What is turbulence? Daniel P. Lathrop University of Maryland
|
|
- Andrea Hopkins
- 5 years ago
- Views:
Transcription
1
2 What is turbulence? Daniel P. Lathrop University of Maryland Goal: grant an intuitive sense of turbulence and its importance in nature, science, and engineering Outline: 1. Definitions 2. Examples 1. Geophysics 2. Astrophysics 3. Engineering 4. Quantum turbulence 5. Optical turbulence
3 Turbulence: an emergent phenomena Rivers!" Niagra Falls"
4 Reynolds number R or Re = U L / ν Re ~ Inertia / viscosity Large R Turbulence
5 Turbulence definitions Turbulence: A Spatially extended field with a large, continuous range of aperiodic spatial and temporal dynamics Newtonian fluid turbulence: Turbulence in a classical, Newtonian viscous fluid Kolmogorov turbulence: Turbulence exhibiting spatial power spectra with Quantum turbulence: A turbulent complex field or interacting set of complex fields Optical turbulence: A turbulent field of electromagnetic amplitudes
6 Turbulence at small scale: strain vorticity
7 Watson: You have to admit Holmes that a supernatural explanation to this case is theoretically possible. Holmes: Agreed, but it is useless to theorize before one has data. Inevitably one begins to twist facts to suit theories instead of theories to suit facts.
8
9 So many natural flows are necessarily turbulent, but we cannot simulate them. Turbulence: Fluctuating in time and space Aperiodic Large range of time and length scales Deterministic
10 So many natural flows are necessarily turbulent, but we cannot simulate them. Turbulence: Fluctuating in time and space Aperiodic Large range of time and length scales Deterministic Anyone who attempts to generate random numbers by deterministic means is, of course, living in a state of sin. John von Neumann
11 Volcanic eruptions Eyjafjallajokull 2010"
12 Volcanic eruptions Cleveland volcano"
13 Atmospheric flows Cumulous"
14 Atmospheric flows Cumulonimbus"
15 Atmospheric flows Cumulonimbus" 2000 m m
16 Atmospheric flows Cumulonimbus" 400 m 2000 m
17 Atmospheric flows Cumulonimbus" 400 m 40 m
18 Geophysical turbulence Rivers!"
19 Geophysical turbulence Rivers!" Missouri River" flood"
20
21 Simple Earth Nonrotating; Spherical Isothermal T = o K Zero axial tilt Quiet atmosphere Quiet crust Quiet mantle Quiet core Core magnetics B = 0
22 Simple Earth Nonrotating; Spherical Isothermal T = o K Zero axial tilt Quiet atmosphere Quiet crust Quiet mantle Quiet core Core magnetics B = 0? Habitable Home One Day Period; Oblate spheroid T core / T space ~ o, precessing Turbulent, zonal atmosphere Brittle quaking crust Complex convecting mantle Turbulent convecting core Active self-inducing geodynamo
23
24
25
26
27
28
29 Astrophysical turbulence Galaxy: M51"
30 Solar turbulence:
31
32
33
34 Aerospace Engin. turbulence Rocket Lauch"
35 Aerospace Engin. turbulence Turbofan engine design" Boundary layer turbulence" Subcritical instabilities" "noise driven" Turbulence control:" "suction!"
36 What is meant by JET in fluid dynamics? Turbulent jet" C. Fukushima and J. Westerweel"
37 Quantum Fluids A state of matter with long range quantum order Type of synchronization partial phase sync of the individual atomic wave functions E.g. BEC atomic systems 4 He 3 He Cooper pair electrons in superconductors Vacuum Quantum Turbulence > turbulence in a quantum fluid Why does it matter?
38 Background: Superfluid Helium
39 Two-Fluid Model Superfluid helium acts as if it s a mixture of a normal and superfluid component Normal and superfluid have separate velocity fields v n and v s, respectively
40 Superfluid Order Parameter Order parameter for superfluid helium is a complex field, Ψ(x) = Ae iφ A is amplitude, and φ is the phase Superfluid velocity given by h = Planck s constant m = mass of helium atom
41 Quantized Vortices Lowest energy state: n=1, so φ wraps 2π around a defect Induces a superflow around the line:
42
43 What is quantum turbulence? An evolving set of quantized vortices: aperiodic large range of length scales and curvatures rings vortices ending at walls knots Simulations by Patricio Jeraldo and Nigel Goldenfeld
44
45 What is turbulence? Daniel P. Lathrop University of Maryland Goal: grant an intuitive sense of turbulence and its importance in nature, science, and engineering Outline: 1. Definitions 2. Examples: 1. Geophysics 2. Astrophysics 3. Engineering 4. Quantum turbulence 5. Optical turbulence
Theoretical physics. Deterministic chaos in classical physics. Martin Scholtz
Theoretical physics Deterministic chaos in classical physics Martin Scholtz scholtzzz@gmail.com Fundamental physical theories and role of classical mechanics. Intuitive characteristics of chaos. Newton
More information(1) BEC (2) BEC (1) (BEC) BEC BEC (5) BEC (LT) (QFS) BEC (3) BEC. 3 He. 4 He. 4 He 3 He
22 (BEC) 4 He BEC We study theoretically and experimentally quantum hydrodynamics in quantum condensed phases at low temperature, namely superfluid helium and atomic Bose-Einstein condensates (BECs). Quantum
More informationSUPERFLUID TURBULENCE
SUPERFLUID TURBULENCE Carlo F. Barenghi School of Mathematics, University of Newcastle Acknowledgments: Demos Kivotides, Daniel Poole, Anthony Youd and Yuri Sergeev (Newcastle), Joe Vinen (Birmingham),
More informationThe Physics of Fluids and Plasmas
The Physics of Fluids and Plasmas An Introduction for Astrophysicists ARNAB RAI CHOUDHURI CAMBRIDGE UNIVERSITY PRESS Preface Acknowledgements xiii xvii Introduction 1 1. 3 1.1 Fluids and plasmas in the
More informationLecture 7. Turbulence
Lecture 7 Content Basic features of turbulence Energy cascade theory scales mixing Basic features of turbulence What is turbulence? spiral galaxies NGC 2207 and IC 2163 Turbulent jet flow Volcano jet flow
More informationEXACT SOLUTIONS TO THE NAVIER-STOKES EQUATION FOR AN INCOMPRESSIBLE FLOW FROM THE INTERPRETATION OF THE SCHRÖDINGER WAVE FUNCTION
EXACT SOLUTIONS TO THE NAVIER-STOKES EQUATION FOR AN INCOMPRESSIBLE FLOW FROM THE INTERPRETATION OF THE SCHRÖDINGER WAVE FUNCTION Vladimir V. KULISH & José L. LAGE School of Mechanical & Aerospace Engineering,
More informationThe Superfluid Phase s of Helium 3
The Superfluid Phase s of Helium 3 DIETER VOLLHARD T Rheinisch-Westfälische Technische Hochschule Aachen, Federal Republic of German y PETER WÖLFL E Universität Karlsruhe Federal Republic of Germany PREFACE
More informationTemperature Effects and Oscillations on Vortices in Superfluid Helium
Temperature Effects and Oscillations on Vortices in Superfluid Helium May Palace and Dr. Rena Zieve UC Davis 2015 Physics REU A new measurement technique for studying kelvin wave oscillations along vortices
More informationFLUID MECHANICS. ! Atmosphere, Ocean. ! Aerodynamics. ! Energy conversion. ! Transport of heat/other. ! Numerous industrial processes
SG2214 Anders Dahlkild Luca Brandt FLUID MECHANICS : SG2214 Course requirements (7.5 cr.)! INL 1 (3 cr.)! 3 sets of home work problems (for 10 p. on written exam)! 1 laboration! TEN1 (4.5 cr.)! 1 written
More informationFluid Dynamics Exercises and questions for the course
Fluid Dynamics Exercises and questions for the course January 15, 2014 A two dimensional flow field characterised by the following velocity components in polar coordinates is called a free vortex: u r
More informationRole of polymers in the mixing of Rayleigh-Taylor turbulence
Physics Department University of Genova Italy Role of polymers in the mixing of Rayleigh-Taylor turbulence Andrea Mazzino andrea.mazzino@unige.it Guido Boffetta: University of Torino (Italy) Stefano Musacchio:
More informationFLUID MECHANICS. Atmosphere, Ocean. Aerodynamics. Energy conversion. Transport of heat/other. Numerous industrial processes
SG2214 Anders Dahlkild Luca Brandt FLUID MECHANICS : SG2214 Course requirements (7.5 cr.) INL 1 (3 cr.) 3 sets of home work problems (for 10 p. on written exam) 1 laboration TEN1 (4.5 cr.) 1 written exam
More information3-Fold Decomposition EFB Closure for Convective Turbulence and Organized Structures
3-Fold Decomposition EFB Closure for Convective Turbulence and Organized Structures Igor ROGACHEVSKII and Nathan KLEEORIN Ben-Gurion University of the Negev, Beer-Sheva, Israel N.I. Lobachevsky State University
More informationTheory and modelling of turbulent transport in astrophysical phenomena
MHD 2017 Tokyo, 29 August 2017 Theory and modelling of turbulent transport in astrophysical phenomena Nobumitsu YOKOI Institute of Industrial Science (IIS), University of Tokyo In collaboration with Akira
More informationPlanetary dynamos: Dipole-multipole transition and dipole reversals
Planetary dynamos: Dipole-multipole transition and dipole reversals Ulrich Christensen Max-Planck-Institute for Solar System Research Katlenburg-Lindau, Germany in collaboration with Hagay Amit, Julien
More informationConvection-driven dynamos in the limit of rapid rotation
Convection-driven dynamos in the limit of rapid rotation Michael A. Calkins Jonathan M. Aurnou (UCLA), Keith Julien (CU), Louie Long (CU), Philippe Marti (CU), Steven M. Tobias (Leeds) *Department of Physics,
More informationSuperfluidity. v s. E. V. Thuneberg Department of Physical Sciences, P.O.Box 3000, FIN University of Oulu, Finland (Dated: June 8, 2012)
Superfluidity E. V. Thuneberg Department of Physical Sciences, P.O.Box 3000, FIN-90014 University of Oulu, Finland (Dated: June 8, 01) PACS numbers: 67.40.-w, 67.57.-z, 74., 03.75.-b I. INTRODUCTION Fluids
More informationTurbulent Rankine Vortices
Turbulent Rankine Vortices Roger Kingdon April 2008 Turbulent Rankine Vortices Overview of key results in the theory of turbulence Motivation for a fresh perspective on turbulence The Rankine vortex CFD
More informationEffects of Forcing Scheme on the Flow and the Relative Motion of Inertial Particles in DNS of Isotropic Turbulence
Effects of Forcing Scheme on the Flow and the Relative Motion of Inertial Particles in DNS of Isotropic Turbulence Rohit Dhariwal and Vijaya Rani PI: Sarma L. Rani Department of Mechanical and Aerospace
More informationWorkshop on Supersolid August Brief introduction to the field. M. Chan Pennsylvania State University, USA
1959-11 Workshop on Supersolid 2008 18-22 August 2008 Brief introduction to the field M. Chan Pennsylvania State University, USA Superfluid and supersolid An introduction at the ICTP Supersolid 2008 workshop
More informationQuantum vortex reconnections
Quantum vortex reconnections A.W. Baggaley 1,2, S. Zuccher 4, Carlo F Barenghi 2, 3, A.J. Youd 2 1 University of Glasgow 2 Joint Quantum Centre Durham-Newcastle 3 Newcastle University 4 University of Verona
More informationGeneration of magnetic fields by large-scale vortices in rotating convection
Generation of magnetic fields by large-scale vortices in rotating convection Céline Guervilly, David Hughes & Chris Jones School of Mathematics, University of Leeds, UK Generation of the geomagnetic field
More informationProblem 4.3. Problem 4.4
Problem 4.3 Problem 4.4 Problem 4.5 Problem 4.6 Problem 4.7 This is forced convection flow over a streamlined body. Viscous (velocity) boundary layer approximations can be made if the Reynolds number Re
More informationNonmodal Growth and the Unstratified MRI Dynamo
MPPC general meeting, Berlin, June 24 Nonmodal Growth and the Unstratified MRI Dynamo Jonathan Squire!! and!! Amitava Bhattacharjee MRI turbulence Observed accretion rate in disks in astrophysical disks
More informationCandidates must show on each answer book the type of calculator used. Log Tables, Statistical Tables and Graph Paper are available on request.
UNIVERSITY OF EAST ANGLIA School of Mathematics Spring Semester Examination 2004 FLUID DYNAMICS Time allowed: 3 hours Attempt Question 1 and FOUR other questions. Candidates must show on each answer book
More informationComputational Fluid Dynamics 2
Seite 1 Introduction Computational Fluid Dynamics 11.07.2016 Computational Fluid Dynamics 2 Turbulence effects and Particle transport Martin Pietsch Computational Biomechanics Summer Term 2016 Seite 2
More informationSuperfluid Helium-3: From very low Temperatures to the Big Bang
Superfluid Helium-3: From very low Temperatures to the Big Bang Dieter Vollhardt Yukawa Institute, Kyoto; November 27, 2007 Contents: The quantum liquids 3 He and 4 He Superfluid phases of 3 He Broken
More informationIntroduction to Turbulence AEEM Why study turbulent flows?
Introduction to Turbulence AEEM 7063-003 Dr. Peter J. Disimile UC-FEST Department of Aerospace Engineering Peter.disimile@uc.edu Intro to Turbulence: C1A Why 1 Most flows encountered in engineering and
More informationSuperfluid Helium-3: From very low Temperatures to the Big Bang
Superfluid Helium-3: From very low Temperatures to the Big Bang Universität Frankfurt; May 30, 2007 Dieter Vollhardt Contents: The quantum liquids 3 He and 4 He Superfluid phases of 3 He Broken symmetries
More information1 Superfluidity and Bose Einstein Condensate
Physics 223b Lecture 4 Caltech, 04/11/18 1 Superfluidity and Bose Einstein Condensate 1.6 Superfluid phase: topological defect Besides such smooth gapless excitations, superfluid can also support a very
More informationEffects of Forcing Scheme on the Flow and the Relative Motion of Inertial Particles in DNS of Isotropic Turbulence
Effects of Forcing Scheme on the Flow and the Relative Motion of Inertial Particles in DNS of Isotropic Turbulence Rohit Dhariwal PI: Sarma L. Rani Department of Mechanical and Aerospace Engineering The
More informationNeutron Stars: Observations
Neutron Stars: Observations Ian Jones School of Mathematics, University of Southampton, UK Neutron star observations: overview From the observational point of view, neutron stars come in many different
More informationContents. I Introduction 1. Preface. xiii
Contents Preface xiii I Introduction 1 1 Continuous matter 3 1.1 Molecules................................ 4 1.2 The continuum approximation.................... 6 1.3 Newtonian mechanics.........................
More informationCorrelation: California State Curriculum Standards of Science for Grade 6 Focus on Earth Science
Correlation: California State Curriculum Standards of Science for Grade 6 Focus on Earth Science To Science Workshop Series Earth Science: Geology The Universe Oceans and Atmosphere Plate Tectonics and
More informationStudy of superfluidity in magnetars by van Hoven and Levin
Study of superfluidity in magnetars by van Hoven and Levin Overview What is a superfluid and how does it look like in neutron stars? What can happen when both a superfluid and a strong magnetic field are
More informationThermographic analysis of turbulent non-isothermal water boundary layer
Thermographic analysis of turbulent non-isothermal water boundary layer Irina A. Znamenskaya 1,*, Ekaterina Y. Koroteeva 1, Anastasiya M. Novinskaya 1, Vladimir I. Fomichev 2 1 Faculty of Physics, Lomonosov
More informationTurbulence Instability
Turbulence Instability 1) All flows become unstable above a certain Reynolds number. 2) At low Reynolds numbers flows are laminar. 3) For high Reynolds numbers flows are turbulent. 4) The transition occurs
More informationWhat is Earth Science? Earth science is the branch of science dealing with the constitution of the earth and its atmosphere.
What is Earth Science? Earth science is the branch of science dealing with the constitution of the earth and its atmosphere. 1 2 The Branches of Earth Science Major Astronomy (celestial objects, space,
More informationSpherical Shallow Water Turbulence: Cyclone-Anticyclone Asymmetry, Potential Vorticity Homogenisation and Jet Formation
Spherical Shallow Water Turbulence: Cyclone-Anticyclone Asymmetry, Potential Vorticity Homogenisation and Jet Formation Jemma Shipton Department of Atmospheric, Oceanic and Planetary Physics, University
More informationVortex Induced Vibrations
Vortex Induced Vibrations By: Abhiroop Jayanthi Indian Institute of Technology, Delhi Some Questions! What is VIV? What are the details of a steady approach flow past a stationary cylinder? How and why
More informationQuantum fluids are compressible In any compressible vortex cores have low density. Example: Tornados
KITP, Santa Barbara 15 February 2011 Vortex Stretching as a Mechanism for Quantum Kinetic Energy Decay Robert M. Kerr, Warwick University Left: Classical Euler, isosurfaces of high vorticity magnitude.
More informationThe influence of short wavelength variations in viscosity on subduction dynamics
1 Introduction Deformation within the earth, driven by mantle convection due primarily to cooling and subduction of oceanic lithosphere, is expressed at every length scale in various geophysical observations.
More informationQuestions that science may help to answer. This module offers opportunities to develop mathematics skills. For example:
3.3.1 Module P1: The Earth in the Universe Overview Scienti c discoveries in the solar system and beyond continue to inspire popular culture and affect our understanding of our place in the Universe. In
More informationThe Madison Dynamo Experiment: magnetic instabilities driven by sheared flow in a sphere. Cary Forest Department of Physics University of Wisconsin
The Madison Dynamo Experiment: magnetic instabilities driven by sheared flow in a sphere Cary Forest Department of Physics University of Wisconsin February 28, 2001 Planets, stars and perhaps the galaxy
More informationCALIFORNIA CONTENT STANDARDS FOCUS ON EARTH SCIENCE, Grade 6. Correlated to AGS EARTH SCIENCE
CALIFORNIA CONTENT STANDARDS FOCUS ON EARTH SCIENCE, Grade 6 Correlated to AGS EARTH SCIENCE PLATE TECTONICS AND EARTH S STRUCTURE 1. Plate tectonics accounts for important features of Earth s surface
More informationVegard B. Sørdal. Thermodynamics of 4He-3He mixture and application in dilution refrigeration
Vegard B. Sørdal Thermodynamics of 4He-3He mixture and application in dilution refrigeration 1. Introduction 2. Crogenic methods Contents of the presentation 3. Properties of Helium 4. Superfluid Helium
More informationThe JHU Turbulence Databases (JHTDB)
The JHU Turbulence Databases (JHTDB) TURBULENT CHANNEL FLOW AT Re τ = 5200 DATA SET Data provenance: M. Lee 1 & R. D. Moser 1 Database ingest and Web Services: Z. Wu 2, G. Lemson 2, R. Burns 2, A. Szalay
More informationLecture 4: Superfluidity
Lecture 4: Superfluidity Previous lecture: Elementary excitations above condensate are phonons in the low energy limit. This lecture Rotation of superfluid helium. Hess-Fairbank effect and persistent currents
More informationVortices and other topological defects in ultracold atomic gases
Vortices and other topological defects in ultracold atomic gases Michikazu Kobayashi (Kyoto Univ.) 1. Introduction of topological defects in ultracold atoms 2. Kosterlitz-Thouless transition in spinor
More informationFundamentals of Fluid Dynamics: Elementary Viscous Flow
Fundamentals of Fluid Dynamics: Elementary Viscous Flow Introductory Course on Multiphysics Modelling TOMASZ G. ZIELIŃSKI bluebox.ippt.pan.pl/ tzielins/ Institute of Fundamental Technological Research
More informationProperties of Light and Atomic Structure. Chapter 7. So Where are the Electrons? Electronic Structure of Atoms. The Wave Nature of Light!
Properties of Light and Atomic Structure Chapter 7 So Where are the Electrons? We know where the protons and neutrons are Nuclear structure of atoms (Chapter 2) The interaction of light and matter helps
More informationA Simulation Model for Drift Resistive Ballooning Turbulence Examining the Influence of Self-consistent Zonal Flows *
A Simulation Model for Drift Resistive Ballooning Turbulence Examining the Influence of Self-consistent Zonal Flows * Bruce I. Cohen, Maxim V. Umansky, Ilon Joseph Lawrence Livermore National Laboratory
More informationNumerical Simulation of the Mantle Convection and Subduction Process
Numerical Simulation of the Mantle Convection and Subduction Process Project Representative Yoshio Fukao Institute for Research on Earth Evolution, Japan Agency for Marine-Earth Science and Technology
More informationA Superfluid Universe
A Superfluid Universe Lecture 2 Quantum field theory & superfluidity Kerson Huang MIT & IAS, NTU Lecture 2. Quantum fields The dynamical vacuum Vacuumscalar field Superfluidity Ginsburg Landau theory BEC
More informationWhy does the magnetic field of the Earth reverse?
IMPRS Solar System Seminar June 2002 Why does the magnetic field of the Earth reverse? Dieter Schmitt (Katlenburg-Lindau) 1. Geomagnetic field >99% of matter in universe is plasma: gas of electrons, ions
More informationNumerical Methods in Aerodynamics. Turbulence Modeling. Lecture 5: Turbulence modeling
Turbulence Modeling Niels N. Sørensen Professor MSO, Ph.D. Department of Civil Engineering, Alborg University & Wind Energy Department, Risø National Laboratory Technical University of Denmark 1 Outline
More informationTurbulent Boundary Layers & Turbulence Models. Lecture 09
Turbulent Boundary Layers & Turbulence Models Lecture 09 The turbulent boundary layer In turbulent flow, the boundary layer is defined as the thin region on the surface of a body in which viscous effects
More informationLow dimensional turbulence
Low dimensional turbulence F. Daviaud in collaboration with A. Chiffaudel, B. Dubrulle P.-P. Cortet, P. Diribarne, D. Faranda, E. Herbert, L. Marié, R. Monchaux, F. Ravelet, B. Saint-Michel, C. Wiertel
More informationGravity Tectonics Volcanism Atmosphere Water Winds Chemistry. Planetary Surfaces
Gravity Tectonics Volcanism Atmosphere Water Winds Chemistry Planetary Surfaces Gravity & Rotation Polar flattening caused by rotation is the largest deviation from a sphere for a planet sized object (as
More informationModeling of turbulence in stirred vessels using large eddy simulation
Modeling of turbulence in stirred vessels using large eddy simulation André Bakker (presenter), Kumar Dhanasekharan, Ahmad Haidari, and Sung-Eun Kim Fluent Inc. Presented at CHISA 2002 August 25-29, Prague,
More informationA Living Planet. Chapter PHYSICAL GEOGRAPHY. What you will learn in this chapter. Summary of the chapter
QUIT Main Ideas What you will learn in this chapter Summary Summary of the chapter Test your geographic knowledge by playing the. Main Ideas Section 1: The Earth Inside and Out The earth is the only habitable
More informationHow can solid rock be bent, squished, stretched, and cracked?
AST 105 Intro Astronomy The Solar System MIDTERM II: Tuesday, April 5 4 Processes that Shape Surfaces Volcanism Eruption of molten rock onto surface Impact cratering Impacts by asteroids or comets Tectonics
More informationNonlinear Evolution of a Vortex Ring
Nonlinear Evolution of a Vortex Ring Yuji Hattori Kyushu Institute of Technology, JAPAN Yasuhide Fukumoto Kyushu University, JAPAN EUROMECH Colloquium 491 Vortex dynamics from quantum to geophysical scales
More informationCONDENSED MATTER: towards Absolute Zero
CONDENSED MATTER: towards Absolute Zero The lowest temperatures reached for bulk matter between 1970-2000 AD. We have seen the voyages to inner & outer space in physics. There is also a voyage to the ultra-cold,
More informationThe phases of matter familiar for us from everyday life are: solid, liquid, gas and plasma (e.f. flames of fire). There are, however, many other
1 The phases of matter familiar for us from everyday life are: solid, liquid, gas and plasma (e.f. flames of fire). There are, however, many other phases of matter that have been experimentally observed,
More informationS6E1. Obtain, evaluate, and communicate information about current scientific views of the universe and how those views evolved. a.
S6E1. Obtain, evaluate, and communicate information about current scientific views of the universe and how those views evolved. a. Ask questions to determine changes in models of Earth s position in the
More informationShape and Size of the Earth
Planet Earth Shape and Size of the Earth Gravity is what gives Earth its spherical shape Only effective if the body is of a critical size Critical radius is about 350 km Shape and Size of the Earth Earth
More informationGeodynamo Simulations and Electromagnetic Induction Studies
Chapter 2 Solid Earth Simulation Geodynamo Simulations and Electromagnetic Induction Studies Project Representative Yozo Hamano Japan Agency for Marine-Earth Science and Technology Authors Yozo Hamano
More informationContents. 1.1 Prerequisites and textbooks Physical phenomena and theoretical tools The path integrals... 9
Preface v Chapter 1 Introduction 1 1.1 Prerequisites and textbooks......................... 1 1.2 Physical phenomena and theoretical tools................. 5 1.3 The path integrals..............................
More informationMHD turbulence in the solar corona and solar wind
MHD turbulence in the solar corona and solar wind Pablo Dmitruk Departamento de Física, FCEN, Universidad de Buenos Aires Motivations The role of MHD turbulence in several phenomena in space and solar
More informationPhysics 127a: Class Notes
Physics 127a: Class Notes Lecture 15: Statistical Mechanics of Superfluidity Elementary excitations/quasiparticles In general, it is hard to list the energy eigenstates, needed to calculate the statistical
More informationBoundary-Layer Theory
Hermann Schlichting Klaus Gersten Boundary-Layer Theory With contributions from Egon Krause and Herbert Oertel Jr. Translated by Katherine Mayes 8th Revised and Enlarged Edition With 287 Figures and 22
More informationGeneral classifications:
General classifications: Physics is perceived as fundamental basis for study of the universe Chemistry is perceived as fundamental basis for study of life Physics consists of concepts, principles and notions,
More informationQuantum Theory of Matter
Quantum Theory of Matter Overview Lecture Derek Lee Imperial College London January 2007 Outline 1 Course content Introduction Superfluids Superconductors 2 Course Plan Resources Outline 1 Course content
More informationSuperfluidity and Superconductivity
Superfluidity and Superconductivity These are related phenomena of flow without resistance, but in very different systems Superfluidity: flow of helium IV atoms in a liquid Superconductivity: flow of electron
More informationMagnetic field reversals in turbulent dynamos
Magnetic field reversals in turbulent dynamos Stéphan Fauve LPS-ENS-Paris APS, San Antonio, november 23, 2008 Cosmic magnetic fields Earth 0.5 G Sun 1 G (Hale, 1908) 10 3 G Neutrons stars 10 10-10 13 G
More information7. Basics of Turbulent Flow Figure 1.
1 7. Basics of Turbulent Flow Whether a flow is laminar or turbulent depends of the relative importance of fluid friction (viscosity) and flow inertia. The ratio of inertial to viscous forces is the Reynolds
More informationMixing and Combustion in Dense Mixtures by William A. Sirignano and Derek Dunn-Rankin
Mixing and Combustion in Dense Mixtures by William A. Sirignano and Derek Dunn-Rankin At very high pressures and densities, what is different and what is similar about the processes of Injection and Atomization,
More informationSimulation Study on the Generation and Distortion Process of the Geomagnetic Field in Earth-like Conditions
Chapter 1 Earth Science Simulation Study on the Generation and Distortion Process of the Geomagnetic Field in Earth-like Conditions Project Representative Yozo Hamano Authors Ataru Sakuraba Yusuke Oishi
More informationEffects of Variation of the Flame Area and Natural Damping on Primary Acoustic Instability of Downward Propagating Flames in a Tube
5 th ICDERS August 7, 015 Leeds, UK Effects of Variation of the Flame Area and Natural Damping on Primary Acoustic Instability of Downward Propagating Flames in a Tube Sung Hwan Yoon and Osamu Fujita Division
More informationFluctuation dynamo amplified by intermittent shear bursts
by intermittent Thanks to my collaborators: A. Busse (U. Glasgow), W.-C. Müller (TU Berlin) Dynamics Days Europe 8-12 September 2014 Mini-symposium on Nonlinear Problems in Plasma Astrophysics Introduction
More informationSpace Plasma Physics Thomas Wiegelmann, 2012
Space Plasma Physics Thomas Wiegelmann, 2012 1. Basic Plasma Physics concepts 2. Overview about solar system plasmas Plasma Models 3. Single particle motion, Test particle model 4. Statistic description
More informationInfluence of high temperature gradient on turbulence spectra
NIA CFD Conference, Hampton, August 6-8, 2012 Future Directions in CFD Research, A Modeling and Simulation Conference Influence of high temperature gradient on turbulence spectra Sylvain Serra Françoise
More informationMagnetic field nomenclature
Magnetic field nomenclature Declination trend angle between horizontal projection of F and true North Inclination plunge angle between horizontal and F Magnetic equator location on surface where field
More informationDynamics of Zonal Shear Collapse in Hydrodynamic Electron Limit. Transport Physics of the Density Limit
Dynamics of Zonal Shear Collapse in Hydrodynamic Electron Limit Transport Physics of the Density Limit R. Hajjar, P. H. Diamond, M. Malkov This research was supported by the U.S. Department of Energy,
More informationQuantum Turbulence, and How it is Related to Classical Turbulence
Quantum Turbulence, and How it is Related to Classical Turbulence Xueying Wang xueying8@illinois.edu University of Illinois at Urbana-Champaign May 13, 2018 Abstract Since the discovery of turbulence in
More informationExperimental setup for probing a von Karman type flow of normal and superfluid helium
Journal of Low Temperature Physics - QFS2009 manuscript No. (will be inserted by the editor) Experimental setup for probing a von Karman type flow of normal and superfluid helium D. Schmoranzer L. Skrbek
More informationA descriptive explanation of ocean tides.
A descriptive explanation of ocean tides. by Donald E. Simanek Anyone who has spent some time on a beach has noticed the periodic phenomenon of the tides. The water level at the shoreline rises to a maximum,
More informationTheoretical Geomagnetism. Lecture 2: Self- Exciting Dynamos: Kinematic Theory
Theoretical Geomagnetism Lecture 2: Self- Exciting Dynamos: Kinematic Theory 1 2.0 What is a self-exciting dynamo? Dynamo = A device that converts kinetic energy into electromagnetic energy. Dynamos use
More informationBig Idea Clarifying Statement Assessment boundary
Energy Big Idea Clarifying Statement Assessment boundary HS-PS3-1. Create a computational model to calculate the change in the energy of one component in a system when the change in energy of the other
More informationPhase Oscillation between Superfluid and Normal State of Neutrons in Neutron Stars The Origin of Glitches of Pulsars 1
Phase Oscillation between Superfluid and Normal State of Neutrons in Neutron Stars The Origin of Glitches of Pulsars Qiu-he Peng a,b ( qhpeng@nju.edu.cn ) Zhi quan Luo a,c a School of Physics and electronic
More informationMax Planck Institut für Plasmaphysik
ASDEX Upgrade Max Planck Institut für Plasmaphysik 2D Fluid Turbulence Florian Merz Seminar on Turbulence, 08.09.05 2D turbulence? strictly speaking, there are no two-dimensional flows in nature approximately
More informationThermoacoustic Instabilities Research
Chapter 3 Thermoacoustic Instabilities Research In this chapter, relevant literature survey of thermoacoustic instabilities research is included. An introduction to the phenomena of thermoacoustic instability
More informationSuperfluid Helium-3: From very low Temperatures to the Big Bang
Center for Electronic Correlations and Magnetism University of Augsburg Superfluid Helium-3: From very low Temperatures to the Big Bang Dieter Vollhardt Dvořák Lecture Institute of Physics, Academy of
More informationLecture 2. Turbulent Flow
Lecture 2. Turbulent Flow Note the diverse scales of eddy motion and self-similar appearance at different lengthscales of this turbulent water jet. If L is the size of the largest eddies, only very small
More informationThe Bohr Model of the Atom
Unit 4: The Bohr Model of the Atom Properties of light Before the 1900 s, light was thought to behave only as a wave. Light is a type of electromagnetic radiation - a form of energy that exhibits wave
More informationFluid Mechanics Theory I
Fluid Mechanics Theory I Last Class: 1. Introduction 2. MicroTAS or Lab on a Chip 3. Microfluidics Length Scale 4. Fundamentals 5. Different Aspects of Microfluidcs Today s Contents: 1. Introduction to
More informationTurbulence is a ubiquitous phenomenon in environmental fluid mechanics that dramatically affects flow structure and mixing.
Turbulence is a ubiquitous phenomenon in environmental fluid mechanics that dramatically affects flow structure and mixing. Thus, it is very important to form both a conceptual understanding and a quantitative
More informationNoise, AFMs, and Nanomechanical Biosensors
Noise, AFMs, and Nanomechanical Biosensors: Lancaster University, November, 2005 1 Noise, AFMs, and Nanomechanical Biosensors with Mark Paul (Virginia Tech), and the Caltech BioNEMS Collaboration Support:
More informationVorticity and Dynamics
Vorticity and Dynamics In Navier-Stokes equation Nonlinear term ω u the Lamb vector is related to the nonlinear term u 2 (u ) u = + ω u 2 Sort of Coriolis force in a rotation frame Viscous term ν u = ν
More information