User:Tohline/Appendix/Ramblings/ToroidalCoordinates

Toroidal Configurations and Related Coordinate Systems

Preamble

As I have studied the structure and analyzed the stability of (both self-gravitating and non-self-gravitating) toroidal configurations over the years, I have often wondered whether it might be useful to examine such systems mathematically using a toroidal — or at least a toroidal-like — coordinate system. Is it possible, for example, to build an equilibrium torus for which the density distribution is one-dimensional as viewed from a well-chosen toroidal-like system of coordinates?

I should begin by clarifying my terminology. In volume II (p. 666) of their treatise on Methods of Theoretical Physics, Morse & Feshbach (1953; hereafter MF53) define an orthogonal toroidal coordinate system in which the Laplacian is separable.¹ (See details, below.) It is only this system that I will refer to as the toroidal coordinate system; all other functions that trace out toroidal surfaces but that don't conform precisely to Morse & Feshbach's coordinate system will be referred to as toroidal-like.

I became particularly interested in this idea while working with Howard Cohl (when he was an LSU graduate student). Howie's dissertation research uncovered a Compact Cylindrical Greens Function technique for evaluating Newtonian potentials of rotationally flattened, axisymmetric potentials.^2,3 The technique involves a multipole expansion in terms of half-integer-degree Legendre functions of the <math>2^\mathrm{nd}</math> kind where, if I recall correctly, the argument of this special function (or its inverse) seemed to resemble the radial coordinate of Morse & Feshbach's orthogonal toroidal coordinate system.

Toroidal Coordinates

Presentation by MF53

The orthogonal toroidal coordinate system <math>(\xi_1,\xi_2,\xi_3=\cos\varphi)</math> discussed by MF53 has the following properties:

<math> \frac{x}{a} </math>	<math> = </math>	<math> \biggl[ \frac{(\xi_1^2 - 1)^{1/2}}{\xi_1 - \xi_2} \biggr]\cos\varphi </math>
<math> \frac{y}{a} </math>	<math> = </math>	<math> \biggl[ \frac{(\xi_1^2 - 1)^{1/2}}{\xi_1 - \xi_2} \biggr]\sin\varphi </math>
<math> \frac{z}{a} </math>	<math> = </math>	<math> \frac{(1-\xi_2^2)^{1/2}}{\xi_1 - \xi_2} </math>
<math> \frac{\varpi}{a} \equiv \biggl[ \biggl(\frac{x}{a}\biggr)^2 + \biggl(\frac{y}{a}\biggr)^2 \biggr]^{1/2} </math>	<math> = </math>	<math> \frac{(\xi_1^2 - 1)^{1/2}}{\xi_1 - \xi_2} </math>
<math> \frac{r}{a} \equiv \biggl[ \biggl(\frac{x}{a}\biggr)^2 + \biggl(\frac{y}{a}\biggr)^2 + \biggl(\frac{z}{a}\biggr)^2\biggr]^{1/2} </math>	<math> = </math>	<math> \biggl[ \frac{\xi_1 + \xi_2}{\xi_1 - \xi_2} \biggr]^{1/2} </math>

According to MF53, the associated scale factors of this orthogonal coordinate system are:

<math> \frac{h_1}{a} </math>	<math> = </math>	<math> \frac{1}{(\xi_1 - \xi_2)(\xi_1^2 - 1)^{1/2}} </math>
<math> \frac{h_2}{a} </math>	<math> = </math>	<math> \frac{1}{(\xi_1 - \xi_2)(1-\xi_2^2)^{1/2}} </math>
<math> \frac{h_3}{a} </math>	<math> = </math>	<math> \biggl[ \frac{(\xi_1^2 - 1)^{1/2}}{\xi_1 - \xi_2} \biggr]\frac{1}{\sin\varphi} </math>

Tohline's Ramblings

My inversion of these coordinate definitions has lead to the following expressions:

<math> \xi_1 </math>	<math> = </math>	<math> \frac{r(r^2 + 1)} {[\chi^2(r^2-1)^2 + \zeta^2(r^2+1)^2]^{1/2}} </math>
<math> \xi_2 </math>	<math> = </math>	<math> \frac{r(r^2 - 1)}{[\chi^2(r^2-1)^2 + \zeta^2(r^2+1)^2]^{1/2}} </math>

where,

<math> \chi \equiv \frac{\varpi}{a} ~~~;~~~\zeta\equiv\frac{z}{a} ~~~\mathrm{and} ~~~ r=(\chi^2 + \zeta^2)^{1/2} . </math>

Apparently the allowed ranges of the two meridional-plane coordinates are:

<math> +1 \leq \xi_1 \leq \infty ~~~\mathrm{and} ~~~ -1 \leq \xi_2 \leq +1 . </math>

Example Toroidal Surfaces

In the accompanying figure, we've outlined three different a <math>\xi_1 = \mathrm{constant}</math> meridional contours for the MF53 toroidal coordinate system. The illustrated values are,

<math> \xi_1 </math>	=	1.1		(blue);
<math> \xi_1 </math>	=	1.2		(red);
<math> \xi_1 </math>	=	1.5		(gold).

The inner and outer edges of the toroidal surface in the equatorial plane should be determined by setting <math>\xi_2 = -1</math> (inner) and <math>\xi_2 = +1</math> (outer). Hence,

<math> \chi_\mathrm{inner} </math>	=	<math> \frac{(\xi_1^2 - 1)^{1/2}}{\xi_1 +1} = \biggl[\frac{(\xi_1 - 1)}{(\xi_1 + 1)} \biggr]^{1/2} </math>
<math> \chi_\mathrm{outer} </math>	=	<math> \frac{(\xi_1^2 - 1)^{1/2}}{\xi_1 - 1} = \biggl[\frac{(\xi_1 + 1)}{(\xi_1 - 1)} \biggr]^{1/2} </math>

The equatorial-plane location of the "center" of each torus is,

<math> \chi_0 = \frac{1}{2} (\chi_\mathrm{outer} + \chi_\mathrm{inner}) = \frac{\xi_1}{(\xi_1^2 - 1)^{1/2}} , </math>

and the so-called distortion parameter,

<math> \delta \equiv \frac{\chi_\mathrm{outer}-\chi_\mathrm{inner}}{\chi_0}= \frac{2}{\xi_1} . </math>

Properties of <math>\xi_1 = \mathrm{constant}</math> Toroidal Surfaces
Curve in Figure	<math>\xi_1</math>	<math>\chi_\mathrm{inner}</math>	<math>\chi_\mathrm{outer}</math>	<math>\chi_0</math>	<math>\delta</math>
Blue	1.1	0.218	4.583	2.400	1.818
Red	1.2	0.302	3.317	1.809	1.667
Gold	1.5	0.447	2.236	1.342	1.333

What function <math>\zeta(\varpi)</math> coincides with these <math>\xi_1 = \mathrm{constant}</math> surfaces? (To be answered!)

References

1. Morse, P.M. & Feshmach, H. 1953, Methods of Theoretical Physics — Volumes I and II
2. Cohl, H.S. & Tohline, J.E. 1999, ApJ, 527, 86-101
3. Cohl, H.S., Rau, A.R.P., Tohline, J.E., Browne, D.A., Cazes, J.E. & Barnes, E.I. 2001, Phys. Rev. A, 64, 052509

 

© 2014 - 2021 by Joel E. Tohline |   H_Book Home   |   YouTube   | Appendices: | Equations | Variables | References | Ramblings | Images | myphys.lsu | ADS | Recommended citation:   Tohline, Joel E. (2021), The Structure, Stability, & Dynamics of Self-Gravitating Fluids, a (MediaWiki-based) Vistrails.org publication, https://www.vistrails.org/index.php/User:Tohline/citation