Appendix/Ramblings/T6CoordinatesPt2: Difference between revisions

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====Relationship To T3 Coordinates====
If we set, <math>~q = 1</math>, but continue to assume that <math>~p > 1</math>, we expect to see a representation that resembles our previously discussed, [[User:Tohline/Appendix/Ramblings/T3Integrals#Integrals_of_Motion_in_T3_Coordinates|T3 Coordinates]].  Note, for example, that the new "radial" coordinate is,
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\lambda_1^2</math>
  </td>
  <td align="center">
<math>~\rightarrow</math>
  </td>
  <td align="left">
<math>~
(\varpi^2 + p^2z^2) \, ,
</math>
  </td>
<td align="center">&nbsp; &nbsp; &nbsp; and, &nbsp; &nbsp; &nbsp; </td>
  <td align="right">
<math>~\mathcal{D}^2</math>
  </td>
  <td align="center">
<math>~\rightarrow</math>
  </td>
  <td align="left">
<math>~
\biggl[
(1 + \tan^2\varphi)(p^2 + \tan^2\theta)
\biggr]  \, .
</math>
  </td>
</tr>
</table>
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\Rightarrow ~~~ \frac{p^2z^2}{\lambda_1^2}</math>
  </td>
  <td align="center">
<math>~\rightarrow</math>
  </td>
  <td align="left">
<math>~\frac{ p^2}{(p^2 + \tan^2\theta)} = \frac{ 1}{(1 + p^{-2} \tan^2\theta)}\, ,</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>~\frac{\varpi^2}{\lambda_1^2} = \frac{x^2}{\lambda_1^2} + \frac{y^2}{\lambda_1^2}</math>
  </td>
  <td align="center">
<math>~\rightarrow</math>
  </td>
  <td align="left">
<math>~1 -  p^2 \biggl( \frac{z^2}{\lambda_1^2}\biggr)
=
\biggl[1 -  \frac{ 1}{(1 + p^{-2}\tan^2\theta)} \biggr] \, .</math>
  </td>
</tr>
</table>
We also see that,
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\frac{\varpi^2}{p^2z^2}</math>
  </td>
  <td align="center">
<math>~\rightarrow</math>
  </td>
  <td align="left">
<math>~
(1 + p^{-2}\tan^2\theta)\biggl[1 -  \frac{ 1}{(1 + p^{-2}\tan^2\theta)} \biggr]
=
p^{-2}\tan^2\theta \, .
</math>
  </td>
</tr>
</table>


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Revision as of 16:34, 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.

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