Appendix/Ramblings/T6CoordinatesPt2: Difference between revisions

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</tr>
</tr>
</table>
</table>
===Speculation6===
====Determine &lambda;<sub>2</sub>====
This is very similar to the [[#Speculation2|above, Speculation2]].
Try,
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\lambda_2</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
\frac{x y^{1/q^2}}{ z^{2/p^2}} \, ,
</math>
  </td>
</tr>
</table>
in which case,
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\frac{\partial \lambda_2}{\partial x}</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
\frac{\lambda_2}{x} \, ,
</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>~\frac{\partial \lambda_2}{\partial y}</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
\frac{x}{z^{2/p^2}} \biggl(\frac{1}{q^2}\biggr) y^{1/q^2 - 1}
=
\frac{\lambda_2}{q^2 y}
\, ,
</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>~\frac{\partial \lambda_2}{\partial z}</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
-\frac{2\lambda_2}{p^2 z}
\, .
</math>
  </td>
</tr>
</table>
The associated scale factor is, then,
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~h_2</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~\biggl[
\biggl( \frac{\partial \lambda_2}{\partial x} \biggr)^2
+
\biggl( \frac{\partial \lambda_2}{\partial y} \biggr)^2
+
\biggl( \frac{\partial \lambda_2}{\partial z} \biggr)^2
\biggr]^{-1 / 2}
</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~\biggl[
\biggl( \frac{ \lambda_2}{x} \biggr)^2
+
\biggl( \frac{\lambda_2}{q^2y} \biggr)^2
+
\biggl( - \frac{2\lambda_2}{p^2z} \biggr)^2
\biggr]^{-1 / 2}
</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~\frac{1}{\lambda_2}\biggl[
\frac{ 1}{x^2}
+
\frac{1}{q^4y^2}
+
\frac{4}{p^4z^2}
\biggr]^{-1 / 2}
</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~\frac{1}{\lambda_2}\biggl[
\frac{ (q^4 y^2 p^4 z^2 + x^2 p^4 z^2 + 4x^2q^4y^2}{x^2 q^4 y^2 p^4 z^2}
\biggr]^{-1 / 2}
</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
\frac{1}{\lambda_2}\biggl[
\frac{x q^2 y p^2 z}{ \mathcal{D}}
\biggr] \, .
</math>
  </td>
</tr>
</table>
where,
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\mathcal{D}</math>
  </td>
  <td align="center">
<math>~\equiv</math>
  </td>
  <td align="left">
<math>~(q^4 y^2 p^4 z^2 + x^2 p^4 z^2 + 4x^2q^4y^2)^{1 / 2} \, .</math>
  </td>
</tr>
</table>
The associated unit vector is, then,
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\hat{e}_2</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
\hat{\imath} h_2 \biggl( \frac{\partial \lambda_2}{\partial x} \biggr)
+ \hat{\jmath} h_2 \biggl( \frac{\partial \lambda_2}{\partial y} \biggr)
+ \hat{k} h_2 \biggl( \frac{\partial \lambda_2}{\partial z} \biggr)
</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~ \frac{x q^2 y p^2 z}{\mathcal{D}} \biggl\{
\hat{\imath} \biggl( \frac{1}{x} \biggr)
+ \hat{\jmath}  \biggl( \frac{1}{q^2 y} \biggr)
+ \hat{k} \biggl( -\frac{2}{p^2 z} \biggr)
\biggr\} \ .
</math>
  </td>
</tr>
</table>
Recalling that the unit vector associated with the "first" coordinate is,
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\hat{e}_1 </math>
  </td>
  <td align="center">
<math>~\equiv</math>
  </td>
  <td align="left">
<math>~
\hat\imath (x \ell_{3D}) + \hat\jmath (q^2y \ell_{3D}) + \hat{k} (p^2 z \ell_{3D}) \, ,
</math>
  </td>
</tr>
</table>
where,
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\ell_{3D}</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~(x^2 + q^4y^2 + p^4 z^2 )^{- 1 / 2} \, ,</math>
  </td>
</tr>
</table>
let's check to see whether the "second" unit vector is orthogonal to the "first."
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\hat{e}_1 \cdot \hat{e}_2</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
\frac{(x q^2 y p^2 z) \ell_{3D}}{\mathcal{D}} \biggl[
1 + 1 - 2
\biggr] = 0 \, .
</math>
  </td>
</tr>
</table>
<font color="red">'''Hooray!'''</font>


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Revision as of 16:42, 23 July 2021

Concentric Ellipsoidal (T6) Coordinates (Part 2)

Orthogonal Coordinates

Speculation5

Spherical Coordinates

rcosθ

=

z,

rsinθ

=

(x2+y2)1/2,

tanφ

=

yx.

Use λ1 Instead of r

Here, as above, we define,

λ12

x2+q2y2+p2z2

Using this expression to eliminate "x" (in favor of λ1) in each of the three spherical-coordinate definitions, we obtain,

r2x2+y2+z2

=

λ12y2(q21)z2(p21);

tan2θx2+y2z2

=

1z2[λ12y2(q21)p2z2];

1tan2φx2y2

=

λ12p2z2y2q2.

After a bit of additional algebraic manipulation, we find that,

z2λ12

=

(1+tan2φ)𝒟2,

y2λ12

=

[𝒟2tan2φp2tan2φ(1+tan2φ)(1+q2tan2φ)𝒟2],

x2λ12

=

1q2(y2λ12)p2(z2λ12),

where,

𝒟2

[(1+q2tan2φ)(p2+tan2θ)p2(q21)tan2φ].

As a check, let's set q2=p2=1, which should reduce to the normal spherical coordinate system.

λ12

r2,

      and,      

𝒟2

[(1+tan2φ)(1+tan2θ)].

z2λ12

11+tan2θ=cos2θ=z2r2;

y2λ12

[(1+tan2φ)(1+tan2θ)tan2φtan2φ(1+tan2φ)(1+tan2φ)(1+tan2φ)(1+tan2θ)]

 

=

tan2φ(1+tan2φ)[tan2θ(1+tan2θ)]=sin2θsin2φ=y2r2;

x2λ12

1(y2λ12)(z2λ12),

 

1sin2θsin2φcos2θ=sin2θsin2φ+sin2θ=sin2θcos2φ=x2r2.

Relationship To T3 Coordinates

If we set, q=1, but continue to assume that p>1, we expect to see a representation that resembles our previously discussed, T3 Coordinates. Note, for example, that the new "radial" coordinate is,

λ12

(ϖ2+p2z2),

      and,      

𝒟2

[(1+tan2φ)(p2+tan2θ)].

p2z2λ12

p2(p2+tan2θ)=1(1+p2tan2θ),

ϖ2λ12=x2λ12+y2λ12

1p2(z2λ12)=[11(1+p2tan2θ)].

We also see that,

ϖ2p2z2

(1+p2tan2θ)[11(1+p2tan2θ)]=p2tan2θ.

Again Consider Full 3D Ellipsoid

Let's try to replace everywhere, [ϖ/(pz)]2=p2tan2θ with λ2. This gives,

𝒟2p2

[(1+q2tan2φ)λ2(q21)tan2φ].

which means that,

p2z2λ12

=

(1+tan2φ)[(1+q2tan2φ)λ2(q21)tan2φ]

 

=

(1+tan2φ)/tan2φ[q2λ2(1+q2tan2φ)/(q2tan2φ)(q21)]=1/sin2φ[q2λ2Q2(q21)],

q2y2λ12

=

q2tan2φ(1+q2tan2φ)q2tan2φ(1+tan2φ)(1+q2tan2φ)[(1+q2tan2φ)λ2(q21)tan2φ]

 

=

q2tan2φ(1+q2tan2φ){1(1+tan2φ)[(1+q2tan2φ)λ2(q21)tan2φ]}

 

=

q2tan2φ(1+q2tan2φ){1(1+tan2φ)/tan2φ[q2λ2(1+q2tan2φ)/(q2tan2φ)(q21)]}

 

=

1Q2{11/sin2φ[q2λ2Q2(q21)]}=1Q2[][[]1sin2φ],

x2λ12

=

1q2tan2φ(1+q2tan2φ){1(1+tan2φ)[(1+q2tan2φ)λ2(q21)tan2φ]}

 

 

(1+tan2φ)[(1+q2tan2φ)λ2(q21)tan2φ]

 

=

1q2tan2φ(1+q2tan2φ){(1+tan2φ)[(1+q2tan2φ)λ2(q21)tan2φ]}

 

=

11Q2{1/sin2φ[q2λ2Q2(q21)]}=1Q2[]{Q2[][]Q2sin2φ},

x2+q2y2λ12

=

1[1+q2tan2φ(1+q2tan2φ)]{(1+tan2φ)[(1+q2tan2φ)λ2(q21)tan2φ]}.

Now, notice that,

q2y2Q2λ12

=

11[]sin2φ,

and,

x2λ12+1Q2

=

11[]sin2φ.

Hence,

x2λ12+1Q2

=

q2y2Q2λ12

0

=

Q4(q2y2λ12)Q2(x2λ12)1

 

=

Q4Q2(x2q2y2)(λ12q2y2),

where,

Q2

1+q2tan2φq2tan2φ.

Solving the quadratic equation, we have,

Q2

=

12{(x2q2y2)±[(x2q2y2)2+4(λ12q2y2)]1/2}

 

=

(x22q2y2){1±[1+4(λ12q2y2x4)]1/2}.

Tentative Summary

λ1

(x2+q2y2+p2z2)1/2,

λ2

(x2+y2)1/2pz,

λ3=Q2

(x22q2y2){1±[1+4(λ12q2y2x4)]1/2}.

Partial Derivatives & Scale Factors

First Coordinate

λ1x

=

xλ1,

λ1y

=

q2yλ1,

λ1z

=

p2zλ1.

h12

=

(λ1x)2+(λ1y)2+(λ1z)2

=

(xλ1)2+(q2yλ1)2+(p2zλ1)2.

h1

=

λ13D,

where,

3D(x2+q4y2+p4z2)1/2.

As a result, the associated unit vector is,

e^1

=

ı^h1(λ1x)+ȷ^h1(λ1y)+k^h1(λ1z)

 

=

ı^x3D+ȷ^q2y3D+k^p2z3D.

Notice that,

e^1e^1

=

(x2+q4y2+p4z2)3D2=1.


Second Coordinate (1st Try)

λ2x

=

1pz[x(x2+y2)1/2],

λ2y

=

1pz[y(x2+y2)1/2],

λ2z

=

(x2+y2)1/2pz2.

h22

=

(λ2x)2+(λ2y)2+(λ2z)2

 

=

{1pz[x(x2+y2)1/2]}2+{1pz[y(x2+y2)1/2]}2+{(x2+y2)1/2pz2}2

 

=

{[x2(x2+y2)p2z2]}+{[y2(x2+y2)p2z2]}+{(x2+y2)p2z4}

 

=

1p2z2+(x2+y2)p2z4=(x2+y2+z2)p2z4

h2

=

pz2r

As a result, the associated unit vector is,

e^2

=

ı^h2(λ2x)+ȷ^h2(λ2y)+k^h2(λ2z)

 

=

ı^[xzr(x2+y2)1/2]+ȷ^[yzr(x2+y2)1/2]k^[(x2+y2)1/2r].

Notice that,

e^2e^2

=

[x2z2r2(x2+y2)]+[y2z2r2(x2+y2)]+[(x2+y2)r2]=1.

Let's check to see if this "second" unit vector is orthogonal to the "first."

e^1e^2

=

x3D[xzr(x2+y2)1/2]+q2y3D[yzr(x2+y2)1/2]p2z3D[(x2+y2)1/2r]

 

=

3D{[x2zr(x2+y2)1/2]+[q2y2zr(x2+y2)1/2][p2z(x2+y2)1/2r]}

 

=

z3Dr(x2+y2)1/2{[x2]+[q2y2][p2(x2+y2)]}

 

0 .


Second Coordinate (2nd Try)

Let's try,

λ2

=

[(x2+q2y2+𝔣p2z2)1/2pz],

λ2x

=

xpz(x2+q2y2+𝔣p2z2)1/2=xp2z2λ2,

λ2y

=

q2ypz(x2+q2y2+𝔣p2z2)1/2=q2yp2z2λ2,

λ2z

=

𝔣p2zpz(x2+q2y2+𝔣p2z2)1/2(x2+q2y2+𝔣p2z2)1/2pz2=1p2z2λ2(𝔣p2z)λ2z=1p2z2λ2(𝔣p2zp2zλ22).

Hence,

h22

=

(λ2x)2+(λ2y)2+(λ2z)2

 

=

[xp2z2λ2]2+[q2yp2z2λ2]2+[𝔣zλ2λ2z]2

 

=

[x2+q4y2p4z4λ22]+[1zλ2(𝔣λ22)]2

 

=

1p4z4λ22[x2+q4y2+p4z2(𝔣λ22)2]

h2

=

p2z2λ2[x2+q4y2+p4z2(𝔣λ22)2]1/2.

So, the associated unit vector is,

e^2

=

ı^h2(λ2x)+ȷ^h2(λ2y)+k^h2(λ2z)

 

=

ı^{x[x2+q4y2+p4z2(𝔣λ22)2]1/2}+ȷ^{q2y[x2+q4y2+p4z2(𝔣λ22)2]1/2}+k^{p2z(𝔣λ22)[x2+q4y2+p4z2(𝔣λ22)2]1/2}.

Checking orthogonality …

e^1e^2

=

x3D{x[x2+q4y2+p4z2(𝔣λ22)2]1/2}+q2y3D{q2y[x2+q4y2+p4z2(𝔣λ22)2]1/2}+p2z3D{p2z(𝔣λ22)[x2+q4y2+p4z2(𝔣λ22)2]1/2}

 

=

3D[x2+q4y2+p4z2(𝔣λ22)2]1/2{x2+q4y2+p4z2(𝔣λ22)}.

 

=

3D[x2+q4y2+p4z2(𝔣λ22)2]1/2{x2+q4y2+p4z2(𝔣λ22)}.

If 𝔣=0, we have …

p2z(𝔣λ22)

       

[p2zλ22]𝔣=0=p2z[(x2+q2y2+𝔣0p2z2)1/2pz]2=(x2+q2y2)z,

which, in turn, means …

[x2+q4y2+p4z2(𝔣0λ22)2]1/2

=

[x2+q4y2+p4z2λ24]1/2

 

=

{x2+q4y2+p4z2[(x2+q2y2+𝔣0p2z2)1/2pz]4}1/2

 

=

{x2+q4y2+[(x2+q2y2)2z2]}1/2

 

=

(x2+q4y2)1/2[1+(x2+q2y2)z2]1/2

 

=

(x2+q4y2)1/2z[z2+(x2+q2y2)]1/2,

and,

e^1e^2

=

3D[x2+q4y2+p4z2(𝔣λ22)2]1/2{x2+q4y2+p4z2(𝔣λ22)}.

Speculation6

Determine λ2

This is very similar to the above, Speculation2. Try,

λ2

=

xy1/q2z2/p2,

in which case,

λ2x

=

λ2x,

λ2y

=

xz2/p2(1q2)y1/q21=λ2q2y,

λ2z

=

2λ2p2z.

The associated scale factor is, then,

h2

=

[(λ2x)2+(λ2y)2+(λ2z)2]1/2

 

=

[(λ2x)2+(λ2q2y)2+(2λ2p2z)2]1/2

 

=

1λ2[1x2+1q4y2+4p4z2]1/2

 

=

1λ2[(q4y2p4z2+x2p4z2+4x2q4y2x2q4y2p4z2]1/2

 

=

1λ2[xq2yp2z𝒟].

where,

𝒟

(q4y2p4z2+x2p4z2+4x2q4y2)1/2.

The associated unit vector is, then,

e^2

=

ı^h2(λ2x)+ȷ^h2(λ2y)+k^h2(λ2z)

 

=

xq2yp2z𝒟{ı^(1x)+ȷ^(1q2y)+k^(2p2z)} .

Recalling that the unit vector associated with the "first" coordinate is,

e^1

ı^(x3D)+ȷ^(q2y3D)+k^(p2z3D),

where,

3D

=

(x2+q4y2+p4z2)1/2,

let's check to see whether the "second" unit vector is orthogonal to the "first."

e^1e^2

=

(xq2yp2z)3D𝒟[1+12]=0.

Hooray!


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