Doppler Sonography: a Brief History
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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. -
Intrarenal Doppler Ultrasonography Reflects Hemodynamics and Predicts
www.nature.com/scientificreports OPEN Intrarenal Doppler ultrasonography refects hemodynamics and predicts prognosis in patients with heart failure Akiomi Yoshihisa1*, Koichiro Watanabe1, Yu Sato1, Shinji Ishibashi2, Mitsuko Matsuda2, Yukio Yamadera2, Yasuhiro Ichijo1, Tetsuro Yokokawa1, Tomofumi Misaka1, Masayoshi Oikawa1, Atsushi Kobayashi1 & Yasuchika Takeishi1 We aimed to clarify clinical implications of intrarenal hemodynamics assessed by intrarenal Doppler ultrasonography (IRD) and their prognostic impacts in heart failure (HF). We performed a prospective observational study, and examined IRD and measured interlobar renal artery velocity time integral (VTI) and intrarenal venous fow (IRVF) patterns (monophasic or non-monophasic pattern) to assess intrarenal hypoperfusion and congestion in HF patients (n = 341). Seven patients were excluded in VTI analysis due to unclear imaging. The patients were divided into groups based on (A) VTI: high VTI (VTI ≥ 14.0 cm, n = 231) or low VTI (VTI < 14.0 cm, n = 103); and (B) IRVF patterns: monophasic (n = 36) or non-monophasic (n = 305). We compared post-discharge cardiac event rate between the groups, and right-heart catheterization was performed in 166 patients. Cardiac index was lower in low VTI than in high VTI (P = 0.04), and right atrial pressure was higher in monophasic than in non-monophasic (P = 0.03). In the Kaplan–Meier analysis, cardiac event rate was higher in low VTI and monophasic groups (P < 0.01, respectively). In the Cox proportional hazard analysis, the combination of low VTI and a monophasic IRVF pattern was a predictor of cardiac events (P < 0.01). IRD imaging might be associated with cardiac output and right atrial pressure, and prognosis. -
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. -
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. -
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 . -
Evaluation of Systolic Murmurs by Doppler Ultrasonography
Br Heart J: first published as 10.1136/hrt.50.4.337 on 1 October 1983. Downloaded from Br HeartJ 1983; 50: 337-42 Evaluation of systolic murmurs by Doppler ultrasonography ANDREAS HOFFMANN, DIETER BURCKHARDT From the Deparment ofCardiology, University Hospital, Bask., Switzerland SUMMARY Non-invasive continuous and pulsed wave Doppler ultrasonography was performed in 102 consecutive patients with clinically ill defined systolic murmurs to differentiate between flow murmurs, mitral regurgitation, aortic stenosis, and ventricular septal defect, as well as to assess the severity of aortic stenosis. Diagnoses with the Doppler method were based on velocity, direction, and duration of flow signals and were subsequently verified by cardiac catheterisation in all patients. Multiple evaluations were made in 31 patients. Sensitivity and specificity were 0-87 and 0 77 in mitral regurgitation, 0.9 and 1.0 in aortic stenosis, and 1.0 and 1.0 in ventricular septal defect. In 67 patients the estimation of severity of aortic stenosis using the Doppler technique to calculate aortic pressure gradients from maximum flow velocity was significantly correlated with that determined at catheterisation. It is concluded that Doppler ultrasonography is a highly useful technique for the non-invasive evaluation of clinically ill defined systolic murmurs. Systolic murmurs may present difficult diagnostic were studied before catheterisation using non-invasive problems, even to the experienced clinician. This is Doppler ultrasonography.'45 The problems to be especially -
The Search for Christian Doppler
meeting summary Report from the International Workshop on Remote Sensing in Geophysics Using Doppler Techniques* Arnaldo Brandolini,a+ Ben B. Balsley,b# Antonio Mabres,c# Ronald F. Woodman,d# Carlo Capsoni,3 Michele D'Amico,3 Warner L. Ecklund,e Tor Hagfors/ Robert Harper^ Malcolm L. Heron,h Wayne K. Hocking; Markku S. Lehtinen; Jurgen Rottger,k Martin F. Sarango,d Torn Sato,1 Richard J. Stauch,m J. M. Vaughn," Lucy R. Wyatt,0 and Dusan S. Zrnic? 1. Introduction (A. Brandolini, B. Balsley, in different application areas of Doppler remote sens- A. Mabres, R. Woodman) ing. Actually, Doppler remote sensing is employed in a wide range of applications, from atmospheric bound- The International Workshop on Remote Sensing in ary layer sensing to wind profiling, from sea surface Geophysics Using Doppler Techniques was held on 11- sensing to radar astronomy. Such different applications 15 March 1996 in Bellagio, Italy, at the Rockefeller face different challenges, which sometimes lead to Study and Conference Center. Supported by the development of very different techniques. Rockefeller Foundation, the workshop brought to- In the organizers' opinion, a discussion of such gether a small number of expert researchers working techniques between researchers working in different application areas could be both interesting and useful. *Organized by the Department of Electrical Engineering of In particular, ideas of signal-processing techniques Politecnico di Milano. could be profitably exchanged. The purpose of the +Workshop organizing committee. workshop was in fact to provide a forum where such aPolitecnico di Milano, Milan, Italy. a discussion could take place. bUniversity of Colorado at Boulder, Boulder, Colorado. -
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teaching and education Synchrotron radiation and X-ray free-electron lasers (X-FELs) explained to all users, active and potential ISSN 1600-5775 Yeukuang Hwua,b,c* and Giorgio Margaritondod* aInstitute of Physics, Academia Sinica, Taipei 11529, Taiwan, bDepartment of Engineering Science, National Cheng Kung University, Tainan 70101, Taiwan, cBrain Research Center, National Tsing Hua University, Hsinchu 30013, Taiwan, and dFaculte´ des Sciences de Base, Ecole Polytechnique Fe´de´rale de Lausanne, 1015 Lausanne, Switzerland. Received 8 September 2020 *Correspondence e-mail: [email protected], [email protected] Accepted 29 March 2021 Synchrotron radiation evolved over one-half century into a gigantic worldwide Edited by M. Yamamoto, RIKEN SPring-8 enterprise involving tens of thousands of researchers. Initially, almost all users Center, Japan were physicists. But now they belong to a variety of disciplines: chemistry, materials science, the life sciences, medical research, ecology, cultural heritage Keywords: synchrotron; X-FEL; relativity; and others. This poses a challenge: explaining synchrotron sources without ponderomotive. requiring a sophisticated background in theoretical physics. Here this challenge is met with an innovative approach that only involves elementary notions, commonly possessed by scientists of all domains. 1. Background Synchrotron radiation sources and free-electron lasers (Margaritondo, 1988, 2002; Winick, 1995; Willmott, 2011; Mobilio et al., 2015; Bordovitsyn, 1999) are, arguably, the most important practical applications of Albert Einstein’s special relativity (Rafelski, 2017). Indeed, they exploit relativistic properties to produce electromagnetic radiation in spectral ranges where other emitters are unsatisfactory, most notably X-rays. Explaining such sources to non-physicists is not easy. We propose here an approach that only requires a few basic scientific notions. -
Color Doppler Ultrasonography and Multislice Computer Tomography
Volumen 68, Broj 5 VOJNOSANITETSKI PREGLED Strana 423 UDC: 616.133-073 ORIGINAL ARTICLE DOI:10.2298/VSP1105423V Color Doppler ultrasonography and multislice computer tomography angiography in carotid plaque detection and characterization Primena kolor dopler ultrasonografije i višeslojne kompjuterizovane tomografske angiografije u otkrivanju i karakterizaciji karotidnog plaka Viktorija Vučaj-Ćirilović*, Miloš Lučić†, Kosta Petrović*, Olivera Nikolić*, Mira Govorčin*, Sanja Stojanović* *Clinical Center of Vojvodina, Radiology Department, Novi Sad, Serbia; †Vojvodina Institute of Oncology, Center for Imaging Diagnostics, Sremska Kamenica, Serbia Abstract 97%; for plaques with irregular surface CDU 75% : MSCTA 87%; for ulcerations CDU 54% : MSCTA 87%). Regarding Beckground/Aim. Cerebrovascular diseases are the third determination of plaque structure (mixed plaque CDU 66% leading cause of mortality in the world, following malignant : MSCTA 70%; correlation with HP findings CDU 94% : and cardiovascular diseases. Therefore, their timely and pre- MSCTA 96%) and localization (CDU 63% : MSCTA 65%), cise diagnostics is of great importance. The aim of this study and in terms of sensitivity and specificity, both methods was to compare duplex scan Color Doppler ultrasonogra- showed almost the same results. Also, there is no statistical phy (CDU) with multislice computed tomography angiog- difference between these two methods for the degree of raphy (MSCTA) in detection of morphological and func- stenosis (CDU 96% : MSCTA 98%). Conclusion. Athero- tional disorders at extracranial level of carotid arteries. sclerotic disease of extracranial part of carotid arteries pri- Methods. The study included 75 patients with 150 carotid marily affects population of middle-aged and elderly, arteries examined in the period from January 2008 to April showing more associated risk factors.