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A Scaling Technique for the Design Of
A SCALING TECHNIQUE FOR THE DESIGN OF IDEALIZED ELECTROMAGNETIC LENSES Tj:lesis by Carl E. Baum Capt . , USAF In Partial Fulfillment of the Requi rements For the Degree of Doctor of Philosophy California Institute of Technology Pasadena, California 1969 (Submitte d August 22 , 1968) -ii- ACKNOWLEDGEMENT We would like to thank Professor C. H. Papas for his guidance and encouragement and Mrs. R. Stratton for typing the text. -iii- ABSTRACT A technique is developed for the design of lenses for transi tioning TEM waves between conical and/or cylindrical transmission lines, ideally with no reflection or distortion of the waves. These lenses utilize isotropic but inhomogeneous media and are based on a soluti on of Maxwell's equations instead of just geometrical optics. The technique employs the expression of the constitutive parameters, £ and µ , plus Maxwell's equations, in a general orthogonal curvilinear coordinate system in tensor form, giving what we term as formal quantities. Solving the problem for certain types of formal constitutive parameters, these are transformed to give £ and µ as functions of position. Several examples of such l enses are considered in detail. -iv- TABLE OF CONTENTS I. Introduction l II. Formal Vectors and Operators 5 III. Formal Electromagnetic Quantities lO IV. Restriction of Constitutive Parameters to Scalars l4 V. General Case with Field Components in All Three 16 Coordinate Directions VI . Three- Dimensional TEM Waves 19 VII. Three-Dimensional TEM Lenses 29 A. Modified Spherical Coordinates 29 B. Mo dif i ed Bispherical Coordinates 33 c. Modified Toroidal Coordinates 47 D. Modified Cylindrical Coordinates 57 VIII. -
Computer Facilitated Generalized Coordinate Transformations of Partial Differential Equations with Engineering Applications
Computer Facilitated Generalized Coordinate Transformations of Partial Differential Equations With Engineering Applications A. ELKAMEL,1 F.H. BELLAMINE,1,2 V.R. SUBRAMANIAN3 1Department of Chemical Engineering, University of Waterloo, 200 University Avenue West, Waterloo, Ontario, Canada N2L 3G1 2National Institute of Applied Science and Technology in Tunis, Centre Urbain Nord, B.P. No. 676, 1080 Tunis Cedex, Tunisia 3Department of Chemical Engineering, Tennessee Technological University, Cookeville, Tennessee 38505 Received 16 February 2008; accepted 2 December 2008 ABSTRACT: Partial differential equations (PDEs) play an important role in describing many physical, industrial, and biological processes. Their solutions could be considerably facilitated by using appropriate coordinate transformations. There are many coordinate systems besides the well-known Cartesian, polar, and spherical coordinates. In this article, we illustrate how to make such transformations using Maple. Such a use has the advantage of easing the manipulation and derivation of analytical expressions. We illustrate this by considering a number of engineering problems governed by PDEs in different coordinate systems such as the bipolar, elliptic cylindrical, and prolate spheroidal. In our opinion, the use of Maple or similar computer algebraic systems (e.g. Mathematica, Reduce, etc.) will help researchers and students use uncommon transformations more frequently at the very least for situations where the transformations provide smarter and easier solutions. ß2009 Wiley Periodicals, Inc. Comput Appl Eng Educ 19: 365À376, 2011; View this article online at wileyonlinelibrary.com; DOI 10.1002/cae.20318 Keywords: partial differential equations; symbolic computation; Maple; coordinate transformations INTRODUCTION usual Cartesian, polar, and spherical coordinates. For example, Figure 1 shows two identical pipes imbedded in a concrete slab. -
In George Warner Swenson, Jr. B.S., Michigan College of Mining And
SOLUTION OF LAPLACE'S EQUATION in INVERTED COORDINATE SYSTEMS by George Warner Swenson, Jr. B.S., Michigan College of Mining and Technology (1944) Submitted in Partial Fulfillment of the Requirements for the Degree of MASTER OF SCIENCE at the MASSACHUSETTS INSTITUTE OF TECHNOLOGY 1948 Signature of Author ..0 Q .........0 .. .. Department of Electrical Engineering Certified by .. S....uper. ... .... .. Thesis Supervisor Chairman, Departmental Committee on Graduate Students ACKNOWLEDGMENT The author wishes to express his sincerest apprecia- tion to Professor Parry Moon, of the Department of Electrical Engineering, who suggested the general topic of this thesis. His lectures in electrostatic field theory have provided the essential background for the investigation and his interest in the problem has prompted many helpful suggestions. In addition, the author is indebted to Dr. R. M. Redheffer, of the Department of Mathematics, without whose patient interpretation of his Doctorate thesis and frequent assistance in overcoming mathematical difficulties the present work could hardly have been accomplished. 2982i19 ii CONTENTS ABSTRACT.............................................. iv I ORIENTATION .............. ,............ *,*.*..*** 1 II THE GEOMETRICAL PROPERTIES OF INVERTED SYSTEMS.... 7 A. The Process of Inversion ..................... 7 B. Practical Methods of Inversion................ 8 (1' Graphical Method ... ................... 8 2 Optical Method ......... ................. 10 C. The Inverted Coordinate Systems .............. 19 1) Inverse Rectangular Coordinates ......... 19 2) Inverse Spheroidal Coordinates .......... 19 3) Inverse Parabolic CooDrdinates ........... 21 III LAPLACE'S EQUATION IN INVERTED COORDINATE SYSTEMS. 30 A. The Form of the Equation ..................... 30 B. Separation of Variables ...................... 30 C. Tabulation of the Separated Equations for the Inverted Coordinate Systems *..........*......35 IV TBE APPLICATION OF THE INVERTED COORDINATE SYSTEMS TO BOUNDARY VALUE PROBLEMS ...................... -
The Charged Bowl in Toroidal Coordinates.Pdf
The Charged Bowl in Toroidal Coordinates Phil Lucht Rimrock Digital Technology, Salt Lake City, Utah 84103 last update: January 5, 2016 Maple code is available upon request. Comments and errata are welcome. The material in this document is copyrighted by the author. The graphics look ratty in Windows Adobe PDF viewers when not scaled up, but look just fine in this excellent freeware viewer: http://www.tracker-software.com/pdf-xchange-products-comparison-chart . Overview and Summary.........................................................................................................................3 1. Bipolar and toroidal coordinates .......................................................................................................7 1.1 Bipolar coordinates .........................................................................................................................7 1.2 Toroidal coordinates .......................................................................................................................9 2. The charged bowl potential in toroidal coordinates ......................................................................16 2.1 Level curves, the charged ellipsoid problem and a dashed hope ..................................................16 2.2 Cartesian, spherical, toroidal and ellipsoidal atomic forms ..........................................................17 2.3 Smythian forms and one for the bowl...........................................................................................18 2.4 Solution -
Symmetry and Separation of Variables for the Helmholtz and Laplace Equations
C. P. Boyer, E. G. Kalnins, and W. Miller, Jr. Nagoya Math. J. Vol. 60 (1976), 35-80 SYMMETRY AND SEPARATION OF VARIABLES FOR THE HELMHOLTZ AND LAPLACE EQUATIONS C. P. BOYER, E. G. KALNINS, AND W. MILLER, JR. Introduction. This paper is one of a series relating the symmetry groups of the principal linear partial differential equations of mathematical physics and the coordinate systems in which variables separate for these equations. In particular, we mention [1] and paper [2] which is a survey of and introduction to the series. Here we apply group-theoretic methods to study the separable coordinate systems for the Helmholtz equation. 2 (4* + ω )Ψ(x) = 0 , x = (xlf x29 x3) , 4* = 3ii + d22 + d33 , ω > 0 , and the Laplace equation (0.2) ΔzW{x) = 0 . It is well-known that (0.1) separates in eleven coordinate systems, see [3], Chapter 5, and references contained therein. Moreover, in [4] it is shown that these systems correspond to commuting pairs of second order symmetric operators in the enveloping algebra of <?(3), the sym- metry algebra of (0.1). However, we show here for the first time how one can systematically make use of the representation theory of the Euclidean symmetry group £7(3) of the Helmholtz equation to derive identities relating the different separable solutions. As we will point out, some of these identities are new. It is also known that there are 17 types of cyclidic coordinate systems which permit i?-separation of variables in the Laplace equation and these appear to be the only such separable systems for (0.2), [5]. -
C:\Book\Booktex\C1s3.DVI
65 §1.3 SPECIAL TENSORS Knowing how tensors are defined and recognizing a tensor when it pops up in front of you are two different things. Some quantities, which are tensors, frequently arise in applied problems and you should learn to recognize these special tensors when they occur. In this section some important tensor quantities are defined. We also consider how these special tensors can in turn be used to define other tensors. Metric Tensor Define yi,i=1,...,N as independent coordinates in an N dimensional orthogonal Cartesian coordinate system. The distance squared between two points yi and yi + dyi,i=1,...,N is defined by the expression ds2 = dymdym =(dy1)2 +(dy2)2 + ···+(dyN )2. (1.3.1) Assume that the coordinates yi are related to a set of independent generalized coordinates xi,i=1,...,N by a set of transformation equations yi = yi(x1,x2,...,xN ),i=1,...,N. (1.3.2) To emphasize that each yi depends upon the x coordinates we sometimes use the notation yi = yi(x), for i =1,...,N. The differential of each coordinate can be written as ∂ym dym = dxj ,m=1,...,N, (1.3.3) ∂xj and consequently in the x-generalized coordinates the distance squared, found from the equation (1.3.1), becomes a quadratic form. Substituting equation (1.3.3) into equation (1.3.1) we find ∂ym ∂ym ds2 = dxidxj = g dxidxj (1.3.4) ∂xi ∂xj ij where ∂ym ∂ym g = ,i,j=1,...,N (1.3.5) ij ∂xi ∂xj i are called the metrices of the space defined by the coordinates x ,i=1,...,N. -
Orthogonal Curvilinear Coordinate Systems A
Orthogonal Curvilinear Coordinate Systems A A-l Curvilinear Coordinates The location of a point in three-dimensional space (with respect to some origin) is usually specified by giving its three cartesian coordinates (x, y, z) or, what is equivalent, by specifying the position vector R of the point. It is often more convenient to describe the position of the point by another set of coordinates more appropriate to the problem at hand, common examples being spherical and cylindrical coordinates. ,These are but special cases of curvilinear coordinate systems, whose general properties we propose to ex amine in detail. Suppose that ql> q2> and qa are independent functions of position such that ql = ql (x, y, z), q2 = q2(X, y, z), qa = qa(x, y, z) (A-1.l) or, in terms of the position vector, qk = qk(R) (k = 1,2,3) In regions where the Jacobian determinant, oql oql oql ox oy oz o(ql> q2' qa) = Oq2 Oq2 ~ (A-1.2) o(x,y, z) ox oy oz oqa oqa oqa ox oy oz 474 Orthogonol Curvilinear Coordinate Systems 475 is different from zero this system of equations can be solved simultaneously for x, y, and z, giving y = y(qj, q2, q3), or R = R(qj, q2' q3) A vanishing of the Jacobian implies that qj, q2' and q3 are not independent functions but, rather, are connected by a functional relationship of the form f(qj, q2, q3) = O. In accordance with (A-I.3), the specification of numerical values for qj, q2, and q3 leads to a corresponding set of numerical values for x, y, z; that is, it locates a point (x, y, z) in space. -
Curvilinear Coordinates
Curvilinear Coordinates Cylindrical Coordinates A 3-dimensional coordinate transformation is a mapping of the form T (u; v; w) = x (u; v; w) ; y (u; v; w) ; z (u; v; w) h i Correspondingly, a 3-dimensional coordinate transformation T maps a solid in the uvw-coordinate system to a solid T ( ) in the xyz-coordinate system (and similarly, T maps curves in uvw to curves in xyz; surfaces in uvw to surfaces in xyz; and so on). In this section, we introduce and explore two of the more important 3-dimensional coordinate transformations. To begin with, the cylindrical coordinates of a point P are Cartesian co- ordinates in which the x and y coordinates have been transformed into polar coordinates (and the z-coordinate is left as is). 1 Not surprisingly, to convert to cylindrical coordinates, we simply apply x = r cos () and y = r sin () to the x and y coordinates. That is, the cylindrical coordinate transformation is T (r; ; z) = r cos () ; r sin () ; z h i Cylindrical coordinates get their name from the fact that the surface ”r = constant”is a cylinder. For example, the cylinder r (; z) = cos () ; sin () ; z h i is obtained by setting r = 1 in the cylindrical coordinate transformation. Likewise, parameterizations of many other level surfaces can be derived from the cylindrical coordinate transformation. In particular, if points in the xy-plane are in polar coordinates, then z = f (r; ) is a surface in 3 dimensional space, and the parameterization of that surface is r (r; ) = cos () ; sin () ; f (r; ) h i More generally, U (r; ; z) = k de…nes a level surface in which the xy components are represented in polar coordinates. -
14.2.2 Covariant and Contravariant Coordinates
14. Vector Algebra and Vector Analysis 2016-07-07 $Version 10.0 for Mac OS X x86 (64-bit) (December 4, 2014) Mathematica 9: The commands for vector analysis are contained in the kernel in contrast to earlier versions. Mathematica 7 or 8: The package must be loaded by the command << "VectorAnalysis`" . Some of the commands differ from those given in version 9, so in these lecture notes. In particular, the arguments of the operators do not contain the list of the independent variables as arguments. Ph. Boylard: A Guide to Standard Mathematica Packages. Mathematica Technical Report (1991). E. Martin: Mathematica 3.0 Standard Add-On Packages. Cambridge University Press. pp.74-82. 14.1 Rectangular, Cylindrical and Spherical Coordinates Rectangular (as well as cylindrical and spherical) coordinates have been treated at the end of Chap.3. Knowledge of these subjects is pressuposed in this chapter. 14.2 Curvilinear Orthogonal Coordinates 14.2.1 Literature Murray R. Spiegel, Schaum's Mathemtical Handbook of Formulas and Tables, McGraw-Hill, New York 1968, pp.116-130 Philip M. Morse, Herman Feshbach: Methods of Theoretical Physics, McGraw-Hill, New York, 1953. (MF), 656ff. George B. Arken, Mathematical Methods for Pysicists, 3 rd ed., Academic Press, New York, 1985. B. Schnizer, Analytical methods in applied theoretrical physics. Lecture notes (in German). Chaps. 6 and 7. http://itp.tugraz.at/~schnizer/AnalyticalMethods/ P. Moon, D.E. Spencer, Field Theory Handbook. 2 nd ed., Springer, 1988. (MS) G. Wendt, Statische Felder und Stationäre Ströme. Hb. d. Physik XVI Springer, 1958, S.1 ff. W.R. Smith, Static and Dynamic Electricity, McGraw-Hill, 1950 14.2.2 Covariant and contravariant coordinates A general non-singular transformation from Cartesian coordinates x1, x2, x3 to more general curvilinear coordinates u1, u2, u3 is given by: xi = xi (u1, u2, u3), uk = uk (x1, x2, x3); i, k = 1, 2, 3. -
On the Numerical Solution of the Cylindrical Poisson Equation for Isolated Self -Gravitating Systems
Louisiana State University LSU Digital Commons LSU Historical Dissertations and Theses Graduate School 1999 On the Numerical Solution of the Cylindrical Poisson Equation for Isolated Self -Gravitating Systems. Howard Saul Cohl Louisiana State University and Agricultural & Mechanical College Follow this and additional works at: https://digitalcommons.lsu.edu/gradschool_disstheses Recommended Citation Cohl, Howard Saul, "On the Numerical Solution of the Cylindrical Poisson Equation for Isolated Self -Gravitating Systems." (1999). LSU Historical Dissertations and Theses. 6983. https://digitalcommons.lsu.edu/gradschool_disstheses/6983 This Dissertation is brought to you for free and open access by the Graduate School at LSU Digital Commons. It has been accepted for inclusion in LSU Historical Dissertations and Theses by an authorized administrator of LSU Digital Commons. For more information, please contact [email protected]. INFORMATION TO USERS This manuscript has been reproduced from the microfilm master. UMI films the text directly from the original or copy submitted. Thus, some thesis and dissertation copies are in typewriter face, while others may be from any type of computer printer. The quality of this reproduction is dependent upon the quality of the copy subm itted. Broken or indistinct print, colored or poor quality illustrations and photographs, print bleedthrough, substandard margins, and improper alignment can adversely affect reproduction. In the unlikely event that the author did not send UMI a complete manuscript and there are missing pages, these will be noted. Also, if unauthorized copyright material had to be removed, a note will indicate the deletion. Oversize materials (e.g., maps, drawings, charts) are reproduced by sectioning the original, beginning at the upper left-hand comer and continuing from left to right in equal sections with small overlaps. -
Bipolar Coordinates and the Two-Cylinder Capacitor Phil Lucht Rimrock Digital Technology, Salt Lake City, Utah 84103 Last Update: June 15, 2015
Bipolar Coordinates and the Two-Cylinder Capacitor Phil Lucht Rimrock Digital Technology, Salt Lake City, Utah 84103 last update: June 15, 2015 Maple code is available upon request. Comments and errata are welcome. The material in this document is copyrighted by the author. The graphics look ratty in Windows Adobe PDF viewers when not scaled up, but look just fine in this excellent freeware viewer: http://www.tracker-software.com/pdf-xchange-products-comparison-chart . The table of contents has live links. Most PDF viewers provide these links as bookmarks on the left. Overview and Summary.........................................................................................................................3 1. Reminder of regular polar coordinates.............................................................................................5 2. Bipolar Coordinates............................................................................................................................6 3. The metric tensor, scale factors, distance, and the Jacobian ........................................................12 4. The inverse transformation..............................................................................................................13 5. Connection to Toroidal and Bispherical Coordinates ...................................................................15 6. Interpretation of the coordinates ξ and u .......................................................................................16 7. The circle angle θ ..............................................................................................................................18 -
Developments in Determining the Gravitational Potential Using Toroidal Functions ∗
Astron. Nachr. 321 (2000) 5/6, 363–372 Developments in determining the gravitational potential using toroidal functions ∗ H.S. Cohl, J.E. Tohline and A.R.P. Rau, Baton Rouge, Louisiana, U.S.A. Department of Physics andAstronomy, Louisiana State University H.M. Srivastava, Victoria, British Columbia, Canada Department of Mathematics andStatistics, University of Victoria Received2000 October 24; accepted2000 November 15 Cohl & Tohline (1999) have shown how the integration/summation expression for the Green’s function in cylindrical coor- dinates can be written as an azimuthal Fourier series expansion, with toroidal functions as expansion coefficients. In this paper, we show how this compact representation can be extended to other rotationally invariant coordinate systems which are known to admit separable solutions for Laplace’s equation. Key words: stars: formation – stars: evolution – galaxies: formation – galaxies: evolution – separation of Laplace’s equation – spheroidal coordinates – parabolic coordinates – toroidal coordinates 1. Introduction The Newtonian gravitational and Coulomb potentials, Φ(x,t), due to a mass or charge distribution ρ(x,t), are important throughout our physical world. In an astrophysical context (cf., §2.1 in Binney & Tremaine 1987), the Newtonian potential is determined by solving the appropriate boundary-value problem that is given by the three-dimensional Poisson equation, ∇2Φ(x)=4πGρ(x), (1) where ∇2 is the Laplacian, and G 6.6742 × 10−8 cm3 g−1 sec−2 is the gravitational constant (see Gundlach & Merkowitz 2000). Exterior to an isolated mass distribution, physically correct boundary conditions may be imposed on Poisson’s equation through the following integral formulation of the potential problem, ρ − (x ) d3x.