PHYS 352. On Measurement, Systematic and Statistical Errors. Errors in Measurement

Size: px
Start display at page:

Download "PHYS 352. On Measurement, Systematic and Statistical Errors. Errors in Measurement"

Transcription

1 PHYS 352 On Measurement, Systematic and Statistical Errors Errors in Measurement when you make a measurement you should quote an estimate of the uncertainty or error all measurements have systematic errors some measurements have statistical errors e.g. measurement of the total solar neutrino flux by the Sudbury Neutrino Observatory [4.94 ± 0.21 (stat.) ± 0.36 (syst.)] 10 6 cm 2 s 1 1

2 Statistical Errors physicists consider them as the easy one to deal with statistical errors arise whenever a probability is involved radioactive decay when a sample of an ensemble is measured if the measurement is at the quantum level example: measuring very low levels of illumination the light source being measured is so weak that only single photons are arriving at the light detector (e.g. a photomultiplier tube) not all photons from the light source are detected i.e. there is some probability that any given photon makes it to the light detector and is subsequently detected the size of the electrical signal from the light detector (integrated over a fixed time interval) is a measure of the light source intensity and this measure has statistical error in some time intervals a few more photons are detected and some time intervals less the mean value and the statistical spread of the number of detected photons are precisely understood by physicists statistics determine the uncertainty in the measurement easy! Systematic Error from Sayer: Systematic error. This is the degree to which a measured value differs from the 'true' value because of errors inherent in the measurement. This may be due to an incorrect scale, a wrong calibration or an erroneous assumption. In instrumentation, changes in the original calibration of an instrument over time, or if the instrument is used under abnormal conditions are major sources of systematic error. Systematic errors are generally not statistical in nature and sometimes may be corrected by measurement of a standard. physicists often deal with systematic errors as though they are statistical because there isn t a better alternative meaning that we combine systematic errors in quadrature as though they were statistically independent; but much of the time they are not 2

3 How to Think About Systematics? how could my measurement be wrong? leads to: how could my measurement system be wrong? leads to: how could my transducer give a wrong value leads to: examining transducer characteristics four classes of transducer characteristics lead to four important classes of systematics accuracy/calibration repeatability linearity noise or backgrounds Calibration Systematics absolute calibration is wrong water was at 99 C when the thermometer tick for 100 C was marked calibration drifts with time transducer (and its associated electronics) are turned on and it outputs accurate readings; then, it starts to warm up (electrical heating) and its output changes with its internal temperature example: how to estimate calibration accuracy systematic? apply a reference standard as input and measure the transducer output value boil water (controlled) and temperature probe measures this as C make desired temperature measurements repeat measurement of reference standard boil water again, and temperature probe outputs 99.7 C the calibration correction factor is either 1/1.015 or 1/0.997; make the correction, split the difference, and use the difference as error you have bounded the calibration stability and accuracy between the times the reference was checked, one postulates the accuracy lies within the observed range 3

4 Linearity Systematic linearity curve (output y(x) versus input x) is not what you think; this is a possible systematic e.g. your assumption is perfect linearity whereas the transducer has small nonlinearity at the end of its range example how to estimate linearity systematic make multiple measurements of y versus x fit a straight line to y(x): get slope m±δm and intercept b±δb the uncertainties in the parameters for the linearity curve help estimate the systematic error due to non-linearity thus, for any measurement y (corresponding ideally to a single input x), there is a range of values for x that is consistent with the fitted linearity curve parameters millivolts thermocouple output Example: Repeated Measurement say you are making a measurement of some quantity, call it X you make a single measurement of that quantity and estimate the sources of error X ± ΔX you then take repeated measurements of the same quantity and find the scatter distribution of the measured X values is smaller than ΔX from a single measurement? perhaps you have overestimated the uncertainty? is the same as ΔX from a single measurement? perhaps you did a good job with your error estimate? is greater than ΔX from the single measurement? you could increase your original error estimate to account for the poor repeatability to do this, you could calculate the standard deviation of the mean (for example) and use that as the uncertainty; optionally a weighted average of multiple measurements and their errors determines the ensemble s error summary: unaccounted for systematics may lead to expanded uncertainties or use if different measurements have different uncertainties 4

5 Plot: Repeated Measurements Caution: Uncertainty from Scatter this is what we do as experimental physicists and it s correct (acceptable) to do this but we need to be aware of the perils we are applying statistical analysis to systematics something is causing the measured points to scatter something is causing the poor repeatability of the transducer that something could be an undiscovered effect or, that something could be easily corrected if you find a systematic effect, and you find out how to correct it, it is no longer a systematic error 5

6 What s the Point? this course is Measurement, Instrumentation and Experiment Design understanding the underlying concepts behind statistical and systematic errors is crucial and it comes from understanding the instrumentation (and measurement system) what you want to know: show me how to estimate systematic errors; what procedure do I follow? my answer: there is no fixed procedure for assigning systematic errors that s applicable in the realm of all possible measurements and I can t describe a procedure for you to follow that s correct every time; but I can tell you that the most important thing is to understand and think about the basics measurement is the reality; it is not always correct but there is always a reason why an instrument (transducer) is producing the measurement (accurate or offset) that it is the more you know about transducers, the better you will be at estimating the systematic errors they produce 6

Chapter 8. Linear Regression. Copyright 2010 Pearson Education, Inc.

Chapter 8. Linear Regression. Copyright 2010 Pearson Education, Inc. Chapter 8 Linear Regression Copyright 2010 Pearson Education, Inc. Fat Versus Protein: An Example The following is a scatterplot of total fat versus protein for 30 items on the Burger King menu: Copyright

More information

Chapter 8. Linear Regression. The Linear Model. Fat Versus Protein: An Example. The Linear Model (cont.) Residuals

Chapter 8. Linear Regression. The Linear Model. Fat Versus Protein: An Example. The Linear Model (cont.) Residuals Chapter 8 Linear Regression Copyright 2007 Pearson Education, Inc. Publishing as Pearson Addison-Wesley Slide 8-1 Copyright 2007 Pearson Education, Inc. Publishing as Pearson Addison-Wesley Fat Versus

More information

Graphing. y m = cx n (3) where c is constant. What was true about Equation 2 is applicable here; the ratio. y m x n. = c

Graphing. y m = cx n (3) where c is constant. What was true about Equation 2 is applicable here; the ratio. y m x n. = c Graphing Theory At its most basic, physics is nothing more than the mathematical relationships that have been found to exist between different physical quantities. It is important that you be able to identify

More information

FUNDAMENTAL CONCEPTS IN MEASUREMENT & EXPERIMENTATION (continued) Measurement Errors and Uncertainty:

FUNDAMENTAL CONCEPTS IN MEASUREMENT & EXPERIMENTATION (continued) Measurement Errors and Uncertainty: FUNDAMENTAL CNCEPTS N MEASUREMENT & EXPERMENTATN (continued) Measurement Errors and Uncertainty: The Error in a measurement is the difference between the Measured Value and the True Value of the Measurand.

More information

37-6 Watching the electrons (matter waves)

37-6 Watching the electrons (matter waves) 37-6 Watching the electrons (matter waves) 1 testing our proposition: the electrons go either through hole 1 or hole 2 add a very strong light source behind walls between two holes, electrons will scatter

More information

1 Some Statistical Basics.

1 Some Statistical Basics. Q Some Statistical Basics. Statistics treats random errors. (There are also systematic errors e.g., if your watch is 5 minutes fast, you will always get the wrong time, but it won t be random.) The two

More information

Linear Regression. Linear Regression. Linear Regression. Did You Mean Association Or Correlation?

Linear Regression. Linear Regression. Linear Regression. Did You Mean Association Or Correlation? Did You Mean Association Or Correlation? AP Statistics Chapter 8 Be careful not to use the word correlation when you really mean association. Often times people will incorrectly use the word correlation

More information

Measurements and Data Analysis

Measurements and Data Analysis Measurements and Data Analysis 1 Introduction The central point in experimental physical science is the measurement of physical quantities. Experience has shown that all measurements, no matter how carefully

More information

Uncertainty, Error, and Precision in Quantitative Measurements an Introduction 4.4 cm Experimental error

Uncertainty, Error, and Precision in Quantitative Measurements an Introduction 4.4 cm Experimental error Uncertainty, Error, and Precision in Quantitative Measurements an Introduction Much of the work in any chemistry laboratory involves the measurement of numerical quantities. A quantitative measurement

More information

Error analysis for IPhO contestants

Error analysis for IPhO contestants Error analysis for IPhO contestants Heikki Mäntysaari University of Jyväskylä, Department of Physics Abstract In the experimental part of IPhO (and generally when performing measurements) you have to estimate

More information

Some Statistics. V. Lindberg. May 16, 2007

Some Statistics. V. Lindberg. May 16, 2007 Some Statistics V. Lindberg May 16, 2007 1 Go here for full details An excellent reference written by physicists with sample programs available is Data Reduction and Error Analysis for the Physical Sciences,

More information

appstats8.notebook October 11, 2016

appstats8.notebook October 11, 2016 Chapter 8 Linear Regression Objective: Students will construct and analyze a linear model for a given set of data. Fat Versus Protein: An Example pg 168 The following is a scatterplot of total fat versus

More information

Modern Methods of Data Analysis - WS 07/08

Modern Methods of Data Analysis - WS 07/08 Modern Methods of Data Analysis Lecture VIa (19.11.07) Contents: Uncertainties (II): Re: error propagation Correlated uncertainties Systematic uncertainties Re: Error Propagation (I) x = Vi,j and µi known

More information

The Physics of Neutrinos

The Physics of Neutrinos AAAS Feb. 15, 2004 The Physics of Neutrinos Boris Kayser Neutrinos are Abundant We, and all the everyday objects around us here on earth, are made of electrons, protons, and neutrons. In the universe,

More information

Neutrino Oscillations

Neutrino Oscillations Neutrino Oscillations Supervisor: Kai Schweda 5/18/2009 Johannes Stiller 1 Outline The Standard (Solar) Model Detecting Neutrinos The Solar Neutrino Problem Neutrino Oscillations Neutrino Interactions

More information

APPENDIX 1 BASIC STATISTICS. Summarizing Data

APPENDIX 1 BASIC STATISTICS. Summarizing Data 1 APPENDIX 1 Figure A1.1: Normal Distribution BASIC STATISTICS The problem that we face in financial analysis today is not having too little information but too much. Making sense of large and often contradictory

More information

that relative errors are dimensionless. When reporting relative errors it is usual to multiply the fractional error by 100 and report it as a percenta

that relative errors are dimensionless. When reporting relative errors it is usual to multiply the fractional error by 100 and report it as a percenta Error Analysis and Significant Figures Errors using inadequate data are much less than those using no data at all. C. Babbage No measurement of a physical quantity can be entirely accurate. It is important

More information

Solar Interior. Sources of energy for Sun Nuclear fusion Solar neutrino problem Helioseismology

Solar Interior. Sources of energy for Sun Nuclear fusion Solar neutrino problem Helioseismology Solar Interior Sources of energy for Sun Nuclear fusion Solar neutrino problem Helioseismology Solar Atmosphere Solar interior Solar facts Luminosity: 3.8x10 26 J/s Mass: 2.0x10 30 kg Composition: 73%

More information

Measuring the Top Quark Mass using Kinematic Endpoints

Measuring the Top Quark Mass using Kinematic Endpoints Journal of Physics: Conference Series OPEN ACCESS Measuring the Top Quark Mass using Kinematic Endpoints To cite this article: Benjamin Nachman and the Cms Collaboration 13 J. Phys.: Conf. Ser. 45 156

More information

Take the measurement of a person's height as an example. Assuming that her height has been determined to be 5' 8", how accurate is our result?

Take the measurement of a person's height as an example. Assuming that her height has been determined to be 5' 8, how accurate is our result? Error Analysis Introduction The knowledge we have of the physical world is obtained by doing experiments and making measurements. It is important to understand how to express such data and how to analyze

More information

WHY DO SOLAR NEUTRINO EXPERIMENTS BELOW 1 MEV? a

WHY DO SOLAR NEUTRINO EXPERIMENTS BELOW 1 MEV? a WHY DO SOLAR NEUTRINO EXPERIMENTS BELOW 1 MEV? a J. N. BAHCALL Institute for Advanced Study, Princeton, NJ 08540, USA E-mail: jnb@sns.ias.edu I discuss why we need solar neutrino experiments below 1 MeV.

More information

1. Create a scatterplot of this data. 2. Find the correlation coefficient.

1. Create a scatterplot of this data. 2. Find the correlation coefficient. How Fast Foods Compare Company Entree Total Calories Fat (grams) McDonald s Big Mac 540 29 Filet o Fish 380 18 Burger King Whopper 670 40 Big Fish Sandwich 640 32 Wendy s Single Burger 470 21 1. Create

More information

BRIDGE CIRCUITS EXPERIMENT 5: DC AND AC BRIDGE CIRCUITS 10/2/13

BRIDGE CIRCUITS EXPERIMENT 5: DC AND AC BRIDGE CIRCUITS 10/2/13 EXPERIMENT 5: DC AND AC BRIDGE CIRCUITS 0//3 This experiment demonstrates the use of the Wheatstone Bridge for precise resistance measurements and the use of error propagation to determine the uncertainty

More information

Experimental Uncertainty (Error) and Data Analysis

Experimental Uncertainty (Error) and Data Analysis Experimental Uncertainty (Error) and Data Analysis Advance Study Assignment Please contact Dr. Reuven at yreuven@mhrd.org if you have any questions Read the Theory part of the experiment (pages 2-14) and

More information

AE2160 Introduction to Experimental Methods in Aerospace

AE2160 Introduction to Experimental Methods in Aerospace AE160 Introduction to Experimental Methods in Aerospace Uncertainty Analysis C.V. Di Leo (Adapted from slides by J.M. Seitzman, J.J. Rimoli) 1 Accuracy and Precision Accuracy is defined as the difference

More information

Basic Business Statistics 6 th Edition

Basic Business Statistics 6 th Edition Basic Business Statistics 6 th Edition Chapter 12 Simple Linear Regression Learning Objectives In this chapter, you learn: How to use regression analysis to predict the value of a dependent variable based

More information

Measurement and Uncertainty

Measurement and Uncertainty Measurement and Uncertainty Michael Gold Physics 307L September 16, 2006 Michael Gold (Physics 307L) Measurement and Uncertainty September 16, 2006 1 / 9 Goal of Experiment Measure a parameter: statistical

More information

4/3/2019. Advanced Measurement Systems and Sensors. Dr. Ibrahim Al-Naimi. Chapter one. Introduction to Measurement Systems

4/3/2019. Advanced Measurement Systems and Sensors. Dr. Ibrahim Al-Naimi. Chapter one. Introduction to Measurement Systems Advanced Measurement Systems and Sensors Dr. Ibrahim Al-Naimi Chapter one Introduction to Measurement Systems 1 Outlines Control and measurement systems Transducer/sensor definition and classifications

More information

Inferences for Regression

Inferences for Regression Inferences for Regression An Example: Body Fat and Waist Size Looking at the relationship between % body fat and waist size (in inches). Here is a scatterplot of our data set: Remembering Regression In

More information

Measurement: The Basics

Measurement: The Basics I. Introduction Measurement: The Basics Physics is first and foremost an experimental science, meaning that its accumulated body of knowledge is due to the meticulous experiments performed by teams of

More information

Experimental Uncertainty (Error) and Data Analysis

Experimental Uncertainty (Error) and Data Analysis E X P E R I M E N T 1 Experimental Uncertainty (Error) and Data Analysis INTRODUCTION AND OBJECTIVES Laboratory investigations involve taking measurements of physical quantities, and the process of taking

More information

COUNTING ERRORS AND STATISTICS RCT STUDY GUIDE Identify the five general types of radiation measurement errors.

COUNTING ERRORS AND STATISTICS RCT STUDY GUIDE Identify the five general types of radiation measurement errors. LEARNING OBJECTIVES: 2.03.01 Identify the five general types of radiation measurement errors. 2.03.02 Describe the effect of each source of error on radiation measurements. 2.03.03 State the two purposes

More information

Solar spectrum. Nuclear burning in the sun produce Heat, Luminosity and Neutrinos. pp neutrinos < 0.4 MeV

Solar spectrum. Nuclear burning in the sun produce Heat, Luminosity and Neutrinos. pp neutrinos < 0.4 MeV SOLAR NEUTRINOS Solar spectrum Nuclear burning in the sun produce Heat, Luminosity and Neutrinos pp neutrinos < 0.4 MeV Beryllium neutrinos 0.86 MeV Monochromatic since 2 body decay 2 kev width due to

More information

Oklahoma State University. Solar Neutrinos and their Detection Techniques. S.A.Saad. Department of Physics

Oklahoma State University. Solar Neutrinos and their Detection Techniques. S.A.Saad. Department of Physics Oklahoma State University Solar Neutrinos and their Detection Techniques S.A.Saad Department of Physics Topics to be covered Solar Neutrinos Solar Neutrino Detection Techniques Solar Neutrino Puzzle and

More information

II. Frequentist probabilities

II. Frequentist probabilities II. Frequentist probabilities II.4 Statistical interpretation or calibration 1 II.4.1 What is statistical interpretation doing? 2 In light of a (non-perfect) forecast performance corrections are applied

More information

Intermediate Lab PHYS 3870

Intermediate Lab PHYS 3870 Intermediate Lab PHYS 3870 Lecture 2 Defining Errors References: Taylor Ch. 1, 2, 3 Introduction Section 0 Lecture 1 Slide 1 Also refer to [HANDOUT] Baird Problems (Ch 5-See web site) Glossary of Important

More information

arxiv: v1 [physics.ins-det] 27 Jun 2017

arxiv: v1 [physics.ins-det] 27 Jun 2017 Double Calorimetry System in JUNO Miao He on behalf of the JUNO collaboration arxiv:1706.08761v1 [physics.ins-det] 27 Jun 2017 Institute of High Energy Physics, Beijing hem@ihep.ac.cn Abstract. The Jiangmen

More information

Observation of flavor swap process in supernova II neutrino spectra

Observation of flavor swap process in supernova II neutrino spectra Observation of flavor swap process in supernova II neutrino spectra David B. Cline and George Fuller Abstract. We review the concept of quantum flavor swap in a SNII explosion. There will be a specific

More information

Intermediate Lab PHYS 3870

Intermediate Lab PHYS 3870 Intermediate Lab PHYS 3870 Lecture 4 Comparing Data and Models Quantitatively Linear Regression Introduction Section 0 Lecture 1 Slide 1 References: Taylor Ch. 8 and 9 Also refer to Glossary of Important

More information

Chapter 10 Regression Analysis

Chapter 10 Regression Analysis Chapter 10 Regression Analysis Goal: To become familiar with how to use Excel 2007/2010 for Correlation and Regression. Instructions: You will be using CORREL, FORECAST and Regression. CORREL and FORECAST

More information

Revision Guide for Chapter 8

Revision Guide for Chapter 8 Revision Guide for Chapter 8 Contents Revision Checklist Revision Notes Scalar quantity...4 Vectors...4 Vector components...5 Displacement...5 Velocity and speed...6 Vector addition...7 Distance time graph...7

More information

Beta Spectrum. T β,max = kev kev 2.5 ms. Eγ = kev

Beta Spectrum. T β,max = kev kev 2.5 ms. Eγ = kev HOM, 1/14/05; DVB 014-Jan-9, 01-Dec-17, 013-Oct-16 Beta Spectrum Goal: to investigate the spectrum of β rays emitted by a 137 Cs source. The instrument used is a so-called 180 o magnetic spectrometer that

More information

Counting Photons to Calibrate a Photometer for Stellar Intensity Interferometry

Counting Photons to Calibrate a Photometer for Stellar Intensity Interferometry Counting Photons to Calibrate a Photometer for Stellar Intensity Interferometry A Senior Project Presented to the Department of Physics California Polytechnic State University, San Luis Obispo In Partial

More information

The 64th Compton Lecture Series Unsolved Mysteries of the Universe: Looking for Clues in Surprising Places

The 64th Compton Lecture Series Unsolved Mysteries of the Universe: Looking for Clues in Surprising Places The 64th Compton Lecture Series Unsolved Mysteries of the Universe: Looking for Clues in Surprising Places Brian Odom Fall 2006 http://kicp.uchicago.edu/~odom/compton.htm Lecture 2: From the Big Bang to

More information

Neutrino Experiments: Lecture 2 M. Shaevitz Columbia University

Neutrino Experiments: Lecture 2 M. Shaevitz Columbia University Neutrino Experiments: Lecture 2 M. Shaevitz Columbia University 1 Outline 2 Lecture 1: Experimental Neutrino Physics Neutrino Physics and Interactions Neutrino Mass Experiments Neutrino Sources/Beams and

More information

Principles and Problems. Chapter 1: A Physics Toolkit

Principles and Problems. Chapter 1: A Physics Toolkit PHYSICS Principles and Problems Chapter 1: A Physics Toolkit CHAPTER 1 A Physics Toolkit BIG IDEA Physicists use scientific methods to investigate energy and matter. CHAPTER 1 Table Of Contents Section

More information

THE COMPTON EFFECT Last Revised: January 5, 2007

THE COMPTON EFFECT Last Revised: January 5, 2007 B2-1 THE COMPTON EFFECT Last Revised: January 5, 2007 QUESTION TO BE INVESTIGATED: How does the energy of a scattered photon change after an interaction with an electron? INTRODUCTION: When a photon is

More information

Physics: Uncertainties - Student Material (AH) 1

Physics: Uncertainties - Student Material (AH) 1 UNCERTAINTIES Summary of the Basic Theory associated with Uncertainty It is important to realise that whenever a physical quantity is being measured there will always be a degree of inaccuracy associated

More information

appstats27.notebook April 06, 2017

appstats27.notebook April 06, 2017 Chapter 27 Objective Students will conduct inference on regression and analyze data to write a conclusion. Inferences for Regression An Example: Body Fat and Waist Size pg 634 Our chapter example revolves

More information

Lecture 2 - Length Contraction

Lecture 2 - Length Contraction Lecture 2 - Length Contraction A Puzzle We are all aware that if you jump to the right, your reflection in the mirror will jump left. But if you raise your hand up, your reflection will also raise its

More information

Computer simulation of radioactive decay

Computer simulation of radioactive decay Computer simulation of radioactive decay y now you should have worked your way through the introduction to Maple, as well as the introduction to data analysis using Excel Now we will explore radioactive

More information

Stat 101 L: Laboratory 5

Stat 101 L: Laboratory 5 Stat 101 L: Laboratory 5 The first activity revisits the labeling of Fun Size bags of M&Ms by looking distributions of Total Weight of Fun Size bags and regular size bags (which have a label weight) of

More information

PHYS 352 Assignment #1 Solutions

PHYS 352 Assignment #1 Solutions PHYS 352 Assignment #1 Solutions 1. Steinhart-Hart Equation for a thermistor In[1]:= a : 0.00128 In[2]:= b : 0.000236 In[3]:= In[4]:= d : 9.27 10^ 8 t r_ : a b Log r d Log r ^3 ^ 1 Note: Mathematica Log

More information

P3TMA Experimental Projects

P3TMA Experimental Projects P3TMA Experimental Projects 3 credits Take place @ S1 (from end of September to December); Enters in the average of the second semester. Projects currently available : Stern-Gerlach Experiment Quantum

More information

Chapter 38 Quantum Mechanics

Chapter 38 Quantum Mechanics Chapter 38 Quantum Mechanics Units of Chapter 38 38-1 Quantum Mechanics A New Theory 37-2 The Wave Function and Its Interpretation; the Double-Slit Experiment 38-3 The Heisenberg Uncertainty Principle

More information

LECTURE 15: SIMPLE LINEAR REGRESSION I

LECTURE 15: SIMPLE LINEAR REGRESSION I David Youngberg BSAD 20 Montgomery College LECTURE 5: SIMPLE LINEAR REGRESSION I I. From Correlation to Regression a. Recall last class when we discussed two basic types of correlation (positive and negative).

More information

One of elements driving cosmological evolution is the presence of radiation (photons) Early universe

One of elements driving cosmological evolution is the presence of radiation (photons) Early universe The Frontier Matter and Antimatter One of elements driving cosmological evolution is the presence of radiation (photons) Early universe Matter and antimatter But we live in universe full of matter -- where

More information

Chapter 27 Summary Inferences for Regression

Chapter 27 Summary Inferences for Regression Chapter 7 Summary Inferences for Regression What have we learned? We have now applied inference to regression models. Like in all inference situations, there are conditions that we must check. We can test

More information

DELAYED COINCIDENCE METHOD FOR PICOSECOND LIFETIME MEASUREMENTS

DELAYED COINCIDENCE METHOD FOR PICOSECOND LIFETIME MEASUREMENTS 306 DELAYED COINCIDENCE METHOD FOR PICOSECOND LIFETIME MEASUREMENTS ZHANG WEIJIE China Institute of Atomic Energy E-mail: zhangreatest@163.com The advanced time delay (ATD) technique, based by delayed

More information

1 Measurement Uncertainties

1 Measurement Uncertainties 1 Measurement Uncertainties (Adapted stolen, really from work by Amin Jaziri) 1.1 Introduction No measurement can be perfectly certain. No measuring device is infinitely sensitive or infinitely precise.

More information

Neutrinos: What we ve learned and what we still want to find out. Jessica Clayton Astronomy Club November 10, 2008

Neutrinos: What we ve learned and what we still want to find out. Jessica Clayton Astronomy Club November 10, 2008 Neutrinos: What we ve learned and what we still want to find out Jessica Clayton Astronomy Club November 10, 2008 Neutrinos, they are very small, they have no charge and have no mass, and do not interact

More information

Chapter 32 Lecture Notes

Chapter 32 Lecture Notes Chapter 32 Lecture Notes Physics 2424 - Strauss Formulas: mc 2 hc/2πd 1. INTRODUCTION What are the most fundamental particles and what are the most fundamental forces that make up the universe? For a brick

More information

John Ellison University of California, Riverside. Quarknet 2008 at UCR

John Ellison University of California, Riverside. Quarknet 2008 at UCR Cosmic Rays John Ellison University of California, Riverside Quarknet 2008 at UCR 1 What are Cosmic Rays? Particles accelerated in astrophysical sources incident on Earth s atmosphere Possible sources

More information

Looking at data: relationships

Looking at data: relationships Looking at data: relationships Least-squares regression IPS chapter 2.3 2006 W. H. Freeman and Company Objectives (IPS chapter 2.3) Least-squares regression p p The regression line Making predictions:

More information

EXPERIMENTAL UNCERTAINTY

EXPERIMENTAL UNCERTAINTY 3 EXPERIMENTAL UNCERTAINTY I am no matchmaker, as you well know, said Lady Russell, being much too aware of the uncertainty of all human events and calculations. --- Persuasion 3.1 UNCERTAINTY AS A 95%

More information

a) Do you see a pattern in the scatter plot, or does it look like the data points are

a) Do you see a pattern in the scatter plot, or does it look like the data points are Aim #93: How do we distinguish between scatter plots that model a linear versus a nonlinear equation and how do we write the linear regression equation for a set of data using our calculator? Homework:

More information

Lecture 32. Lidar Error and Sensitivity Analysis

Lecture 32. Lidar Error and Sensitivity Analysis Lecture 3. Lidar Error and Sensitivity Analysis Introduction Accuracy in lidar measurements Precision in lidar measurements Error analysis for Na Doppler lidar Sensitivity analysis Summary 1 Errors vs.

More information

Introduction to Uncertainty and Treatment of Data

Introduction to Uncertainty and Treatment of Data Introduction to Uncertainty and Treatment of Data Introduction The purpose of this experiment is to familiarize the student with some of the instruments used in making measurements in the physics laboratory,

More information

My data doesn t look like that..

My data doesn t look like that.. Testing assumptions My data doesn t look like that.. We have made a big deal about testing model assumptions each week. Bill Pine Testing assumptions Testing assumptions We have made a big deal about testing

More information

Uncertainty, Measurement, and Models. Lecture 2 Physics 2CL Summer Session 2011

Uncertainty, Measurement, and Models. Lecture 2 Physics 2CL Summer Session 2011 Uncertainty, Measurement, and Models Lecture 2 Physics 2CL Summer Session 2011 Outline What is uncertainty (error) analysis and what can it do for you Issues with measurement and observation What does

More information

Chapter 12 - Part I: Correlation Analysis

Chapter 12 - Part I: Correlation Analysis ST coursework due Friday, April - Chapter - Part I: Correlation Analysis Textbook Assignment Page - # Page - #, Page - # Lab Assignment # (available on ST webpage) GOALS When you have completed this lecture,

More information

Physics 509: Propagating Systematic Uncertainties. Scott Oser Lecture #12

Physics 509: Propagating Systematic Uncertainties. Scott Oser Lecture #12 Physics 509: Propagating Systematic Uncertainties Scott Oser Lecture #1 1 Additive offset model Suppose we take N measurements from a distribution, and wish to estimate the true mean of the underlying

More information

MECHANICAL ENGINEERING SYSTEMS LABORATORY

MECHANICAL ENGINEERING SYSTEMS LABORATORY MECHANICAL ENGINEERING SYSTEMS LABORATORY Group 02 Asst. Prof. Dr. E. İlhan KONUKSEVEN FUNDAMENTAL CONCEPTS IN MEASUREMENT AND EXPERIMENTATION MEASUREMENT ERRORS AND UNCERTAINTY THE ERROR IN A MEASUREMENT

More information

Solar Neutrinos and the 2015 Nobel Prize

Solar Neutrinos and the 2015 Nobel Prize Solar Neutrinos and the 2015 Nobel Prize UBC/TRIUMF Saturday Morning Lecture Series November 2016 Outline 1. What's a neutrino? 2. How do you detect neutrinos? 3. The solar neutrino problem 4. Neutrino

More information

Control Engineering BDA30703

Control Engineering BDA30703 Control Engineering BDA30703 Lecture 3: Performance characteristics of an instrument Prepared by: Ramhuzaini bin Abd. Rahman Expected Outcomes At the end of this lecture, students should be able to; 1)

More information

Photoelectric effect

Photoelectric effect Laboratory#3 Phys4480/5480 Dr. Cristian Bahrim Photoelectric effect In 1900, Planck postulated that light is emitted and absorbed in discrete but tiny bundles of energy, E = hν, called today photons. Here

More information

Heat & Temperature. What are heat & temperature and how do they relate?

Heat & Temperature. What are heat & temperature and how do they relate? Heat & Temperature What are heat & temperature and how do they relate? SPS7. Students will relate transformations and flow of energy within a system. a. Identify energy transformations within a system

More information

arxiv: v1 [physics.ins-det] 3 Feb 2011

arxiv: v1 [physics.ins-det] 3 Feb 2011 Nuclear Instruments and Methods in Physics Research A 00 (2018) 1 5 Alogo.pdf Nuclear Instruments and Methods in Physics Research A Scintillation decay time and pulse shape discrimination in oxygenated

More information

MULTIPLE REGRESSION METHODS

MULTIPLE REGRESSION METHODS DEPARTMENT OF POLITICAL SCIENCE AND INTERNATIONAL RELATIONS Posc/Uapp 816 MULTIPLE REGRESSION METHODS I. AGENDA: A. Residuals B. Transformations 1. A useful procedure for making transformations C. Reading:

More information

Graphical Analysis and Errors MBL

Graphical Analysis and Errors MBL Graphical Analysis and Errors MBL I Graphical Analysis Graphs are vital tools for analyzing and displaying data Graphs allow us to explore the relationship between two quantities -- an independent variable

More information

Monte Carlo Simulations for Future Geoneutrino Detectors

Monte Carlo Simulations for Future Geoneutrino Detectors Monte Carlo Simulations for Future Geoneutrino Detectors Morgan Askins Abstract The main contribution of heat in the earth s mantle is thought to be the radioactive decays of 238 U, 232 T h, and 40 K.

More information

PHYSICS LAB: CONSTANT MOTION

PHYSICS LAB: CONSTANT MOTION PHYSICS LAB: CONSTANT MOTION Introduction Experimentation is fundamental to physics (and all science, for that matter) because it allows us to prove or disprove our hypotheses about how the physical world

More information

Solar Neutrino Oscillations

Solar Neutrino Oscillations Solar Neutrino Oscillations ( m 2, θ 12 ) Background (aka where we were): Radiochemical experiments Kamiokande and Super-K Where we are: Recent results SNO and KamLAND Global picture Where we are going:

More information

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) In the equation E = hf, the f stands for 1) A) the smaller wavelengths of visible light. B) wave

More information

Notes Errors and Noise PHYS 3600, Northeastern University, Don Heiman, 6/9/ Accuracy versus Precision. 2. Errors

Notes Errors and Noise PHYS 3600, Northeastern University, Don Heiman, 6/9/ Accuracy versus Precision. 2. Errors Notes Errors and Noise PHYS 3600, Northeastern University, Don Heiman, 6/9/2011 1. Accuracy versus Precision 1.1 Precision how exact is a measurement, or how fine is the scale (# of significant figures).

More information

Chapter 10: Special Relativity

Chapter 10: Special Relativity Chapter 10: Special Relativity Einstein s revolutionary demolition of the classical notions of absolute space and time and motion, as well as a radically new insight into mass & energy. Common sense consists

More information

Absorption and Backscattering ofβrays

Absorption and Backscattering ofβrays Experiment #54 Absorption and Backscattering ofβrays References 1. B. Brown, Experimental Nucleonics 2. I. Kaplan, Nuclear Physics 3. E. Segre, Experimental Nuclear Physics 4. R.D. Evans, The Atomic Nucleus

More information

A Quick Introduction to Data Analysis (for Physics)

A Quick Introduction to Data Analysis (for Physics) A Quick Introduction to Data Analysis for Physics Dr. Jeff A. Winger What is data analysis? Data analysis is the process by which experimental data is used to obtain a valid and quantifiable result. Part

More information

Seeing and Believing: Detection, Measurement, and Inference in Experimental Physics

Seeing and Believing: Detection, Measurement, and Inference in Experimental Physics The 67th Compton Lecture Series at the University of Chicago Seeing and Believing: Detection, Measurement, and Inference in Experimental Physics Kathryn Schaffer, lecturer Notes and thoughts for Lecture

More information

Compton Scattering. Aim

Compton Scattering. Aim Compton Scattering Aim The aim of this experiment is to look at how scattering angle is related to photon energy in Compton Scattering. We will then use these results to deduce the mass of an electron.

More information

USING THE EXCEL CHART WIZARD TO CREATE CURVE FITS (DATA ANALYSIS).

USING THE EXCEL CHART WIZARD TO CREATE CURVE FITS (DATA ANALYSIS). USING THE EXCEL CHART WIZARD TO CREATE CURVE FITS (DATA ANALYSIS). Note to physics students: Even if this tutorial is not given as an assignment, you are responsible for knowing the material contained

More information

Fitting a Straight Line to Data

Fitting a Straight Line to Data Fitting a Straight Line to Data Thanks for your patience. Finally we ll take a shot at real data! The data set in question is baryonic Tully-Fisher data from http://astroweb.cwru.edu/sparc/btfr Lelli2016a.mrt,

More information

Regression and Nonlinear Axes

Regression and Nonlinear Axes Introduction to Chemical Engineering Calculations Lecture 2. What is regression analysis? A technique for modeling and analyzing the relationship between 2 or more variables. Usually, 1 variable is designated

More information

The Sun Closest star to Earth - only star that we can see details on surface - easily studied Assumption: The Sun is a typical star

The Sun Closest star to Earth - only star that we can see details on surface - easily studied Assumption: The Sun is a typical star The Sun Closest star to Earth - only star that we can see details on surface - easily studied Assumption: The Sun is a typical star Why is the Sun hot and bright? Surface Temperature of the Sun: T =

More information

Table 2.1 presents examples and explains how the proper results should be written. Table 2.1: Writing Your Results When Adding or Subtracting

Table 2.1 presents examples and explains how the proper results should be written. Table 2.1: Writing Your Results When Adding or Subtracting When you complete a laboratory investigation, it is important to make sense of your data by summarizing it, describing the distributions, and clarifying messy data. Analyzing your data will allow you to

More information

The Treatment of Numerical Experimental Results

The Treatment of Numerical Experimental Results Memorial University of Newfoundl Department of Physics Physical Oceanography The Treatment of Numerical Experimental Results The purpose of these notes is to introduce you to some techniques of error analysis

More information

Absorption and Backscattering of β-rays

Absorption and Backscattering of β-rays Experiment #54 Absorption and Backscattering of β-rays References 1. B. Brown, Experimental Nucleonics 2. I. Kaplan, Nuclear Physics 3. E. Segre, Experimental Nuclear Physics 4. R.D. Evans, The Atomic

More information

n=0 l (cos θ) (3) C l a lm 2 (4)

n=0 l (cos θ) (3) C l a lm 2 (4) Cosmic Concordance What does the power spectrum of the CMB tell us about the universe? For that matter, what is a power spectrum? In this lecture we will examine the current data and show that we now have

More information

Last Revision: August,

Last Revision: August, A3-1 HALL EFFECT Last Revision: August, 21 2007 QUESTION TO BE INVESTIGATED How to individual charge carriers behave in an external magnetic field that is perpendicular to their motion? INTRODUCTION The

More information

Reteach 2-3. Graphing Linear Functions. 22 Holt Algebra 2. Name Date Class

Reteach 2-3. Graphing Linear Functions. 22 Holt Algebra 2. Name Date Class -3 Graphing Linear Functions Use intercepts to sketch the graph of the function 3x 6y 1. The x-intercept is where the graph crosses the x-axis. To find the x-intercept, set y 0 and solve for x. 3x 6y 1

More information