Appendix/Ramblings/EllipticCylinderCoordinates

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Elliptic Cylinder Coordinates[edit]

Background[edit]

Building on our general introduction to Direction Cosines in the context of orthogonal curvilinear coordinate systems, here we detail the properties of Elliptic Cylinder Coordinates. First, we present this coordinate system in the manner described by [MF53]; second, we provide an alternate presentation, obtained from Wikipedia; then, third, we investigate whether or not a related coordinate system based on concentric (rather than confocal) elliptic surfaces can be satisfactorily described.

It is useful to keep in mind various properties of a set of confocal ellipses in which the location of the pair of foci is fixed at, (x,y)=(±c,0), and the semi-major axis, a, is the parameter. The relevant prescriptive relation is,

1

=

x2a2+y2a2−c2      for,   a>c.

The semi-minor axis length, b, and the eccentricity, e, of the ellipse are, respectively,

b

=

(a2−c2)1/2,

      and,      

e≡[1−b2a2]1/2

=

ca.

The length, ℓ1, of the chord that connects one focus to a point, P(x,y), on the ellipse is,

ℓ1

=

a+(ca)x;

and the length, ℓ2, of the chord that connects the second focus to that same point on the ellipse is,

ℓ2

=

a−(ca)x.

It is easy to see that, for any point on the ellipse, the sum of these two lengths is, 2a. It is worth noting as well that the associated y coordinate of the relevant point can be obtained from the relation,

ℓ12

=

y2+(c+x)2

⇒(ay)2

=

(aℓ1)2−(ac+ax)2

 

=

(a2+cx)2−(ac+ax)2

 

=

(a4+2a2cx+c2x2)−(a2c2+2a2cx+a2x2)

 

=

(a4+c2x2)−(a2c2+a2x2)

 

=

(a2−x2)(a2−c2)

⇒y

=

±1a[(a2−x2)(a2−c2)]1/2.

MF53[edit]

Definition[edit]

From MF53's Table of Separable Coordinates in Three Dimensions (see their Chapter 5, beginning on p. 655), we find the following description of Elliptic Cylinder Coordinates (p. 657).

Elliptic Cylindrical Coordinates
(MF53 Primary Definition)

x

=

ξ1ξ2

y

=

[(ξ12−d2)(1−ξ22)]1/2

z

=

ξ3

Alternate Definition

Making the substitutions, ξ3→z, ξ2→cos⁡ν, and ξ1→dcosh⁡μ, we equally well obtain:

x

=

dcosh⁡μ⋅cos⁡ν

y

=

dsinh⁡μ⋅sin⁡ν

z

=

z


Notice that,

x2d2cosh2μ+y2d2sinh2μ

=

cos2ν+sin2ν=1.

Hence, as is pointed out in a related Wikipedia discussion, "… this shows that curves of constant μ form ellipses." For a given choice of μ — say, μ0 — let's see how the shape of the resulting ellipse relates to the standard ellipses described in our background discussion, above. The semi-major axis of the selected ellipse must be,

a=dcosh⁡μ0.

And its eccentricity must be obtainable from the relation,

a2−c2=a2(1−e2)

=

d2sinh2μ0

 

=

a2tanh2μ0=a2(1−1cosh2μ0)

⇒e2

=

1cosh2μ0.

We note, as well, that the x-coordinate location of the focus of the selected ellipse is,

c2=a2e2

=

d2.

This emphasizes a key property of the MF53 Elliptic Cylindrical Coordinate system, viz., the family of ellipses that result from selecting various values of μ0 is a family of confocal ellipses.

Scale Factors[edit]

Primary[edit]

Appreciating that,

∂y∂ξ1

=

+[(ξ12−d2)(1−ξ22)]−1/2ξ1(1−ξ22),       and that,

∂y∂ξ2

=

−[(ξ12−d2)(1−ξ22)]−1/2ξ2(ξ12−d2),

we find that the respective scale factors are given by the expressions,

h12

=

(∂x∂ξ1)2+(∂y∂ξ1)2+(∂z∂ξ1)2

 

=

ξ22+[(ξ12−d2)(1−ξ22)]−1ξ12(1−ξ22)2

 

=

(ξ12−d2)−1[(ξ12−d2)ξ22+ξ12(1−ξ22)]

 

=

[ξ12−d2ξ22ξ12−d2];

h22

=

(∂x∂ξ2)2+(∂y∂ξ2)2+(∂z∂ξ2)2

 

=

ξ12+[(ξ12−d2)(1−ξ22)]−1ξ22(ξ12−d2)2

 

=

(1−ξ22)−1[ξ12(1−ξ22)+ξ22(ξ12−d2)]

 

=

[ξ12−d2ξ221−ξ22];

h32

=

(∂x∂ξ3)2+(∂y∂ξ3)2+(∂z∂ξ3)2

 

=

1.

These match the scale-factor expressions found in MF53.

Alternatively[edit]

Alternatively, the Wikipedia discussion gives,

hμ=hν

=

dsinh2μ+sin2ν

∇2Φ

=

1d2(sinh2μ+sin2ν)[∂2Φ∂μ2+∂2Φ∂ν2]+∂2Φ∂z2.

Inverting Coordinate Mapping[edit]

Inverting the original coordinate mappings, we find,

y2

=

(ξ12−a2)[1−(xξ1)2]

⇒0

=

(ξ12−a2)(ξ12−x2)−ξ12y2

 

=

(ξ12−a2)ξ12−(ξ12−a2)x2−ξ12y2

 

=

ξ14−ξ12(a2+x2+y2)+a2x2

⇒ξ12

=

12{(a2+x2+y2)±[(a2+x2+y2)2−4a2x2]1/2}

Only the superior — that is, only the positive — sign will ensure positive values of ξ12, so in summary we have,

Coordinate Transformation

ξ1

=

12{[(a2+x2+y2)2−4a2x2]1/2+(a2+x2+y2)}1/2;

ξ2

=

xξ1;

ξ3

=

z.

Alternative Wikipedia Definition[edit]

This same MF53 coordinate system — with different variable notation — is referred to in a Wikipedia discussion as an "alternative and geometrically intuitive set of elliptic coordinates." The relevant mapping is, (dσ,τ,z)Wikipedia=(ξ1,ξ2,ξ3)MF53. The identified mapping to Cartesian coordinates is,

x

=

(dσ)τ

=

ξ1ξ2;

y

=

d[(σ2−1)(1−τ2)]1/2

=

[(ξ12−d2)(1−ξ22)]1/2;

z

=

z

=

ξ3.

According to the Wikipedia discussion, the three scale factors are,

hσ2

=

d2[σ2−τ2σ2−1];

     

hτ2

=

d2[σ2−τ21−τ2];

      and,      

hz2

=

1.

Interestingly, the Wikipedia discussion also includes the following expression for the Laplacian in this elliptic cylindrical coordinate system:

∇2Φ

=

1d2(σ2−τ2)[σ2−1∂∂σ(σ2−1∂Φ∂σ)+1−τ2∂∂τ(1−τ2∂Φ∂τ)]+∂2Φ∂z2.

T5 Coordinates[edit]

Introduction[edit]

As has been made clear in our above review of the Elliptic Cylinder Coordinate system (ξ1,ξ2,ξ3)=(dcosh⁡μ,cos⁡ν,z), individual curves within a family of confocal ellipses are identified by one's choice of the "radial" coordinate parameter, μ, or, alternatively, ξ1. Specifically, while the two foci of every ellipse are positioned along the x-axis at the same points — namely, (x,y)=(±d,0) — the length of the semi-major axis is given by, a=ξ1=dcosh⁡μ.

In a separate chapter we have introduced a different orthogonal curvilinear coordinate system that we refer to as, "T3 Coordinates." In this coordinate system, (λ1,λ2,λ3), individual surfaces within a family of concentric spheroids are identified by one's choice of a different "radial" coordinate parameter, λ1. Here we will adopt essentially this same set of orthogonal coordinates, using λ1 and λ2 to describe a family of concentric ellipses that is independent of the vertical-coordinate. We will refer to it as the …

T5 Coordinate System

λ1

≡

xcosh⁡ζ

         

=

(x2+q2y2)1/2

λ2

≡

x(sinh⁡ζ)1/(1−q2)

         

=

(xq2qy)1/(q2−1)

λ3

=

z

         

=

z

where,

ζ

≡

sinh−1(qyx)

and, 0<q<∞ is the (fixed) parameter used to specify the eccentricity, e=[(q2−1)1/2/q], of every λ1= constant curve within the family of concentric ellipses.


Checking these expressions, we have,

λ2≡x(sinh⁡ζ)1/(1−q2)

=

x(qyx)1/(1−q2)=x(xqy)1/(q2−1)=(xq2qy)1/(q2−1).

And,

λ1≡xcosh⁡ζ

=

x[1+sinh2ζ]1/2=x[1+(qyx)2]1/2=(x2+q2y2)1/2.

Comparing this last expression with the above background description of ellipses, we see that λ1= constant — for example, λ0 — is synonymous with an ellipse having …

  • A semi-major axis of length, a=λ0;
  • An eccentricity, e≡(1−b2/a2)1/2=[(q2−1)/q2]1/2;
  • A pair of foci whose coordinate locations along the major axis are, (x,y)=(±c,0), where, c=ae.

Invert Coordinate Mapping[edit]

Solving for x(λ1,λ2), we find …

λ1

=

(x2+q2y2)1/2

⇒y2

=

1q2[λ12−x2].

And,

λ2

=

(xq2qy)1/(q2−1)

⇒y2

=

1q2[x2q2λ22(1−q2)].

Hence,

x2q2λ22(1−q2)+x2−λ12

=

0.

Alternatively, solving for y(λ1,λ2), we find …

λ1

=

(x2+q2y2)1/2

⇒x2

=

λ12−q2y2.

And,

λ2

=

(xq2qy)1/(q2−1)

⇒x

=

(qy)1/q2λ2(q2−1)/q2.

Hence,

(qy)2/q2λ22(q2−1)/q2−λ12+q2y2

=

0.

 

Summary of Inverted Relations

λ22(xλ2)2q2+x2−λ12

=

0;

λ22(qyλ2)2/q2+q2y2−λ12

=

0.

Example:     q2=2

0

=

x4λ2−2+x2−λ12

←   Quadratic Eq. in x2

⇒x2

=

λ222{[1+4λ12λ22]1/2−1}=λ222(Λ−1);

 

0

=

2y2+(21/2λ2)y−λ12

←   Quadratic Eq. in y

⇒y

=

14{−21/2λ2±[2λ22+8λ12]1/2}

 

 

=

λ223/2{[1+4λ12λ22]1/2−1}=λ223/2(Λ−1).

 

where,

Λ≡[1+4λ12λ22]1/2.

Note …

yx2

=

λ223/2⋅2λ22=12λ2;

and,

4y2x2

=

[1+4λ12λ22]1/2−1

⇒1ℓ2≡(x2+4y2)

=

x2[1+4λ12λ22]1/2=x2Λ=λ222Λ(Λ−1)      or,

1ℓ2≡(x2+4y2)

=

2λ2y[1+4λ12λ22]1/2=2λ2yΛ=λ222⋅Λ(Λ−1).

Note as well that, ℓ−2=2λ12Λ/(Λ+1).

Example:     q2=32

0

=

λ22(xλ2)3+x2−λ12

       ←   Cubic Eq. in x

0

=

λ22(3y22λ22)2/3+32y2−λ12

       ←   Cubic Eq. in y2/3

Example:     q2=3

0

=

λ22(xλ2)6+x2−λ12

       ←   Cubic Eq. in x2

0

=

λ22(3y2λ22)1/3+3y2−λ12

       ←   Cubic Eq. in y2/3

Example:     q2=4

0

=

λ22(xλ2)8+x2−λ12

       ←   Quartic Eq. in x2

0

=

λ22(2yλ2)1/2+4y2−λ12

       ←   Quartic Eq. in y1/2

 

Relevant Partial Derivatives[edit]

Before moving forward, we need to evaluate a number of relevant partial derivatives.

∂λ1∂x

=

∂∂x[x2+q2y2]1/2=12[x2+q2y2]−1/22x=xλ1.

∂λ1∂y

=

∂∂y[x2+q2y2]1/2=12[x2+q2y2]−1/22q2y=q2yλ1.

∂λ2∂x

=

∂∂x[xq2/(q2−1)(qy)−1/(q2−1)]=[q2q2−1]λ2x.

∂λ2∂y

=

∂∂y[xq2/(q2−1)(qy)−1/(q2−1)]=−[1q2−1]λ2y.

We may also need the set of complementary partial derivatives. Even though we are unable to explicitly invert the coordinate mappings, once we have in hand expressions for the three scale factors (see immediately below), we can determine expressions for the set of complementary partial derivatives via the generic relation,

∂xi∂λn

=

hn2⋅∂λn∂xi.


Example:     q2=2

y

=

λ223/2{Λ−1},

       

x2

=

λ222{Λ−1},       where,      

Λ

≡

[1+4λ12λ22]1/2.

Noting that,

∂Λ∂λ1

=

1Λλ1[4λ12λ22]

      and,      

∂Λ∂λ2

=

−1Λλ2[4λ12λ22],

we have,

∂y∂λ1

=

λ223/2⋅∂Λ∂λ1=2λ1λ2[1+4λ12λ22]−1/2,

∂y∂λ2

=

123/2[Λ−1]+λ223/2⋅∂Λ∂λ2=(Λ−1)23/2−2λ12Λλ22.

 

=

Λ(Λ−1)−4λ12/λ2223/2Λ=Λ2−Λ−4λ12/λ2223/2Λ

 

=

(1−Λ)23/2Λ.


Let's compare by drawing from the expressions for ℓ2, above, and for hn2 derived below.

[h12⋅∂λ1∂y]q2=2

=

[λ12ℓ2(q2yλ1)]q2=2=[2λ1ℓ2y]q2=2

 

=

2λ1{12λ2Λ}=2λ1λ2Λ.

Yes! This, indeed matches the just-derived expression for ∂y/∂λ1. And we also have,

[h22⋅∂λ2∂y]q2=2

=

{−[1q2−1]λ2y[(q2−1)xyℓλ2]2}q2=2=−[(q2−1)x2yℓ2λ2]q2=2

 

=

(1−Λ)23/2Λ.

Yes, again!

Scale Factors, Direction Cosines & Unit Vectors[edit]

From our accompanying generic discussion of direction cosines, we can write,

h12

=

[(∂λ1∂x)2+(∂λ1∂y)2+(∂λ1∂z)2]−1

 

=

[(xλ1)2+(q2yλ1)2]−1=λ12[x2+q4y2]−1

 

=

λ12ℓ2;

h22

=

{(∂λ2∂x)2+(∂λ2∂y)2+(∂λ2∂z)2}−1

 

=

{[q2q2−1]2(λ2x)2+[1q2−1]2(λ2y)2}−1

 

=

[(q2−1)xyℓλ2]2;

h32

=

{(∂λ3∂x)2+(∂λ3∂y)2+(∂λ3∂z)2}−1=1;

where,

ℓ≡(x2+q4y2)−1/2.


Direction Cosines for T5 Coordinates
γni=hn(∂λn∂xi)

n i=x,y,z
1  
xℓ
 
q2yℓ 0
2

 
q2yℓ


−xℓ 0
3  
0
 
0 1

The unit vectors are,

e^n

=

ı^γn1+ȷ^γn2+k^γn3,

that is,

e^1

=

ı^(xℓ)+ȷ^(q2yℓ),

e^2

=

ı^(q2yℓ)−ȷ^(xℓ),

e^3

=

k^.

Notice that,

e^1⋅e2^

=

q2xyℓ2−q2xyℓ2=0,

and,

e^1⋅e1^

=

x2ℓ2+q4y2ℓ2=ℓ2(x2+q4y2)=1.

These are both desired orthogonality conditions. Alternatively,

ı^

=

e^1γ11+e^2γ21+e^3γ31=e^1(xℓ)+e^2(q2yℓ);

ȷ^

=

e^1γ12+e^2γ22+e^3γ32=e^1(q2yℓ)−e^2(xℓ);

k^

=

e^1γ13+e^2γ23+e^3γ33=e^3.

Spatial Operators[edit]

Summary Reminder

h12

=

λ12ℓ2;

     

h22

=

[(q2−1)xyℓλ2]2;

      and,      

h32

=

1;

In T5 Coordinates, a couple of relevant operators are:

∇F

=

e^1[1h1∂F∂λ1]+e^2[1h2∂F∂λ2]+e^3[1h3∂F∂λ3]

 

=

e^1(1λ1ℓ)∂F∂λ1+e^2[λ2(q2−1)xyℓ]∂F∂λ2+e^3∂F∂λ3.


∇2F

=

1h1h2h3[∂∂λ1(h2h3h1⋅∂F∂λ1)+∂∂λ2(h3h1h2⋅∂F∂λ2)+∂∂λ3(h1h2h3⋅∂F∂λ3)]

 

=

λ2λ1(q2−1)xyℓ2{∂∂λ1[(q2−1)xyλ1λ2⋅∂F∂λ1]+∂∂λ2[λ1λ2(q2−1)xy⋅∂F∂λ2]+∂∂λ3[λ1(q2−1)xyℓ2λ2⋅∂F∂λ3]}

And if F is a function only of λ1, then,

∇2F

=

λ2λ1(q2−1)xyℓ2{∂∂λ1[(q2−1)xyλ1λ2⋅∂F∂λ1]}

 

=

λ2λ1(q2−1)xyℓ2{[(q2−1)xyλ1λ2][∂2F∂λ12]+∂F∂λ1⋅∂∂λ1[(q2−1)xyλ1λ2]}

 

=

[1λ12ℓ2][∂2F∂λ12]+[1λ1xyℓ2]∂F∂λ1⋅∂∂λ1[xyλ1].

In order to complete this evaluation, we need a couple of "complementary partial derivatives." Referencing the relation provided above, we find,

∂∂λ1[xyλ1]

=

xy[∂∂λ1(λ1−1)]+yλ1[∂x∂λ1]+xλ1[∂y∂λ1]

 

=

−xyλ12+yλ1[h12∂λ1∂x]+xλ1[h12∂λ1∂y]

 

=

−xyλ12+h12λ1[xyλ1+q2xyλ1]

 

=

xyλ12[λ12ℓ2(1+q2)−1].

Hence,

∇2F

=

[1λ12ℓ2][∂2F∂λ12]+xyλ12[λ12ℓ2(1+q2)−1][1λ1xyℓ2]∂F∂λ1

 

=

[1λ12ℓ2][∂2F∂λ12]+[λ12ℓ2(1+q2)−1][1λ13ℓ2]∂F∂λ1

 

=

[1λ12ℓ2][∂2F∂λ12]−[1λ13ℓ2]∂F∂λ1+[(1+q2)λ1]∂F∂λ1.

Example (q2 = 2) Poisson Equation[edit]

Setup[edit]

Let's see if we can solve the,

Poisson Equation User:Tohline/Math/EQ Poisson01

obtaining an analytic expression for the gravitational potential in the case where, independent of the coordinate, z,

ρ=ρcσ

=

ρc[1−(x2a2+y2b2)]

 

=

ρc[1−1a2(x2+q2y2)].

Given that the density distribution is independent of z, we expect the potential to be independent of z as well. So, in terms of T5-Coordinates, the Poisson equation may be written as,

λ2λ1(q2−1)xyℓ2{∂∂λ1[(q2−1)xyλ1λ2⋅∂Φ∂λ1]+∂∂λ2[λ1λ2(q2−1)xy⋅∂Φ∂λ2]}

=

4πGρc[1−λ12a2]

If we specifically consider the case where q2=a2/b2=2, this can be rewritten as,

4πGρc[1−λ12a2]

=

λ2λ1(q2−1)xyℓ2{∂∂λ1[(q2−1)xyλ1λ2⋅∂Φ∂λ1]+∂∂λ2[λ1λ2(q2−1)xy⋅∂Φ∂λ2]}

 

=

λ2λ1⋅(Λ−1)−3/222λ22⋅λ222(Λ−1)Λ{∂∂λ1[(Λ−1)2⋅∂Φ∂λ1]+∂∂λ2[2(Λ−1)⋅∂Φ∂λ2]}

 

=

4Λ(Λ−1){∂∂λ1[(Λ−1)2⋅∂Φ∂λ1]+∂∂λ2[2(Λ−1)⋅∂Φ∂λ2]}

where we have used the following expressions derived above:

x2y2

=

(Λ−1)[λ2222(Λ−1)]2,

1ℓ2

=

λ222(Λ−1)Λ=2λ12Λ(Λ+1),

Λ

≡

[1+4λ12λ22]1/2⇒12(Λ2−1)1/2=λ1λ2.

xyλ1λ2

=

122[λ2λ1(Λ−1)3/2]=12(Λ−1).

Now,

∂(Λ−1)∂λ1

=

12Λ(8λ1λ22)=4λ1Λ(λ12λ22)=(Λ2−1)λ1Λ;

∂(Λ−1)−1∂λ2

=

−1(Λ−1)2[12Λ](−8λ12λ23)=4(Λ−1)2[1λ2Λ](λ12λ22)=Λ+1(Λ−1)[1λ2Λ].

Hence,

4πGρc[1−λ12a2]

=

4Λ(Λ−1){(Λ−1)2[∂2Φ∂λ12]+∂Φ∂λ1⋅∂∂λ1[(Λ−1)2]+2(Λ−1)[∂2Φ∂λ22]+∂Φ∂λ2⋅∂∂λ2[2(Λ−1)]}

 

=

4Λ(Λ−1){(Λ−1)2[∂2Φ∂λ12]+[(Λ2−1)2λ1Λ]∂Φ∂λ1+2(Λ−1)[∂2Φ∂λ22]+[2(Λ+1)(Λ−1)λ2Λ]∂Φ∂λ2}

 

=

2Λ[∂2Φ∂λ12]+[2(Λ+1)λ1]∂Φ∂λ1+8Λ(Λ−1)2[∂2Φ∂λ22]+[8(Λ+1)(Λ−1)2λ2]∂Φ∂λ2

 

=

2λ1{Λλ1[∂2Φ∂λ12]+(Λ+1)∂Φ∂λ1}+8λ2(Λ−1)2{Λλ2[∂2Φ∂λ22]+(Λ+1)∂Φ∂λ2}.

Trials[edit]

Try,

Φ

=

Aλ1α+Bλ2β

⇒∂Φ∂λ1

=

Aαλ1α−1,

      and,      

∂Φ∂λ2

=

Bβλ2β−1.

In this case we find,

4πGρc[1−λ12a2]

=

2λ1{Λλ1∂∂λ1[∂Φ∂λ1]+(Λ+1)[∂Φ∂λ1]}+8λ2(Λ−1)2{Λλ2∂∂λ2[∂Φ∂λ2]+(Λ+1)[∂Φ∂λ2]}

 

=

2Aλ1{Λλ1∂∂λ1[αλ1α−1]+(Λ+1)[αλ1α−1]}+8Bλ2(Λ−1)2{Λλ2∂∂λ2[βλ2β−1]+(Λ+1)[βλ2β−1]}

 

=

2Aαλ1{Λ(α−1)λ1α−1+(Λ+1)λ1α−1}+8Bβλ2(Λ−1)2{Λ(β−1)λ2β−1+(Λ+1)λ2β−1}

 

=

2Aαλ1α−2{Λ(α−1)+(Λ+1)}+8Bβλ2β−2(Λ−1)2{Λ(β−1)+(Λ+1)}

 

=

2Aαλ1α−2{αΛ+1}+8Bβλ2β−2(Λ−1)2{βΛ+1}.

If α=4,

8Bβλ2β−2(Λ−1)2[βΛ+1]

=

4πGρc[1−λ12a2]−8Aλ12−32Aλ12Λ

⇒8Bβλ2β−2[βΛ+1]

=

{4πGρc−32Aλ12Λ−λ12[4πGρca2+8A]}(Λ2−2Λ+1).

If, then, 8Aa2=−4πGρc,

⇒8Bβλ2β−2[βΛ+1]

=

4πGρc{1+[4λ12a2]Λ}(Λ2−2Λ+1).

But, we also know that, λ12=λ22(Λ2−1)/4, so …

8a2Bβλ2β−2[βΛ+1]

=

4πGρc{a2+λ22(Λ2−1)Λ}(Λ2−2Λ+1).


(25 October 2020) I give up … for now.

See Also[edit]


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