Lab 4: Kirchhoff migration (Matlab version)

Size: px
Start display at page:

Download "Lab 4: Kirchhoff migration (Matlab version)"

Transcription

1 Due Date: Oktober 29th, 2012 TA: Mandy Wong Lab 4: Kirchhoff migration (Matlab version) Robert U. Terwilliger 1 ABSTRACT In this computer exercise you will modify the Kirchhoff migration and modeling subroutine that was presented in class. First you will limit the propagation angles in the subroutine, and then you will modify the routine to handle v(z). INTRODUCTION The subroutine kirchfast performs migration by summing input data along a hyperbolic trajectory, and modeling by spraying out along a hyperbolic trajectory. Later on in this course you will study the phenomena of operator aliasing. This occurs when operator moveout across adjacent traces exceeds the time sampling rate. Cycle skips occur and the operator is aliased. For a moveout curve with slope dt/dx, and data with a spatial Nyquist frequency of k n, temporal frequencies above are aliased. ω = k n dt/dx Later in the course you will learn about more sophisticated ways of dealing with operator aliasing. In this exercise you will observe the phenomena and deal with it by limiting the slope of the moveout curve. The criteria for limiting the curve will be based on the maximum angle of propagation that you will allow to be migrated. In Chapter 7 of Basic Earth Imaging (BEI) you learned that the ratio of first arrival time on a hyperbola to any other arrival time gives the cosine of the angle of propagation. After coding up the angle-limited migration and testing it on a simple synthetic, you will modify the subroutine to handle depth variable velocity. Your new program will be used to migrate a near-offset section from the Gulf of Mexico. 1 robert@terwilliger.com

2 BEI - Lab 4 2 Kirchhoff EXERCISE This lab is, once again, available online. First download the source code for this lab, lab4 matlab.tar from the BEI class webpage, and save it in the appropriate directory. Then type tar -xvf lab4 matlab.tar to create your Lab4 matlab directory. From your workstation, log onto ssh Xusername@cees tool.stanford.edu and continue to Part 1. To build the first copy of paper.pdf, type make default first and then type make paper. Edit the file paper.tex to answer questions. Part 1 Angle-limited migration The subroutine kirchfast is a version of the fast Kirchhoff modeling and migration routine presented in Chapter 5 of BEI. The routine has been modified to include a variable called amax which is passed from the main program Kapp.m. You should not have to make any modifications to Kapp.m. Edit kirchfast.m so that only the energy which is propagating at angles less than amax is migrated or modeled. On the matlab prompt, type run Kapp to rebuild the figure. Save the figure as Fig/migmodel.pdf to include in this paper. Sharp operator truncations can also cause artifacts in a final image. The Gibbs effect (ringing) is an example of this problem caused by truncation in the Fourier domain. If you are feeling ambitious (or are a SEP student) you can further improve the operator. Instead of truncating the operator at amax, apply a taper, so its amplitude decreases to zero over a small range. Part 2 Field data and v(z) You will now migrate the near-offset section of the Gulf of Mexico data. Figure 5 is an angle-limited migration with a depth variable velocity function. Your objective in this section is to make Figure 4 look better than Figure 5. Don t worry about the fact that you are migrating a near-offset section as if it were a zero-offset section. The approximation is good enough for our purposes. On your Matlab prompt, type run kirmiggom to see a movie of migration as a function of maximum propagation angle (amax). When you watch the movie, notice how the migrated image changes. As angle increases you should see the flanks of the salt dome getting resolved better. As angle increases you will also see more aliasing artifacts. These artifacts appear as systematic dipping noise and as precursors above the first arrival. Before you choose the best frame to include as your final answer, you need to improve the migration velocity function. The current velocity is shown in Figure 3. In kirmiggom.m, choose values for the parameters vwater, alpha, beta, and twater. Use what you have learned in Chapters 3 and 4 about typical Gulf of Mexico v(z)

3 BEI - Lab 4 3 Kirchhoff sections. In order to include the new velocity function, you will have to save the velocity figure with the name Fig/velgulf.pdf Finally edit the parameter slice in kirmiggom.m to choose which frame to include in the report you hand in. Save the best migrated figure with the name Fig/Gulfmig.pdf. QUESTIONS You should edit paper.tex file to answer the following questions. Don t forget to add your name. Question 1 Imagine that you have a seismic survey which corresponds to the geometry and propagation velocity of Figures 1 and 2. What is the maximum angle of propagation that can be observed from a reflection point at two way travel time depth τ = 0.3s and horizontal position x = 640m? How about travel time depth τ = 0.6s and horizontal position x = 640m? Question 2 Watch the migration movie of the Gulf data and describe your observations How does the image change as the angle changes? What kind of changes do you see in different parts of the section? How did adding v(z) change the image? What criteria did you use to select the frame for Figure 4. Question 3 Aperture limitation is sometimes used to avoid aliasing in Kirchhoff migration. What would you change in kirchfast() to limit the spatial size of the aperture and not the angular size. (Don t do it, just tell me what you would change)? What would be the advantage and/or disadvantage of aperture limitation compared to angle limitation?

4 BEI - Lab 4 4 Kirchhoff Question 4 Kirchhoff operators can be implemented as either push operators or pull operators. The forward operator for kirchfast models data by looping over its input space and pushing data along hyperbolas. The adjoint operation, migration, is done by looping over the output space and pulling in data from hyperbolas in the input space. 1. A different subroutine could be written that does Kirchhoff migration by looping over the dataspace and pushing it out along semi-circles (ellipses for v(z)) above it. What would the adjoint operation of this be? 2. Although mathematically equivalent, what would you think are the implementation advantages of push operators vs pull operators? (HINT: Think irregular data) 3. Can the forward and adjoint parts of an operator both be push operators or both be pull operators? 4. Extra Credit: With a green pen mark all spelling and gramar error s in this Lab. Also comment on confusing statements in the Lab or other broken and outdated features/questions. HAND IN When you are all done, type make paper at the shell prompt to rebuild a pdf version of this lab. Print out a copy of your homework and hand it in to your TA s office or it to the TA. filt subroutine in matlab PROGRAMS

5 BEI - Lab 4 5 Kirchhoff % K i r c h h o f f migration and d i f f r a c t i o n % adj = 0, forward operation, data = data + L modl, L i s the K i r c h h o f f % modeling o p e r a t o r % adj = 1, a d j o i n t operation, modl = modl + L data, L i s the K i r c h h o f f % migration o p e r a t or % amax = maximum propagation angle in d e g r e e s f u n c t i o n [ modl, data ]= k i r c h f a s t ( adj, add, v e l h a l f, amax, t0, dt, dx, nt, nx, modl, data ) i f ( add==0) i f ( adj==0) data = z e r o s ( nt, nx ) ; else modl = z e r o s ( nt, nx ) ; pi = 2 acos ( 0. 0 ) ; r2d = 180./ pi ; % loop over o f f s e t for ih= nx : nx h = dx ih ; % h = o f f s e t % loop over t r a v e l time depth for i z =2: nt z = t0 + dt ( iz 1); % z= t r a v e l time depth %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % make chnages to handle v ( z ) media %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% t = s q r t ( z ˆ2 + ( h/ v e l h a l f ( 1 ) ) ˆ 2 ) ; % c a l c u l a t e the corresponding two way t r a v e l i t = f l o o r ( ( t t0 )/ dt ) ; % f i n d the index o f the t r a v e l time in the d i f ( i t > nt ) % i f out o f bounds, break break ; amp = ( z / t ) s q r t ( nt dt / t ) ; % weighting f u n c t i o n %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % add your l i n e s here, you w i l l have to modify the % weighting f u n c t i o n to make i t as a f u n c t i o n o f maximum % migration angle : amax %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% x s t a r t = max( f l o o r (1 ih ), 1 ) ; % x s t a r t and x d e f i n e the migration / modeling x = min ( f l o o r ( nx ih ), nx ) ; i f ( adj == 0) % i f modeling, we g e nerate the data for i x=x s t a r t : x data ( i t, i x+ih)=data ( i t, i x+ih)+modl ( iz, i x ) amp ; else % i f migration, we produce the model

6 BEI - Lab 4 6 Kirchhoff for i x=x s t a r t : x modl ( iz, i x )=modl ( iz, i x )+data ( i t, i x+ih ) amp ; return

7 BEI - Lab 4 7 Kirchhoff 0 Migration 0 Diffraction time [s] 0.6 time [s] x [m] x [m] Figure 1: After you have modified kirchfast() your migration and modeling result should look like Figure 2.

8 BEI - Lab 4 8 Kirchhoff 0 Migration 0 Diffraction time [s] 0.6 time [s] x [m] x [m] Figure 2: The answer: Migration and modeling limited to 45 propagation angle. Your task is to make Figure 1 look like this.

9 BEI - Lab 4 9 Kirchhoff Figure 3: Velocity function used for migrations.

10 BEI - Lab 4 10 Kirchhoff Figure 4: Migration of the Gulf of Mexico data.

11 BEI - Lab 4 11 Kirchhoff Figure 5: What you have to beat: Limited angle migration with preliminary depth variable velocity function.

Lab 5: 2D FFT (Fortran version)

Lab 5: 2D FFT (Fortran version) Due Date: 17:00, Tuesday, November 1, 2011 TA: Xukai Shen (xukai@sep.stanford.edu) Lab 5: 2D FFT (Fortran version) Conrad Schlumberger 1 ABSTRACT In this lab you will modify programs to filter data based

More information

Lab 1-1-D Gradient Operator

Lab 1-1-D Gradient Operator Due Date: 17:00, Friday, October 7, 2011 TA: Yunyue Elita Li (yunyue.li@sep.stanford.edu) Lab 1-1-D Gradient Operator William of Orange 1 ABSTRACT The gradient of a continuous function of more than one

More information

Moveout, velocity, and stacking

Moveout, velocity, and stacking Moveout, velocity, and stacking Jon Claerbout In this chapter we handle data as though the earth had no dipping reflectors. The earth model is one of stratified layers with velocity a (generally increasing)

More information

Matrix formulation of adjoint Kirchhoff datuming

Matrix formulation of adjoint Kirchhoff datuming Stanford Exploration Project, Report 80, May 15, 2001, pages 1 377 Matrix formulation of adjoint Kirchhoff datuming Dimitri Bevc 1 ABSTRACT I present the matrix formulation of Kirchhoff wave equation datuming

More information

Seismic Wave Propagation: HW2 Due 13/5

Seismic Wave Propagation: HW2 Due 13/5 Reading: Scales Chapter 5.1-5.3, 6, 7, 9, Kallweit and Wood (198), Schneider (1978) Problems.1-.8 should be done on your own. You may work together to solve problems.9-.10, but you must hand in your own

More information

Introduction. Pre-Lab Questions: Physics 1CL PERIODIC MOTION - PART II Fall 2009

Introduction. Pre-Lab Questions: Physics 1CL PERIODIC MOTION - PART II Fall 2009 Introduction This is the second of two labs on simple harmonic motion (SHM). In the first lab you studied elastic forces and elastic energy, and you measured the net force on a pendulum bob held at an

More information

Dipping Layer Refraction Problem Moveout and Coincident Source-Receiver Format

Dipping Layer Refraction Problem Moveout and Coincident Source-Receiver Format Environmental and Exploration Geophysics II Dipping Layer Refraction Problem Moveout and Coincident Source-Receiver Format tom.h.wilson tom.wilson@mail.wvu.edu Department of Geology and Geography West

More information

Compensating visco-acoustic effects in anisotropic resverse-time migration Sang Suh, Kwangjin Yoon, James Cai, and Bin Wang, TGS

Compensating visco-acoustic effects in anisotropic resverse-time migration Sang Suh, Kwangjin Yoon, James Cai, and Bin Wang, TGS Compensating visco-acoustic effects in anisotropic resverse-time migration Sang Suh, Kwangjin Yoon, James Cai, and Bin Wang, TGS SUMMARY Anelastic properties of the earth cause frequency dependent energy

More information

Reversible Stolt migration

Reversible Stolt migration Reversible Stolt migration William A. Burnett Robert J. Ferguson ABSTRACT The nonstationary equivalent of the Fourier shift results in a general one-dimensional integral transform that applies to many

More information

Physics I : Oscillations and Waves Prof. S. Bharadwaj Department of Physics and Meteorology Indian Institute of Technology, Kharagpur

Physics I : Oscillations and Waves Prof. S. Bharadwaj Department of Physics and Meteorology Indian Institute of Technology, Kharagpur Physics I : Oscillations and Waves Prof. S. Bharadwaj Department of Physics and Meteorology Indian Institute of Technology, Kharagpur Lecture - 21 Diffraction-II Good morning. In the last class, we had

More information

Homework Assignment 4 Root Finding Algorithms The Maximum Velocity of a Car Due: Friday, February 19, 2010 at 12noon

Homework Assignment 4 Root Finding Algorithms The Maximum Velocity of a Car Due: Friday, February 19, 2010 at 12noon ME 2016 A Spring Semester 2010 Computing Techniques 3-0-3 Homework Assignment 4 Root Finding Algorithms The Maximum Velocity of a Car Due: Friday, February 19, 2010 at 12noon Description and Outcomes In

More information

Continuum Limit and Fourier Series

Continuum Limit and Fourier Series Chapter 6 Continuum Limit and Fourier Series Continuous is in the eye of the beholder Most systems that we think of as continuous are actually made up of discrete pieces In this chapter, we show that a

More information

Summary. Introduction

Summary. Introduction Detailed velocity model building in a carbonate karst zone and improving sub-karst images in the Gulf of Mexico Jun Cai*, Hao Xun, Li Li, Yang He, Zhiming Li, Shuqian Dong, Manhong Guo and Bin Wang, TGS

More information

Homework 1. Johan Jensen ABSTRACT. 1. Theoretical questions and computations related to digital representation of numbers.

Homework 1. Johan Jensen ABSTRACT. 1. Theoretical questions and computations related to digital representation of numbers. Homework 1 Johan Jensen This homework has three parts. ABSTRACT 1. Theoretical questions and computations related to digital representation of numbers. 2. Analyzing digital elevation data from the Mount

More information

Modeling the Motion of a Projectile in Air

Modeling the Motion of a Projectile in Air In this lab, you will do the following: Modeling the Motion of a Projectile in Air analyze the motion of an object fired from a cannon using two different fundamental physics principles: the momentum principle

More information

10.3 Parametric Equations. 1 Math 1432 Dr. Almus

10.3 Parametric Equations. 1 Math 1432 Dr. Almus Math 1432 DAY 39 Dr. Melahat Almus almus@math.uh.edu OFFICE HOURS (212 PGH) MW12-1:30pm, F:12-1pm. If you email me, please mention the course (1432) in the subject line. Check your CASA account for Quiz

More information

EXPERIMENT 7: ANGULAR KINEMATICS AND TORQUE (V_3)

EXPERIMENT 7: ANGULAR KINEMATICS AND TORQUE (V_3) TA name Lab section Date TA Initials (on completion) Name UW Student ID # Lab Partner(s) EXPERIMENT 7: ANGULAR KINEMATICS AND TORQUE (V_3) 121 Textbook Reference: Knight, Chapter 13.1-3, 6. SYNOPSIS In

More information

Introduction. Pre-Lab Questions: Physics 1CL PERIODIC MOTION - PART II Spring 2009

Introduction. Pre-Lab Questions: Physics 1CL PERIODIC MOTION - PART II Spring 2009 Introduction This is the second of two labs on simple harmonic motion (SHM). In the first lab you studied elastic forces and elastic energy, and you measured the net force on a pendulum bob held at an

More information

Chapter 7. Seismic imaging. 7.1 Assumptions and vocabulary

Chapter 7. Seismic imaging. 7.1 Assumptions and vocabulary Chapter 7 Seismic imaging Much of the imaging procedure was already described in the previous chapters. An image, or a gradient update, is formed from the imaging condition by means of the incident and

More information

Experiment 4 Free Fall

Experiment 4 Free Fall PHY9 Experiment 4: Free Fall 8/0/007 Page Experiment 4 Free Fall Suggested Reading for this Lab Bauer&Westfall Ch (as needed) Taylor, Section.6, and standard deviation rule ( t < ) rule in the uncertainty

More information

LAB 3: VELOCITY AND ACCELERATION

LAB 3: VELOCITY AND ACCELERATION Lab 3 - Velocity & Acceleration 25 Name Date Partners LAB 3: VELOCITY AND ACCELERATION A cheetah can accelerate from to 5 miles per hour in 6.4 seconds. A Jaguar can accelerate from to 5 miles per hour

More information

Immersed Boundary Method Assignment

Immersed Boundary Method Assignment Immersed Boundary Method Assignment This assignment is modification of the immersed boundary code that I downloaded from the course website. I constructed new IB objects with changing ibinit.m and afibdriver.m.

More information

LAB 3: WORK AND ENERGY

LAB 3: WORK AND ENERGY 1 Name Date Lab Day/Time Partner(s) Lab TA (CORRECTED /4/05) OBJECTIVES LAB 3: WORK AND ENERGY To understand the concept of work in physics as an extension of the intuitive understanding of effort. To

More information

Stanford Exploration Project, Report 115, May 22, 2004, pages

Stanford Exploration Project, Report 115, May 22, 2004, pages Stanford Exploration Project, Report 115, May 22, 2004, pages 249 264 248 Stanford Exploration Project, Report 115, May 22, 2004, pages 249 264 First-order lateral interval velocity estimates without picking

More information

Lab 1: Handout GULP: an Empirical energy code

Lab 1: Handout GULP: an Empirical energy code Lab 1: Handout GULP: an Empirical energy code We will be using the GULP code as our energy code. GULP is a program for performing a variety of types of simulations on 3D periodic solids, gas phase clusters,

More information

Laboratory handout 5 Mode shapes and resonance

Laboratory handout 5 Mode shapes and resonance laboratory handouts, me 34 82 Laboratory handout 5 Mode shapes and resonance In this handout, material and assignments marked as optional can be skipped when preparing for the lab, but may provide a useful

More information

SUMMARY ANGLE DECOMPOSITION INTRODUCTION. A conventional cross-correlation imaging condition for wave-equation migration is (Claerbout, 1985)

SUMMARY ANGLE DECOMPOSITION INTRODUCTION. A conventional cross-correlation imaging condition for wave-equation migration is (Claerbout, 1985) Comparison of angle decomposition methods for wave-equation migration Natalya Patrikeeva and Paul Sava, Center for Wave Phenomena, Colorado School of Mines SUMMARY Angle domain common image gathers offer

More information

Lab 1: Handout GULP: an Empirical energy code

Lab 1: Handout GULP: an Empirical energy code 3.320/SMA 5.107/ Atomistic Modeling of Materials Spring 2003 1 Lab 1: Handout GULP: an Empirical energy code We will be using the GULP code as our energy code. GULP is a program for performing a variety

More information

AP Physics 1 Summer Assignment Packet

AP Physics 1 Summer Assignment Packet AP Physics 1 Summer Assignment Packet 2017-18 Welcome to AP Physics 1 at David Posnack Jewish Day School. The concepts of physics are the most fundamental found in the sciences. By the end of the year,

More information

Experiment 2. F r e e F a l l

Experiment 2. F r e e F a l l Suggested Reading for this Lab Experiment F r e e F a l l Taylor, Section.6, and standard deviation rule in Taylor handout. Review Chapters 3 & 4, Read Sections 8.1-8.6. You will also need some procedures

More information

LivePhoto Physics Activity 3. Velocity Change. Motion Detector. Sample

LivePhoto Physics Activity 3. Velocity Change. Motion Detector. Sample LivePhoto Physics Activity 3 Name: Date: Analyzing Position vs. Time Graphs: The most fundamental measurements of motion involve the determination of an object s location at a series of times. A very effective

More information

Deconvolution imaging condition for reverse-time migration

Deconvolution imaging condition for reverse-time migration Stanford Exploration Project, Report 112, November 11, 2002, pages 83 96 Deconvolution imaging condition for reverse-time migration Alejandro A. Valenciano and Biondo Biondi 1 ABSTRACT The reverse-time

More information

SEISMIC WAVE PROPAGATION. Lecture 2: Fourier Analysis

SEISMIC WAVE PROPAGATION. Lecture 2: Fourier Analysis SEISMIC WAVE PROPAGATION Lecture 2: Fourier Analysis Fourier Series & Fourier Transforms Fourier Series Review of trigonometric identities Analysing the square wave Fourier Transform Transforms of some

More information

Project 2: Using linear systems for numerical solution of boundary value problems

Project 2: Using linear systems for numerical solution of boundary value problems LINEAR ALGEBRA, MATH 124 Instructor: Dr. T.I. Lakoba Project 2: Using linear systems for numerical solution of boundary value problems Goal Introduce one of the most important applications of Linear Algebra

More information

Name(s): Date: Course/Section: Mass of the Earth

Name(s): Date: Course/Section: Mass of the Earth Name(s): Date: Course/Section: Grade: Part 1: The Angular Size of the Earth Mass of the Earth Examine the image on the lab website. The image of the Earth was taken from the Moon on Aug 23, 1966 by Lunar

More information

LAB 3: GLOBAL SEISMOLOGY

LAB 3: GLOBAL SEISMOLOGY NAME: LAB TIME: LAB 3: GLOBAL SEISMOLOGY This lab will introduce you to the basic concepts of global seismology and the Earth s interior structure. This is a hybrid assignment: some aspects can be done

More information

Static and Kinetic Friction

Static and Kinetic Friction Ryerson University - PCS 120 Introduction Static and Kinetic Friction In this lab we study the effect of friction on objects. We often refer to it as a frictional force yet it doesn t exactly behave as

More information

LAB 3 - VELOCITY AND ACCELERATION

LAB 3 - VELOCITY AND ACCELERATION Name Date Partners L03-1 LAB 3 - VELOCITY AND ACCELERATION OBJECTIVES A cheetah can accelerate from 0 to 50 miles per hour in 6.4 seconds. Encyclopedia of the Animal World A Jaguar can accelerate from

More information

MAT 343 Laboratory 6 The SVD decomposition and Image Compression

MAT 343 Laboratory 6 The SVD decomposition and Image Compression MA 4 Laboratory 6 he SVD decomposition and Image Compression In this laboratory session we will learn how to Find the SVD decomposition of a matrix using MALAB Use the SVD to perform Image Compression

More information

Lab Partner(s) TA Initials (on completion) EXPERIMENT 7: ANGULAR KINEMATICS AND TORQUE

Lab Partner(s) TA Initials (on completion) EXPERIMENT 7: ANGULAR KINEMATICS AND TORQUE TA name Lab section Date TA Initials (on completion) Name UW Student ID # Lab Partner(s) EXPERIMENT 7: ANGULAR KINEMATICS AND TORQUE 117 Textbook Reference: Walker, Chapter 10-1,2, Chapter 11-1,3 SYNOPSIS

More information

Elements of 3D Seismology Second Edition

Elements of 3D Seismology Second Edition Elements of 3D Seismology Second Edition Copyright c 1993-2003 All rights reserved Christopher L. Liner Department of Geosciences University of Tulsa August 14, 2003 For David and Samantha And to the memory

More information

Exploring Operations Involving Complex Numbers. (3 + 4x) (2 x) = 6 + ( 3x) + +

Exploring Operations Involving Complex Numbers. (3 + 4x) (2 x) = 6 + ( 3x) + + Name Class Date 11.2 Complex Numbers Essential Question: What is a complex number, and how can you add, subtract, and multiply complex numbers? Explore Exploring Operations Involving Complex Numbers In

More information

(latitudinal form of solar radiation. The part in parentheses is the 2 nd Legendre polynomial, a polynomial that integrates to zero over the sphere)

(latitudinal form of solar radiation. The part in parentheses is the 2 nd Legendre polynomial, a polynomial that integrates to zero over the sphere) PCC 587 Project 1: Write-up due October 22, 2009 Energy Balance Climate Model This handout describes the first project, and hopefully explains enough to make it work for everyone! If you have questions

More information

Complex-beam Migration and Land Depth Tianfei Zhu CGGVeritas, Calgary, Alberta, Canada

Complex-beam Migration and Land Depth Tianfei Zhu CGGVeritas, Calgary, Alberta, Canada Page 1 of 10 Home Articles Interviews Print Editions Complex-beam Migration and Land Depth Tianfei Zhu CGGVeritas, Calgary, Alberta, Canada DECEMBER 2012 FOCUS ARTICLE Summary Gaussian-beam depth migration

More information

2.4 Investigating Symmetry

2.4 Investigating Symmetry Name Class Date 2.4 Investigating Symmetry Essential Question: How do you determine whether a figure has line symmetry or rotational symmetry? 1 Explore 1 Identifying Line Symmetry A figure has symmetry

More information

Project IV Fourier Series

Project IV Fourier Series Project IV Fourier Series Robert Jerrard Goal of the project To develop understanding of how many terms of a Fourier series are required in order to well-approximate the original function, and of the differences

More information

Basic principles of the seismic method

Basic principles of the seismic method Chapter 2 Basic principles of the seismic method In this chapter we introduce the basic notion of seismic waves. In the earth, seismic waves can propagate as longitudinal (P) or as shear (S) waves. For

More information

Attenuation compensation in least-squares reverse time migration using the visco-acoustic wave equation

Attenuation compensation in least-squares reverse time migration using the visco-acoustic wave equation Attenuation compensation in least-squares reverse time migration using the visco-acoustic wave equation Gaurav Dutta, Kai Lu, Xin Wang and Gerard T. Schuster, King Abdullah University of Science and Technology

More information

Exploring Fourier Transform Techniques with Mathcad Document 1: Introduction to the Fourier Transform

Exploring Fourier Transform Techniques with Mathcad Document 1: Introduction to the Fourier Transform Exploring Fourier Transform Techniques with Mathcad Document : Introduction to the Fourier Transform by Mark Iannone Department of Chemistry Millersville University Millersville, PA 7-3 miannone@maraudermillersvedu

More information

Projects in Geometry for High School Students

Projects in Geometry for High School Students Projects in Geometry for High School Students Goal: Our goal in more detail will be expressed on the next page. Our journey will force us to understand plane and three-dimensional geometry. We will take

More information

Questions for the Edwards formation

Questions for the Edwards formation Name: Professor name: Class Time: The Virtual Field trip is to be completed by your self. You should not work with a partner. This is not group work. Nor should you search for answers on the internet.

More information

Reflection Seismic Method

Reflection Seismic Method Reflection Seismic Method Data and Image sort orders; Seismic Impedance; -D field acquisition geometries; CMP binning and fold; Resolution, Stacking charts; Normal Moveout and correction for it; Stacking;

More information

CSE 331 Winter 2018 Homework 1

CSE 331 Winter 2018 Homework 1 Directions: - Due Wednesday, January 10 by 11 pm. - Turn in your work online using gradescope. You should turn in a single pdf file. You can have more than one answer per page, but please try to avoid

More information

Physics 411: Homework 3

Physics 411: Homework 3 Physics 411: Homework 3 Because of the cancellation of class on January 28, this homework is a double-length homework covering two week s material, and you have two weeks to do it. It is due in class onthursday,

More information

COMP344 Digital Image Processing Fall 2007 Final Examination

COMP344 Digital Image Processing Fall 2007 Final Examination COMP344 Digital Image Processing Fall 2007 Final Examination Time allowed: 2 hours Name Student ID Email Question 1 Question 2 Question 3 Question 4 Question 5 Question 6 Total With model answer HK University

More information

AOS 452 Lab 13 Handout Upper-Level Frontogenesis and Sawyer-Eliassen Circulations

AOS 452 Lab 13 Handout Upper-Level Frontogenesis and Sawyer-Eliassen Circulations AOS 452 Lab 13 Handout Upper-Level Frontogenesis and Sawyer-Eliassen Circulations Introduction As we discussed in class, fronts are locations at which we cannot ignore the effects of ageostrophy. Furthermore,

More information

Complete all the identification fields below or 10% of the lab value will be deduced from your final mark for this lab.

Complete all the identification fields below or 10% of the lab value will be deduced from your final mark for this lab. Simple circuits 3 hr Identification page Instructions: Print this page and the following ones before your lab session to prepare your lab report. Staple them together with your graphs at the end. If you

More information

Mechanics Lecture Notes

Mechanics Lecture Notes Mechanics Lecture Notes Lectures 0 and : Motion in a circle. Introduction The important result in this lecture concerns the force required to keep a particle moving on a circular path: if the radius of

More information

3D beam prestack depth migration with examples from around the world

3D beam prestack depth migration with examples from around the world A Publication of Petroleum Geo-Services Vol. 8 No. 8 August 2008 3D beam prestack depth migration with examples from around the world Introduction In 1999 AGS specialized in 2D seismic depth processing.

More information

LAB 5: ROTATIONAL DYNAMICS

LAB 5: ROTATIONAL DYNAMICS 1 Name Date Day/Time of Lab Partner(s) Lab TA OBJECTIVES LAB 5: ROTATIONAL DYNAMICS To investigate and understand moment of inertia as it relates to rotational motion. To relate angular and linear position,

More information

Stanford Exploration Project, Report 97, July 8, 1998, pages

Stanford Exploration Project, Report 97, July 8, 1998, pages Stanford Exploration Project, Report 97, July 8, 998, pages 7 6 Stanford Exploration Project, Report 97, July 8, 998, pages 7 The offset-midpoint traveltime pyramid in transversely isotropic media Tariq

More information

PHYSICS 3266 SPRING 2016

PHYSICS 3266 SPRING 2016 PHYSICS 3266 SPRIG 2016 Each problem is worth 5 points as discussed in the syllabus. For full credit you must include in your solution a copy of your program (well commented and listed any students that

More information

Phys 531 Lecture 27 6 December 2005

Phys 531 Lecture 27 6 December 2005 Phys 531 Lecture 27 6 December 2005 Final Review Last time: introduction to quantum field theory Like QM, but field is quantum variable rather than x, p for particle Understand photons, noise, weird quantum

More information

Motion II. Goals and Introduction

Motion II. Goals and Introduction Motion II Goals and Introduction As you have probably already seen in lecture or homework, and if you ve performed the experiment Motion I, it is important to develop a strong understanding of how to model

More information

QMUL, School of Physics and Astronomy Date: 18/01/2019

QMUL, School of Physics and Astronomy Date: 18/01/2019 QMUL, School of Physics and stronomy Date: 8//9 PHY Mathematical Techniques Solutions for Exercise Class Script : Coordinate Systems and Double Integrals. Calculate the integral: where the region is defined

More information

The Euler Method for the Initial Value Problem

The Euler Method for the Initial Value Problem The Euler Method for the Initial Value Problem http://people.sc.fsu.edu/ jburkardt/isc/week10 lecture 18.pdf... ISC3313: Introduction to Scientific Computing with C++ Summer Semester 2011... John Burkardt

More information

Lab #8: The Unbalanced Wheel

Lab #8: The Unbalanced Wheel Lab #8: The Unbalanced Wheel OBJECTIVE Use observations to calculate the radius of gyration of a wheel. Apply energy models to the dynamics of an unbalanced rotating wheel. Learn new computing skills.

More information

Designing Information Devices and Systems I Spring 2019 Homework 11

Designing Information Devices and Systems I Spring 2019 Homework 11 Last Updated: 2019-04-12 23:38 1 EECS 16A Designing Information Devices and Systems I Spring 2019 Homework 11 This homework is due April 19, 2019, at 23:59. Self-grades are due April 23, 2019, at 23:59.

More information

PROBLEM SET #1. Galactic Structure 37 pts total. due Tuesday, 2/19/2019

PROBLEM SET #1. Galactic Structure 37 pts total. due Tuesday, 2/19/2019 PROBLEM SET #1 Galactic Structure 37 pts total due Tuesday, 2/19/2019 1. Stellar cluster problem [26 pts] The following refers to a star cluster observed on Aug 15, 2010 at about 4am UT. The cluster is

More information

Overview In chapter 16 you learned how to calculate the Electric field from continuous distributions of charge; you follow four basic steps.

Overview In chapter 16 you learned how to calculate the Electric field from continuous distributions of charge; you follow four basic steps. Materials: whiteboards, computers with VPython Objectives In this lab you will do the following: Computationally model the electric field of a uniformly charged rod Computationally model the electric field

More information

Warm up: Unit circle Fill in the exact values for quadrant 1 reference angles.

Warm up: Unit circle Fill in the exact values for quadrant 1 reference angles. Name: 4-1 Unit Circle and Exact Values Learning Goals: 1) How can we use the unit circle to find the value of sine, cosine, and tangent? 2) Given a point on a circle and the radius of the circle, how can

More information

Finite Volume Method for Scalar Advection in 2D

Finite Volume Method for Scalar Advection in 2D Chapter 9 Finite Volume Method for Scalar Advection in D 9. Introduction The purpose of this exercise is to code a program to integrate the scalar advection equation in two-dimensional flows. 9. The D

More information

Amplitude preserving AMO from true amplitude DMO and inverse DMO

Amplitude preserving AMO from true amplitude DMO and inverse DMO Stanford Exploration Project, Report 84, May 9, 001, pages 1 167 Amplitude preserving AMO from true amplitude DMO and inverse DMO Nizar Chemingui and Biondo Biondi 1 ABSTRACT Starting from the definition

More information

Foundations of Computation

Foundations of Computation The Australian National University Semester 2, 2018 Research School of Computer Science Tutorial 1 Dirk Pattinson Foundations of Computation The tutorial contains a number of exercises designed for the

More information

BASIC TECHNOLOGY Pre K starts and shuts down computer, monitor, and printer E E D D P P P P P P P P P P

BASIC TECHNOLOGY Pre K starts and shuts down computer, monitor, and printer E E D D P P P P P P P P P P BASIC TECHNOLOGY Pre K 1 2 3 4 5 6 7 8 9 10 11 12 starts and shuts down computer, monitor, and printer P P P P P P practices responsible use and care of technology devices P P P P P P opens and quits an

More information

AVO inversion in V (x, z) media

AVO inversion in V (x, z) media Stanford Exploration Project, Report 97, July 8, 998, pages 75 94 AVO inversion in V (x, z) media Yalei Sun and Wenjie Dong keywords:.5-d Kirchhoff integral, AVO inversion, fluid-line section ABSTRACT

More information

Investigating fault shadows in a normally faulted geology

Investigating fault shadows in a normally faulted geology Investigating fault shadows in a normally faulted geology Sitamai Ajiduah* and Gary Margrave CREWES, University of Calgary, sajiduah@ucalgary.ca Summary Fault shadow poses a potential development risk

More information

Residual Statics using CSP gathers

Residual Statics using CSP gathers Residual Statics using CSP gathers Xinxiang Li and John C. Bancroft ABSTRACT All the conventional methods for residual statics analysis require normal moveout (NMO) correction applied on the seismic data.

More information

The Deconvolution of Multicomponent Trace Vectors

The Deconvolution of Multicomponent Trace Vectors The Deconvolution of Multicomponent Trace Vectors Xinxiang Li, Peter Cary and Rodney Couzens Sensor Geophysical Ltd., Calgary, Canada xinxiang_li@sensorgeo.com Summary Deconvolution of the horizontal components

More information

PH 120 Project # 2: Pendulum and chaos

PH 120 Project # 2: Pendulum and chaos PH 120 Project # 2: Pendulum and chaos Due: Friday, January 16, 2004 In PH109, you studied a simple pendulum, which is an effectively massless rod of length l that is fixed at one end with a small mass

More information

1.4 Techniques of Integration

1.4 Techniques of Integration .4 Techniques of Integration Recall the following strategy for evaluating definite integrals, which arose from the Fundamental Theorem of Calculus (see Section.3). To calculate b a f(x) dx. Find a function

More information

Centre for Mathematical Sciences HT 2017 Mathematical Statistics. Study chapters 6.1, 6.2 and in the course book.

Centre for Mathematical Sciences HT 2017 Mathematical Statistics. Study chapters 6.1, 6.2 and in the course book. Lund University Stationary stochastic processes Centre for Mathematical Sciences HT 2017 Mathematical Statistics Computer exercise 2 in Stationary stochastic processes, HT 17. The purpose with this computer

More information

Superposition of waves (review) PHYS 258 Fourier optics SJSU Spring 2010 Eradat

Superposition of waves (review) PHYS 258 Fourier optics SJSU Spring 2010 Eradat Superposition of waves (review PHYS 58 Fourier optics SJSU Spring Eradat Superposition of waves Superposition of waves is the common conceptual basis for some optical phenomena such as: Polarization Interference

More information

( ) ( ), 1, 1. Downloaded 10/14/14 to Redistribution subject to SEG license or copyright; see Terms of Use at

( ) ( ), 1, 1. Downloaded 10/14/14 to Redistribution subject to SEG license or copyright; see Terms of Use at Chao Zhang*, Jie Zhang, University of Science and Technology of China (USTC); Zhikun Sun, GeoTomo LLC Summary Refraction traveltimes have long been applied for deriving long-wavelength statics solutions.

More information

Welcome. to Physics 2135.

Welcome. to Physics 2135. Welcome to Physics 2135. PHYSICS 2135 Engineering Physics II Dr. S. Thomas Vojta Instructor in charge Office: 204 Physics, Phone: 341-4793 vojtat@mst.edu www.mst.edu/~vojtat Office hours: Mon+ Wed 11am-12pm

More information

Structural Geology, GEOL 330 Spring 2012

Structural Geology, GEOL 330 Spring 2012 Developing the Magic Eye for folds This lab exercise is designed to get you thinking about the chronology of structural processes and and the resultant map patterns in areas with flat topography. You may

More information

Lecture 5b: Starting Matlab

Lecture 5b: Starting Matlab Lecture 5b: Starting Matlab James K. Peterson Department of Biological Sciences and Department of Mathematical Sciences Clemson University August 7, 2013 Outline 1 Resources 2 Starting Matlab 3 Homework

More information

Integration to Compute Volumes, Work. Goals: Volumes by Slicing Volumes by Cylindrical Shells Work

Integration to Compute Volumes, Work. Goals: Volumes by Slicing Volumes by Cylindrical Shells Work Week #8: Integration to Compute Volumes, Work Goals: Volumes by Slicing Volumes by Cylindrical Shells Work 1 Volumes by Slicing - 1 Volumes by Slicing In the integration problems considered in this section

More information

Physics 228. Momentum and Force Kinetic Energy Relativistic Mass and Rest Mass Photoelectric Effect Energy and Momentum of Photons

Physics 228. Momentum and Force Kinetic Energy Relativistic Mass and Rest Mass Photoelectric Effect Energy and Momentum of Photons Physics 228 Momentum and Force Kinetic Energy Relativistic Mass and Rest Mass Photoelectric Effect Energy and Momentum of Photons Lorentz Transformations vs. Rotations The Lorentz transform is similar

More information

Lab Week 6. Quiz #3 Voltage Divider Homework P11, P12 Kirchhoff's Voltage Law (KVL) Kirchhoff's Current Law (KCL) KCL + KVL Module Report tips

Lab Week 6. Quiz #3 Voltage Divider Homework P11, P12 Kirchhoff's Voltage Law (KVL) Kirchhoff's Current Law (KCL) KCL + KVL Module Report tips Lab Week 6 Quiz #3 Voltage Divider Homework P11, P12 Kirchhoff's Voltage Law (KVL) Kirchhoff's Current Law (KCL) KCL + KVL Module Report tips Quiz 3 Voltage Divider (20 pts.) Please clear desks and turn

More information

Astronomy 154 Lab 4: The Sun. NASA Image comparing the Earth with the Sun. Image from:

Astronomy 154 Lab 4: The Sun. NASA Image comparing the Earth with the Sun. Image from: Astronomy 154 Lab 3: The Sun NASA Image comparing the Earth with the Sun. Image from: http://www.universetoday.com/16338/the-sun/ The Sun at the center of our Solar System is a massive ball of Hydrogen,

More information

Laboratory handouts, ME 340

Laboratory handouts, ME 340 Laboratory handouts, ME 340 This document contains summary theory, solved exercises, prelab assignments, lab instructions, and report assignments for Lab 4. 2014-2016 Harry Dankowicz, unless otherwise

More information

Graphing Linear Equations: Warm Up: Brainstorm what you know about Graphing Lines: (Try to fill the whole page) Graphing

Graphing Linear Equations: Warm Up: Brainstorm what you know about Graphing Lines: (Try to fill the whole page) Graphing Graphing Linear Equations: Warm Up: Brainstorm what you know about Graphing Lines: (Try to fill the whole page) Graphing Notes: The three types of ways to graph a line and when to use each: Slope intercept

More information

Simple Harmonic Motion ===============================================

Simple Harmonic Motion =============================================== PHYS 1105 Last edit: May 25, 2017 SMU Physics Dept. Simple Harmonic Motion =============================================== Goal To determine the spring constant k and effective mass m eff of a real spring.

More information

Lab 11. Spring-Mass Oscillations

Lab 11. Spring-Mass Oscillations Lab 11. Spring-Mass Oscillations Goals To determine experimentally whether the supplied spring obeys Hooke s law, and if so, to calculate its spring constant. To find a solution to the differential equation

More information

Mathematics 111 (Calculus II) Laboratory Manual

Mathematics 111 (Calculus II) Laboratory Manual Mathematics (Calculus II) Laboratory Manual Department of Mathematics & Statistics University of Regina nd edition prepared by Patrick Maidorn, Fotini Labropulu, and Robert Petry University of Regina Department

More information

Seismic Imaging. William W. Symes. C. I. M. E. Martina Franca September

Seismic Imaging. William W. Symes. C. I. M. E. Martina Franca September Seismic Imaging William W. Symes C. I. M. E. Martina Franca September 2002 www.trip.caam.rice.edu 1 0 offset (km) -4-3 -2-1 1 2 time (s) 3 4 5 How do you turn lots of this... (field seismogram from the

More information

Petrel TIPS&TRICKS from SCM

Petrel TIPS&TRICKS from SCM Petrel TIPS&TRICKS from SCM Knowledge Worth Sharing Fault Model Quality Control Most Petrel projects are faulted. This means that fault models must be built and then checked for accuracy in almost every

More information

Lab I. 2D Motion. 1 Introduction. 2 Theory. 2.1 scalars and vectors LAB I. 2D MOTION 15

Lab I. 2D Motion. 1 Introduction. 2 Theory. 2.1 scalars and vectors LAB I. 2D MOTION 15 LAB I. 2D MOTION 15 Lab I 2D Motion 1 Introduction In this lab we will examine simple two-dimensional motion without acceleration. Motion in two dimensions can often be broken up into two separate one-dimensional

More information

Physics 121H Fall Homework #15 23-November-2015 Due Date : 2-December-2015

Physics 121H Fall Homework #15 23-November-2015 Due Date : 2-December-2015 Reading : Chapters 16 and 17 Note: Reminder: Physics 121H Fall 2015 Homework #15 23-November-2015 Due Date : 2-December-2015 This is a two-week homework assignment that will be worth 2 homework grades

More information