Basic Physical Principles of Medical Ultrasound 9 the Time That a Wave Takes to Vibrate up and Down and Thus Is Reciprocally Related to Frequency
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Glossary Physics (I-Introduction)
1 Glossary Physics (I-introduction) - Efficiency: The percent of the work put into a machine that is converted into useful work output; = work done / energy used [-]. = eta In machines: The work output of any machine cannot exceed the work input (<=100%); in an ideal machine, where no energy is transformed into heat: work(input) = work(output), =100%. Energy: The property of a system that enables it to do work. Conservation o. E.: Energy cannot be created or destroyed; it may be transformed from one form into another, but the total amount of energy never changes. Equilibrium: The state of an object when not acted upon by a net force or net torque; an object in equilibrium may be at rest or moving at uniform velocity - not accelerating. Mechanical E.: The state of an object or system of objects for which any impressed forces cancels to zero and no acceleration occurs. Dynamic E.: Object is moving without experiencing acceleration. Static E.: Object is at rest.F Force: The influence that can cause an object to be accelerated or retarded; is always in the direction of the net force, hence a vector quantity; the four elementary forces are: Electromagnetic F.: Is an attraction or repulsion G, gravit. const.6.672E-11[Nm2/kg2] between electric charges: d, distance [m] 2 2 2 2 F = 1/(40) (q1q2/d ) [(CC/m )(Nm /C )] = [N] m,M, mass [kg] Gravitational F.: Is a mutual attraction between all masses: q, charge [As] [C] 2 2 2 2 F = GmM/d [Nm /kg kg 1/m ] = [N] 0, dielectric constant Strong F.: (nuclear force) Acts within the nuclei of atoms: 8.854E-12 [C2/Nm2] [F/m] 2 2 2 2 2 F = 1/(40) (e /d ) [(CC/m )(Nm /C )] = [N] , 3.14 [-] Weak F.: Manifests itself in special reactions among elementary e, 1.60210 E-19 [As] [C] particles, such as the reaction that occur in radioactive decay. -
M204; the Doppler Effect
MISN-0-204 THE DOPPLER EFFECT by Mary Lu Larsen THE DOPPLER EFFECT Towson State University 1. Introduction a. The E®ect . .1 b. Questions to be Answered . 1 2. The Doppler E®ect for Sound a. Wave Source and Receiver Both Stationary . 2 Source Ear b. Wave Source Approaching Stationary Receiver . .2 Stationary c. Receiver Approaching Stationary Source . 4 d. Source and Receiver Approaching Each Other . 5 e. Relative Linear Motion: Three Cases . 6 f. Moving Source Not Equivalent to Moving Receiver . 6 g. The Medium is the Preferred Reference Frame . 7 Moving Ear Away 3. The Doppler E®ect for Light a. Introduction . .7 b. Doppler Broadening of Spectral Lines . 7 c. Receding Galaxies Emit Doppler Shifted Light . 8 4. Limitations of the Results . 9 Moving Ear Toward Acknowledgments. .9 Glossary . 9 Project PHYSNET·Physics Bldg.·Michigan State University·East Lansing, MI 1 2 ID Sheet: MISN-0-204 THIS IS A DEVELOPMENTAL-STAGE PUBLICATION Title: The Doppler E®ect OF PROJECT PHYSNET Author: Mary Lu Larsen, Dept. of Physics, Towson State University The goal of our project is to assist a network of educators and scientists in Version: 4/17/2002 Evaluation: Stage 0 transferring physics from one person to another. We support manuscript processing and distribution, along with communication and information Length: 1 hr; 24 pages systems. We also work with employers to identify basic scienti¯c skills Input Skills: as well as physics topics that are needed in science and technology. A number of our publications are aimed at assisting users in acquiring such 1. -
AIUM Practice Parameter for the Performance of an Ultrasound Examination of the Abdomen And/Or Retroperitoneum
1 AIUM Practice Parameter for the Performance of an Ultrasound Examination of the Abdomen and/or Retroperitoneum Parameter developed in conjunction with the American College of Radiology (ACR), the Society for Pediatric Radiology (SPR), and the Society of Radiologists in Ultrasound (SRU). The American Institute of Ultrasound in Medicine (AIUM) is a multidisciplinary association dedicated to advancing the safe and effective use of ultrasound in medicine through professional and public education, research, development of parameters, and accreditation. To promote this mission, the AIUM is pleased to publish, in conjunction with the American College of Radiology (ACR), the Society for Pediatric Radiology (SPR), and the Society of Radiologists in Ultrasound (SRU), this AIUM Practice Parameter for the Performance of an Ultrasound Examination of the Abdomen and/or Retroperitoneum. We are indebted to the many volunteers who contributed their time, knowledge, and energy to bringing this document to completion. The AIUM represents the entire range of clinical and basic science interests in medical diagnostic ultrasound, and, with hundreds of volunteers, the AIUM has promoted the safe and effective use of ultrasound in clinical medicine for more than 65 years. This document and others like it will continue to advance this mission. © 2017 American Institute of Ultrasound in Medicine 14750 Sweitzer Ln, Suite 100 Laurel, MD 20707-5906 USA www.aium.org 2 Practice parameters of the AIUM are intended to provide the medical ultrasound community with parameters for the performance and recording of high-quality ultrasound examinations. The parameters reflect what the AIUM considers the minimum criteria for a complete examination in each area but are not intended to establish a legal standard of care. -
Training in Diagnostic Ultrasound: Essentials, Principles and Standards
This report contains the collective views of on international group of experts and does not necessarily represent the decisions or the stated policy offe World Health Organization TRAINING IN DIAGNOSTIC ULTRASOUND: ESSENTIALS, PRINCIPLES AND STANDARDS Report of a WHO Study Group Geneva 1998 WHO L~braryCataloguing In Publ~catlonData Training in diagnostic ultrasound : essentials, principles and standards : report of a WHO study group (WHO technical report series ; 875) 1 .Ultrasonography 2.Diagnostic imag~ng- standards 3.Guidelines 4.Health per- sonnel - education I Title II.Series (NLM Classification: WN 200) The World Health Organization welcomes requests for permission to reproduce or translate its publications, in part or in full Applications and enquiries should be addressed to the Office of Publications, World Health Organization, Geneva, Switzerland, which will be glad to prov~dethe latest information on any changes made to the text, plans for new editions, and reprlnts and translations already available. O World Health Organization 1998 Publications of the World Health Organization enjoy copyright protect~onin accordance with the provisions of Protocol 2 of the Universal Copyright Convention. All rights reserved. The designations employed and the presentation of the material in this publication do not imply the expression of any opnlon whatsoever on the part of the Secretariat of the World Health Organization concerning the legal status of any country, territory, city or area or of its authorities, or concerning the delimitation of its frontiers or boundaries. The mention of specific companies or of certain manufacturers' products does not imply that they are endorsed or recommended by the World Health Organ~zat~onin preference to others of a simllar nature that are not mentioned. -
Determining the Motion of Galaxies Using Doppler Redshift
Determining the Motion of Galaxies Using Doppler Redshift Caitlin M. Matyas The Arts Academy at Benjamin Rush Overview Rationale Objective Strategies Classroom Activities Annotated Bibliography / Resources Standards Appendices Overview The Doppler effect of sound is a method used to determine the relative speeds of an object emitting a sound and an observer. Depending on whether the source and/or observer are moving towards or away from each other, the frequency of the wave will change. This in turn creates a change in pitch perceived by the observer. The relative speeds can easily be calculated using the following formula: � ± �′ = �( ), � ± where f’ represents the shifted frequency, f represents the frequency of the source, v is the speed of sound, vo is the speed of the observer, and vs is the speed of the source. Vo is added if moving towards and subtracted if moving away from the source. vs is added if moving away and subtracted if moving towards the observer. The figures below help to demonstrate the perceived change in frequency. The source is located at the center of the smallest circle. The picture shows waves expanding as they move outwards away from the source, so the earliest emitted waves create the biggest circles. If both the source and observer were stationary, the waves appear to pass at equal periods of time, as seen in figure IA. However, if the source is moving, the frequency appears to change. Figure IB shows what would happen if the source moves towards the right. Although the waves are emitted at a constant frequency, they seem closer together on the right side and farther spaced on the left. -
Glossary | Speed Measuring Device Resources 191.94 KB
GLOSSARY Absorption - The transmitted R.A.D.A.R. beam will, unless otherwise acted upon (absorbed, reflected, or refracted), travel infinitely far. Under practical circumstances, the beam may be partially absorbed by natural and man-made substances. Vegetation such as trees, grass, and bushes will absorb R.A.D.A.R. energy. Freshly turned earth, such as that in a freshly plowed field, will also absorb R.A.D.A.R. Plastics of certain types and foam products will absorb R.A.D.A.R., as makers of "stealth" automotive accessories have discovered. Absorption of R.A.D.A.R. will not result in any inaccuracies in the R.A.D.A.R. readings. It will reduce the strength of the returned signal, and the operational range of the device depending upon the circumstances. Absolute speed limits - Holds that a given speed limit is in force, regardless of environment conditions, i.e., 35 mph or 50 mph. Accuracy - When used in conjunction with R.A.D.A.R. devices means the degree to which the R.A.D.A.R. device measures and displays the correct speed of a target vehicle that it is tracking. Ambient interference - The conducted and/or radiated electromagnetic interference and/or mechanical motion interference at a specific location and at a time which would be detrimental to proper R.A.D.A.R. performance. Antenna horn - The antenna horn is that portion of the R.A.D.A.R. device that shapes and directs the microwave energy (beam). The antenna horn also "catches" the returning microwave energy and directs it to the R.A.D.A.R. -
Doppler Effect
Physical Science Workshop: Astronomy Applications of Light & Color 1 Activity: Doppler Effect Background: • The Doppler effect causes a train whistle, car, or airplane to sound higher when it is moving towards you, and lower when it is moving away from you. From: http://www.physics.purdue.edu/astr263l/inlabs/doppler.html • For sound: high pitch = high frequency = short wavelength • Light is also a wave, and affected by the Doppler effect o longer wavelengths (lower frequencies) of light appear redder o The spectrum of a star moving towards you will appear blueshifted (shorter wavelengths / higher frequencies) o The spectrum of a star moving away from you will appear redshifted (longer wavelengths / lower frequencies) From: http://www.astrosociety.org/education/publications/tnl/55/astrocappella3.html Lab Materials: • computer with internet access S. Sallmen Activity: Doppler Effect Physical Science Workshop: Astronomy Applications of Light & Color 2 Activity: Doppler Basics: • Go to: http://www.fearofphysics.com/Sound/dopwhy2.html 1. Watch the waves reaching your ear if: • the source moves towards your ear at 100 meters / second • the source moves away from your ear at 100 meters / second a. In which case is the frequency of sound higher? b. In which case is the wavelength of the sound waves longest? c. If these were light waves, in which case would the light reaching your eye be redder? d. If these were light waves, in which case would the light reaching your eye be bluer? 2. Watch the waves reaching your ear if: • the source moves away from your ear at 100 meters / second • the source moves away from your ear at 200 meters / second a. -
Gravity Tests with Radio Pulsars
universe Review Gravity Tests with Radio Pulsars Norbert Wex 1,* and Michael Kramer 1,2 1 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany; [email protected] 2 Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK * Correspondence: [email protected] Received: 19 August 2020; Accepted: 17 September 2020; Published: 22 September 2020 Abstract: The discovery of the first binary pulsar in 1974 has opened up a completely new field of experimental gravity. In numerous important ways, pulsars have taken precision gravity tests quantitatively and qualitatively beyond the weak-field slow-motion regime of the Solar System. Apart from the first verification of the existence of gravitational waves, binary pulsars for the first time gave us the possibility to study the dynamics of strongly self-gravitating bodies with high precision. To date there are several radio pulsars known which can be utilized for precision tests of gravity. Depending on their orbital properties and the nature of their companion, these pulsars probe various different predictions of general relativity and its alternatives in the mildly relativistic strong-field regime. In many aspects, pulsar tests are complementary to other present and upcoming gravity experiments, like gravitational-wave observatories or the Event Horizon Telescope. This review gives an introduction to gravity tests with radio pulsars and its theoretical foundations, highlights some of the most important results, and gives a brief outlook into the future of this important field of experimental gravity. Keywords: gravity; general relativity; pulsars 1. -
Incidental Findings General Medical Ultrasound Examinations: Management and Diagnostic Pathways Guidance
w Incidental Findings General Medical Ultrasound Examinations: Management and Diagnostic Pathways Guidance September 2020 Acknowledgements The British Medical Ultrasound Society (BMUS) would like to acknowledge the work and assistance provided by the following in the production of this guideline: The Professional Standards Group BMUS 2019-2020: Chair: Mrs Catherine Kirkpatrick Consultant Sonographer Professor (Dr.) Rhodri Evans BMUS President. Consultant Radiologist Mrs Pamela Parker BMUS President Elect. Consultant Sonographer Dr Peter Cantin PhD. Consultant Sonographer Dr Oliver Byass. Consultant Radiologist Miss Alison Hall Consultant Sonographer Mrs Hazel Edwards Sonographer Mr Gerry Johnson Consultant Sonographer Dr. Mike Smith PhD. Physiotherapist/Senior Lecturer Professor (Dr.) Adrian Lim, Consultant Radiologist In addition, the documentation and protocol evidence from Hull University Teaching Hospitals NHS Trust, Plymouth NHS Trusts and United Lincolnshire Hospitals NHS Trust for template derivation. Foreword The introduction of this guidance document regarding the diagnosis and management of incidental findings is timely. The changing landscapes of ultrasound practice combined with the significant communication challenges within a variety of referral sources can often add to the pressures exerted on the ultrasound practitioner. The demand for diagnostic ultrasound examinations is ever increasing. Faster patient throughput and increasing complexities of patient management, coupled with advancing ultrasound technologies leads to an inevitable increase in ‘incidentalomas’. The challenges facing ultrasound practitioners include the re-definition of ‘normal’ due to increased resolution of imaging, dilemmas around reporting of incidental findings and managing the effects of this for the patients and the referring clinicians. These guidelines are a resource that can be used as a basis for diagnostic pathways and reporting protocols, and can be modified as appropriate to align with locally agreed protocols. -
LNCS 5242, Pp
Real-Time Simulation of Medical Ultrasound from CT Images Ramtin Shams1, Richard Hartley1,2, and Nassir Navab3 1 RSISE, The Australian National University, Canberra 2 NICTA, Canberra, Australia 3 Computer Aided Medical Procedures (CAMP), TU M¨unchen, Germany Abstract. Medical ultrasound interpretation requires a great deal of experience. Real-time simulation of medical ultrasound provides a cost- effective tool for training and easy access to a variety of cases and ex- ercises. However, fully synthetic and realistic simulation of ultrasound is complex and extremely time-consuming. In this paper, we present a novel method for simulation of ultrasound images from 3D CT scans by breaking down the computations into a preprocessing and a run-time phase. The preprocessing phase produces detailed fixed-view 3D scatter- ing images and the run-time phase generates view-dependent ultrasonic artifacts for a given aperture geometry and position within a volume of interest. We develop a simple acoustic model of the ultrasound for the run-time phase, which produces realistic ultrasound images in real-time when combined with the previously computed scattering image. 1 Introduction Ultrasound is a challenging imaging modality to master due to a multitude of pa- rameters involved in acquisition and interpretation of resulting images. Real-time simulation of ultrasound can be used for training to complement a theoretical study program. A recent study in [1] reports a significant improvement in skills of subjects who received additional simulator-based training. The main advantage is easy access to a wealth of standard and rare cases collected over time. Existing methods for real-time simulation of ultrasound such as [2,3,4] are based on acquisition of actual ultrasound images and creating a compounded 3D volume of the region of interest. -
Scope of Practice and Clinical Standards for the Diagnostic Medical Sonographer
Scope of Practice and Clinical Standards for the Diagnostic Medical Sonographer April 13, 2015 This page intentionally left blank. © 2013-2015 by the participating organizations as a “joint work” as defined in 17 U.S. Code § 101 (the Copyright Act). Contact the Society of Diagnostic Medical Sonography for more information. 2 SCOPE OF PRACTICE REVISION PROCESS In May 2013, representatives of sixteen organizations came together to begin the process of revising the existing Scope of Practice and Clinical Practice Standards. Thus began a process that engaged the participating organizations in an unrestricted dialogue about needed changes. The collaborative process and exchange of ideas has led to this document, which is reflective of the current community standard of care. The current participants recommend a similar collaborative process for future revisions that may be required as changes in ultrasound technologies and healthcare occur. PARTICIPATING ORGANIZATIONS The following organizations participated in the development of this document. Those organizations that have formally endorsed the document are identified with the “†” symbol. Supporting organizations are identified with the "*" symbol. • American College of Radiology (ACR) * • American Congress of Obstetricians and Gynecologists (ACOG) * • American Institute of Ultrasound in Medicine (AIUM) * • American Registry for Diagnostic Medical Sonography (ARDMS) * • American Registry of Radiologic Technologists (ARRT) * • American Society of Echocardiography (ASE) † • American Society of -
Lecture 21: the Doppler Effect
Matthew Schwartz Lecture 21: The Doppler effect 1 Moving sources We’d like to understand what happens when waves are produced from a moving source. Let’s say we have a source emitting sound with the frequency ν. In this case, the maxima of the 1 amplitude of the wave produced occur at intervals of the period T = ν . If the source is at rest, an observer would receive these maxima spaced by T . If we draw the waves, the maxima are separated by a wavelength λ = Tcs, with cs the speed of sound. Now, say the source is moving at velocity vs. After the source emits one maximum, it moves a distance vsT towards the observer before it emits the next maximum. Thus the two successive maxima will be closer than λ apart. In fact, they will be λahead = (cs vs)T apart. The second maximum will arrive in less than T from the first blip. It will arrive with− period λahead cs vs Tahead = = − T (1) cs cs The frequency of the blips/maxima directly ahead of the siren is thus 1 cs 1 cs νahead = = = ν . (2) T cs vs T cs vs ahead − − In other words, if the source is traveling directly towards us, the frequency we hear is shifted c upwards by a factor of s . cs − vs We can do a similar calculation for the case in which the source is traveling directly away from us with velocity v. In this case, in between pulses, the source travels a distance T and the old pulse travels outwards by a distance csT .