Dynamic Similarity, the Dimensionless Science
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The Influence of Magnetic Fields in Planetary Dynamo Models
Earth and Planetary Science Letters 333–334 (2012) 9–20 Contents lists available at SciVerse ScienceDirect Earth and Planetary Science Letters journal homepage: www.elsevier.com/locate/epsl The influence of magnetic fields in planetary dynamo models Krista M. Soderlund a,n, Eric M. King b, Jonathan M. Aurnou a a Department of Earth and Space Sciences, University of California, Los Angeles, CA 90095, USA b Department of Earth and Planetary Science, University of California, Berkeley, CA 94720, USA article info abstract Article history: The magnetic fields of planets and stars are thought to play an important role in the fluid motions Received 7 November 2011 responsible for their field generation, as magnetic energy is ultimately derived from kinetic energy. We Received in revised form investigate the influence of magnetic fields on convective dynamo models by contrasting them with 27 March 2012 non-magnetic, but otherwise identical, simulations. This survey considers models with Prandtl number Accepted 29 March 2012 Pr¼1; magnetic Prandtl numbers up to Pm¼5; Ekman numbers in the range 10À3 ZEZ10À5; and Editor: T. Spohn Rayleigh numbers from near onset to more than 1000 times critical. Two major points are addressed in this letter. First, we find that the characteristics of convection, Keywords: including convective flow structures and speeds as well as heat transfer efficiency, are not strongly core convection affected by the presence of magnetic fields in most of our models. While Lorentz forces must alter the geodynamo flow to limit the amplitude of magnetic field growth, we find that dynamo action does not necessitate a planetary dynamos dynamo models significant change to the overall flow field. -
Chapter 5 Dimensional Analysis and Similarity
Chapter 5 Dimensional Analysis and Similarity Motivation. In this chapter we discuss the planning, presentation, and interpretation of experimental data. We shall try to convince you that such data are best presented in dimensionless form. Experiments which might result in tables of output, or even mul- tiple volumes of tables, might be reduced to a single set of curves—or even a single curve—when suitably nondimensionalized. The technique for doing this is dimensional analysis. Chapter 3 presented gross control-volume balances of mass, momentum, and en- ergy which led to estimates of global parameters: mass flow, force, torque, total heat transfer. Chapter 4 presented infinitesimal balances which led to the basic partial dif- ferential equations of fluid flow and some particular solutions. These two chapters cov- ered analytical techniques, which are limited to fairly simple geometries and well- defined boundary conditions. Probably one-third of fluid-flow problems can be attacked in this analytical or theoretical manner. The other two-thirds of all fluid problems are too complex, both geometrically and physically, to be solved analytically. They must be tested by experiment. Their behav- ior is reported as experimental data. Such data are much more useful if they are ex- pressed in compact, economic form. Graphs are especially useful, since tabulated data cannot be absorbed, nor can the trends and rates of change be observed, by most en- gineering eyes. These are the motivations for dimensional analysis. The technique is traditional in fluid mechanics and is useful in all engineering and physical sciences, with notable uses also seen in the biological and social sciences. -
Rotating Fluids
26 Rotating fluids The conductor of a carousel knows about fictitious forces. Moving from horse to horse while collecting tickets, he not only has to fight the centrifugal force trying to kick him off, but also has to deal with the dizzying sideways Coriolis force. On a typical carousel with a five meter radius and turning once every six seconds, the centrifugal force is strongest at the rim where it amounts to about 50% of gravity. Walking across the carousel at a normal speed of one meter per second, the conductor experiences a Coriolis force of about 20% of gravity. Provided the carousel turns anticlockwise seen from above, as most carousels seem to do, the Coriolis force always pulls the conductor off his course to the right. The conductor seems to prefer to move from horse to horse against the rotation, and this is quite understandable, since the Coriolis force then counteracts the centrifugal force. The whole world is a carousel, and not only in the metaphorical sense. The centrifugal force on Earth acts like a cylindrical antigravity field, reducing gravity at the equator by 0.3%. This is hardly a worry, unless you have to adjust Olympic records for geographic latitude. The Coriolis force is even less noticeable at Olympic speeds. You have to move as fast as a jet aircraft for it to amount to 0.3% of a percent of gravity. Weather systems and sea currents are so huge and move so slowly compared to Earth’s local rotation speed that the weak Coriolis force can become a major player in their dynamics. -
Executive Committee Meeting 6:00 Pm, November 22, 2008 Marriott Rivercenter Hotel
Executive Committee Meeting 6:00 pm, November 22, 2008 Marriott Rivercenter Hotel Attendees: Steve Pope, Lex Smits, Phil Marcus, Ellen Longmire, Juan Lasheras, Anette Hosoi, Laurette Tuckerman, Jim Brasseur, Paul Steen, Minami Yoda, Martin Maxey, Jean Hertzberg, Monica Malouf, Ken Kiger, Sharath Girimaji, Krishnan Mahesh, Gary Leal, Bill Schultz, Andrea Prosperetti, Julian Domaradzki, Jim Duncan, John Foss, PK Yeung, Ann Karagozian, Lance Collins, Kimberly Hill, Peggy Holland, Jason Bardi (AIP) Note: Attachments related to agenda items follow the order of the agenda and are appended to this document. Key Decisions The ExCom voted to move $100k of operating funds to an endowment for a new award. The ExCom voted that a new name (not Otto Laporte) should be chosen for this award. In the coming year, the Award committee (currently the Fluid Dynamics Prize committee) should establish the award criteria, making sure to distinguish the criteria from those associated with the Batchelor prize. The committee should suggest appropriate wording for the award application and make a recommendation on the naming of the award. The ExCom voted to move Newsletter publication to the first weeks of June and December each year. The ExCom voted to continue the Ad Hoc Committee on Media and Public Relations for two more years (through 2010). The ExCom voted that $15,000 per year in 2009 and 2010 be allocated for Media and Public Relations activities. Most of these funds would be applied toward continuing to use AIP media services in support of news releases and Virtual Pressroom activities related to the annual DFD meeting. Meeting Discussion 1. -
Turbulence, Entropy and Dynamics
TURBULENCE, ENTROPY AND DYNAMICS Lecture Notes, UPC 2014 Jose M. Redondo Contents 1 Turbulence 1 1.1 Features ................................................ 2 1.2 Examples of turbulence ........................................ 3 1.3 Heat and momentum transfer ..................................... 4 1.4 Kolmogorov’s theory of 1941 ..................................... 4 1.5 See also ................................................ 6 1.6 References and notes ......................................... 6 1.7 Further reading ............................................ 7 1.7.1 General ............................................ 7 1.7.2 Original scientific research papers and classic monographs .................. 7 1.8 External links ............................................. 7 2 Turbulence modeling 8 2.1 Closure problem ............................................ 8 2.2 Eddy viscosity ............................................. 8 2.3 Prandtl’s mixing-length concept .................................... 8 2.4 Smagorinsky model for the sub-grid scale eddy viscosity ....................... 8 2.5 Spalart–Allmaras, k–ε and k–ω models ................................ 9 2.6 Common models ........................................... 9 2.7 References ............................................... 9 2.7.1 Notes ............................................. 9 2.7.2 Other ............................................. 9 3 Reynolds stress equation model 10 3.1 Production term ............................................ 10 3.2 Pressure-strain interactions -
Chapter 5 Frictional Boundary Layers
Chapter 5 Frictional boundary layers 5.1 The Ekman layer problem over a solid surface In this chapter we will take up the important question of the role of friction, especially in the case when the friction is relatively small (and we will have to find an objective measure of what we mean by small). As we noted in the last chapter, the no-slip boundary condition has to be satisfied no matter how small friction is but ignoring friction lowers the spatial order of the Navier Stokes equations and makes the satisfaction of the boundary condition impossible. What is the resolution of this fundamental perplexity? At the same time, the examination of this basic fluid mechanical question allows us to investigate a physical phenomenon of great importance to both meteorology and oceanography, the frictional boundary layer in a rotating fluid, called the Ekman Layer. The historical background of this development is very interesting, partly because of the fascinating people involved. Ekman (1874-1954) was a student of the great Norwegian meteorologist, Vilhelm Bjerknes, (himself the father of Jacques Bjerknes who did so much to understand the nature of the Southern Oscillation). Vilhelm Bjerknes, who was the first to seriously attempt to formulate meteorology as a problem in fluid mechanics, was a student of his own father Christian Bjerknes, the physicist who in turn worked with Hertz who was the first to demonstrate the correctness of Maxwell’s formulation of electrodynamics. So, we are part of a joined sequence of scientists going back to the great days of classical physics. -
Turner Takes Over at the NSF
PEOPLE APPOINTMENTS Turner takes over at the NSF On 1 October 2003 the astrophysicist the Physics of the Universe, which earlier this Michael Turner, from the University of year produced a comprehensive report Chicago in the US, took over as assistant entitled: "Connecting Quarks with the director for mathematical and physical Cosmos: Eleven Science Questions for the sciences at the US National Science New Century". This report contributed to the Foundation (NSF). This $1 billion directorate current US administration's science planning supports research in mathematics, physics, agenda. Turner, who will serve at the NSF for chemistry, materials and astronomy, as well a two-year term, replaces Robert Eisenstein, as multidisciplinary and educational pro who was recently appointed as president of grammes. Turner recently chaired the US the Santa Fe Institute in New Mexico National Research Council's Committee on (see CERN Courier June 2003 p29). Institute of Advanced Study announces its next director Peter Goddard is to become the new director what was to become string theory. Goddard of the Institute for Advanced Study, is currently master of St John's College, Princeton, from 1 January 2004. Goddard, a Cambridge, UK, and is professor of mathematical physicist, is well known for his theoretical physics at the University of work in string theory and conformal field Cambridge, where he was instrumental in theory, for which he received the ICTP's helping to establish the Isaac Newton Dirac prize in 1997, together with David Institute for Mathematical Sciences. Olive. This work dates back to 1970-1972, Photograph courtesy of the Institute for when he held a position as a visiting scientist Advanced Study, Princeton. -
Rotating Convection-Driven Dynamos at Low Ekman Number
PHYSICAL REVIEW E 66, 056308 ͑2002͒ Rotating convection-driven dynamos at low Ekman number Jon Rotvig* and Chris A. Jones School of Mathematical Sciences, University of Exeter, Exeter EX4 4QE, England ͑Received 10 October 2001; revised manuscript received 18 July 2002; published 22 November 2002͒ We present a fully 3D self-consistent convection-driven dynamo model with reference to the geodynamo. A relatively low Ekman number regime is reached, with the aim of investigating the dynamical behavior at low viscosity. This regime is computationally very demanding, which has prompted us to adopt a plane layer model with an inclined rotation vector, and to make use of efficiently parallelized code. No hyperdiffusion is used, all diffusive operators are in the classical form. Our model has infinite Prandtl number, a Rayleigh number that scales as EϪ1/3 (E being the Ekman number͒, and a constant Roberts number. The optimized model allows us to study dynamos with Ekman numbers in the range ͓10Ϫ5,10Ϫ4͔. In this regime we find strong-field dynamos where the induced magnetic fields satisfy Taylor’s constraint to good accuracy. The solutions are characterized by ͑i͒ a MAC balance within the bulk, i.e., Coriolis, pressure, Lorentz, and buoyancy forces are of comparable magnitude, while viscous forces are only significant in thin boundary layers, ͑ii͒ the Elsasser number is O(10), ͑iii͒ the strong magnetic fields cannot prevent small-scale structures from becoming dominant over the large- scale components, ͑iv͒ the Taylor-Proudman effect is detectable, ͑v͒ the Taylorization decreases as the Ekman number is lowered, and ͑vi͒ the ageostrophic velocity component makes up 80% of the flow. -
The 60Th Annual DFD Meeting
FALL 2007 Division of Fluid Dynamics NewsletterDFD News A Division of the American Physical Society DFD ANNUAL ELECTION the 5th DFD meeting in 1952, is a popular tourist destination, and known for it’s mountains and Please vote online in the APS DFD election natural beauty. Salt Lake was the host of the website and vote for one of two candidates 2002 winter Olympics and is a 45 minute drive (Juan Lasheras or Robert Behringer for DFD from seven different ski areas, the closest being Vice Chair and two of four candidates for only 25 minutes away. Mid November usually DFD Executive Committee Members-at-Large marks the beginning of the ski season and (Anette Hosoi, Manoochehr Koochesfahani, attendees may wish to extend their stay for early Laurette Tuckerman or Daniel Lathrop). The season skiing on the “greatest snow on earth!” Vice Chair becomes the Chair-Elect the next Conference Website: year and then the DFD Chair the following http://dfd2007.eng.utah.edu year. The Members-at-Large serve for three year terms. You can easily access the election Hotel Reservations website (with a unique address for each current The main conference Hotel is the Salt Lake City DFD member) with the link that was sent to Downtown Marriott, directly across the street you via email on or about September 24, 2007 from the main entrance to the convention center. from the Division ([email protected]). Short Rooms are also reserved at a special conference biographical sketches of the candidates and rate at the Salt Lake Plaza Inn, also across their statements are included on the website. -
Einstein's Equations for Spin 2 Mass 0 from Noether's Converse Hilbertian
Einstein’s Equations for Spin 2 Mass 0 from Noether’s Converse Hilbertian Assertion October 4, 2016 J. Brian Pitts Faculty of Philosophy, University of Cambridge [email protected] forthcoming in Studies in History and Philosophy of Modern Physics Abstract An overlap between the general relativist and particle physicist views of Einstein gravity is uncovered. Noether’s 1918 paper developed Hilbert’s and Klein’s reflections on the conservation laws. Energy-momentum is just a term proportional to the field equations and a “curl” term with identically zero divergence. Noether proved a converse “Hilbertian assertion”: such “improper” conservation laws imply a generally covariant action. Later and independently, particle physicists derived the nonlinear Einstein equations as- suming the absence of negative-energy degrees of freedom (“ghosts”) for stability, along with universal coupling: all energy-momentum including gravity’s serves as a source for gravity. Those assumptions (all but) imply (for 0 graviton mass) that the energy-momentum is only a term proportional to the field equations and a symmetric curl, which implies the coalescence of the flat background geometry and the gravitational potential into an effective curved geometry. The flat metric, though useful in Rosenfeld’s stress-energy definition, disappears from the field equations. Thus the particle physics derivation uses a reinvented Noetherian converse Hilbertian assertion in Rosenfeld-tinged form. The Rosenfeld stress-energy is identically the canonical stress-energy plus a Belinfante curl and terms proportional to the field equations, so the flat metric is only a convenient mathematical trick without ontological commitment. Neither generalized relativity of motion, nor the identity of gravity and inertia, nor substantive general covariance is assumed. -
Scottish Fluid Mechanics Meeting Wednesday 30 Th May 2012
25 th Scottish Fluid Mechanics Meeting Wednesday 30 th May 2012 Book of Abstracts Hosted by School of Engineering and Physical Sciences & School of the Built Environment Sponsored by Dantec Dynamics Ltd. 25 th Scottish Fluid Mechanics Meeting, Heriot-Watt University, 30 th May 2012 Programme of Event: 09:00 – 09:30 Coffee and registration* 09:30 – 09:45 Welcome (Wolf-Gerrit Früh)** 09:45 – 11:00 Session 1 (5 papers) (Chair: Wolf-Gerrit Früh)** 11:00 – 11:30 Coffee break & Posters*** 11:30 – 12:45 Session 2 (5 papers) (Chair: Stephen Wilson) 12:45 – 13:45 Lunch & Posters 13:45 – 15:00 Session 3 (5 papers) (Chair: Yakun Guo) 15:00 – 15:30 Coffee break & Posters 15:30 – 17:00 Session 4 (6 papers) (Chair: Peter Davies) 17:00 – 17:10 Closing remarks (Wolf-Gerrit Früh) 17:10 – 18:00 Drinks reception * Coffee and registration will be outside Lecture Theatre 3, Hugh Nisbet Building. ** Welcome and all sessions will be held in Lecture Theatre 3, Hugh Nisbet Building. *** All other refreshments (morning and afternoon coffee breaks, lunch and the drinks reception) and posters will be held in NS1.37 (the Nasmyth Common room and Crush Area), James Nasmyth Building. 25 th Scottish Fluid Mechanics Meeting, Heriot-Watt University, 30 th May 2012 Programme of Oral Presentations (* denotes presenting author) Session 1 (09:40 – 11:00): 09:45 – 10:00 Flow control for VATT by fixed and oscillating flap Qing Xiao, Wendi Liu* & Atilla Incecik, University of Strathclyde 10:00 – 10:15 Shear stress on the surface of a mono-filament woven fabric Yuan Li* & Jonathan -
Lecture 3/4: Dynamics of the Earth's Core
Lecture 3/4: Dynamics of the Earth’s core Celine´ Guervilly School of Mathematics, Statistics and Physics, Newcastle University, UK Navier-Stokes equation @u 1 + u · ru + 2Ω × u = - rP + νr2u + F @t ρ r · u = 0 F is a forcing term (e.g. buoyancy force, Lorentz force). Ω = Ωez with Ω the rotation rate. ρ is the density, ν the viscosity. Like in the oceans and atmosphere, the rotation is very important for the dynamics of the Earth’s core. Golf Stream in the Atlantic Ocean (NASA) Taking the curl, @r2u = -2Ω · r! @t Differentiating wrt time, @2r2u @! = -2Ω · r @t2 @t we obtain the inertial wave equation @2r2u = -4(Ω · r)2u @t2 We seek solutions in the modal form u = Refuˆ ei(k·x-!t)g, where uˆ is the (complex) amplitude, k is the (real) wavevector and ! is the (possibly complex) frequency. Inertial waves We linearise the invisid NS equation about a background state of uniform rotation, i.e. ub = 0. The equation for the vorticity, ! = r × u, is @! = 2Ω · ru @t Differentiating wrt time, @2r2u @! = -2Ω · r @t2 @t we obtain the inertial wave equation @2r2u = -4(Ω · r)2u @t2 We seek solutions in the modal form u = Refuˆ ei(k·x-!t)g, where uˆ is the (complex) amplitude, k is the (real) wavevector and ! is the (possibly complex) frequency. Inertial waves We linearise the invisid NS equation about a background state of uniform rotation, i.e. ub = 0. The equation for the vorticity, ! = r × u, is @! = 2Ω · ru @t Taking the curl, @r2u = -2Ω · r! @t we obtain the inertial wave equation @2r2u = -4(Ω · r)2u @t2 We seek solutions in the modal form u = Refuˆ ei(k·x-!t)g, where uˆ is the (complex) amplitude, k is the (real) wavevector and ! is the (possibly complex) frequency.