEOUS MEDIA WITH CURVED INTERFACES AND ARE NOT CONSIDERED IN SEIS88. THEY MIGHT BE, OF COURSE,SIMULATED BY SLIGHTLY REFRACTED WAVES.

Calculation of Dynamic Ray Tracing “PROGRAM SEIS88”

Page 25: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

GEOMETRICAL SPREADING IS DETERMINED BY SOLVING A SYSTEM OF TWO LINEAR ORDINARY DIFFERENTIAL EQUATIONS OF FIRST ORDER (SO CALLED DYNAMIC RAY TRACING SYSTEM) BY A MODIFIED EULER'S METHOD. SLIGHT ABSORPTION MAY BE CONSIDERED. IN THIS CASE, A GLOBAL ABSORPTION FACTOR(QUANTITY OBTAINED AS A TIME INTEGRAL OF 1/Q ALONG A RAY, WHERE Q IS A QUALITY FACTOR) IS ALSO EVALUATED.

PROGRAM SEIS88 IS SUPPLEMENTED BY PROGRAMS FOR PREPARATION OF DATA FOR VELOCITY MODEL (PROGRAM SMOOTH), TO COMPUTE SYNTHETIC SEISMOGRAMS (PROGRAM SYNTPL), AND TO PLOT RAYS, TRAVEL-TIME AND AMPLITUDE-DISTANCE CURVES (PROGRAM RAYPLOT), SYNTHETIC SEIS-MOGRAMS (PROGRAM SEISPLOT) OR PARTICLE MOTION DIAGRAMS (PROGRAM POLARPLOT).

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Page 26: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

THANK YOU

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Page 27: H. Sadi Kuleli, W Rodi, Fuxian Song, M. Nafi Toksoz Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge,MA,

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