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| =Concentric Ellipsoidal (T8) Coordinates=
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|
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| ==Background==
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| Building on our [[User:Tohline/Appendix/Ramblings/DirectionCosines|general introduction to ''Direction Cosines'']] in the context of orthogonal curvilinear coordinate systems, and on our previous development of [[User:Tohline/Appendix/Ramblings/T3Integrals|T3]] (concentric oblate-spheroidal) and [[User:Tohline/Appendix/Ramblings/EllipticCylinderCoordinates#T5_Coordinates|T5]] (concentric elliptic) coordinate systems, here we explore the creation of a concentric ellipsoidal (T8) coordinate system. This is motivated by our [[User:Tohline/ThreeDimensionalConfigurations/Challenges#Trial_.232|desire to construct a fully analytically prescribable model of a nonuniform-density ellipsoidal configuration that is an analog to Riemann S-Type ellipsoids]].
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|
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| Note that, in a [[User:Tohline/Appendix/Ramblings/ConcentricEllipsodalCoordinates#Background|separate but closely related discussion]], we made attempts to define this coordinate system, numbering the trials up through "T7." In this "T7" effort, we were able to define a set of three, mutually orthogonal unit vectors that should work to define a fully three-dimensional, concentric ellipsoidal coordinate system. But we were unable to figure out what coordinate function, <math>~\lambda_3(x, y, z)</math>, was associated with the third unit vector. In addition, we found the <math>~\lambda_2</math> coordinate to be rather strange in that it was not oriented in a manner that resembled the classic spherical coordinate system. Here we begin by redefining the <math>~\lambda_2</math> coordinate such that its associated <math>~\hat{e}_3</math> unit vector lies parallel to the x-y plane.
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|
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| ==Realigning the Second Coordinate==
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|
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| The first coordinate remains the same as before, namely,
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| <table border="0" cellpadding="5" align="center">
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|
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| <tr>
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| <td align="right">
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| <math>~\lambda_1^2</math>
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~x^2 + q^2 y^2 + p^2 z^2 \, .</math>
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| </td>
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| </tr>
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| </table>
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| This may be rewritten as,
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| <table border="0" cellpadding="5" align="center">
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|
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| <tr>
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| <td align="right">
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| <math>~1</math>
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~\biggl( \frac{x}{a}\biggr)^2 + \biggl( \frac{y}{b}\biggr)^2 + \biggl(\frac{z}{c}\biggr)^2 \, ,</math>
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| </td>
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| </tr>
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| </table>
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| where,
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| <table border="0" cellpadding="5" align="center">
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|
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| <tr>
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| <td align="right">
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| <math>~a = \lambda_1 \, ,</math>
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| </td>
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| <td align="center"> </td>
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| <td align="center">
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| <math>~b = \frac{\lambda_1}{q} \, ,</math>
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| </td>
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| <td align="center"> </td>
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| <td align="left">
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| <math>~c = \frac{\lambda_1}{p} \, .</math>
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| </td>
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| </tr>
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| </table>
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|
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| By specifying the value of <math>~z = z_0 < c</math>, as well as the value of <math>~\lambda_1</math>, we are picking a plane that lies parallel to, but a distance <math>~z_0</math> above, the equatorial plane. The elliptical curve that defines the intersection of the <math>~\lambda_1</math>-constant surface with this plane is defined by the expression,
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| <table border="0" cellpadding="5" align="center">
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|
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| <tr>
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| <td align="right">
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| <math>~\lambda_1^2 - p^2z_0^2</math>
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~x^2 + q^2 y^2 </math>
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| </td>
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| </tr>
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|
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| <tr>
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| <td align="right">
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| <math>~\Rightarrow~~~1</math>
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~\biggl( \frac{x}{a_{2D}}\biggr)^2 + \biggl( \frac{y}{b_{2D}}\biggr)^2 \, ,</math>
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| </td>
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| </tr>
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| </table>
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| where,
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| <table border="0" cellpadding="5" align="center">
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|
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| <tr>
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| <td align="right">
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| <math>~a_{2D} = \biggl(\lambda_1^2 - p^2z_0^2 \biggr)^{1 / 2} \, ,</math>
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| </td>
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| <td align="center"> </td>
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| <td align="left">
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| <math>~b_{2D} = \frac{1}{q} \biggl(\lambda_1^2 - p^2z_0^2 \biggr)^{1 / 2} \, .</math>
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| </td>
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| </tr>
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| </table>
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|
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| At each point along this elliptic curve, the line that is tangent to the curve has a slope that can be determined by simply differentiating the equation that describes the curve, that is,
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| <table border="0" cellpadding="5" align="center">
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|
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| <tr>
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| <td align="right">
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| <math>~0</math>
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~\frac{2x dx}{a_{2D}^2} + \frac{2y dy}{b_{2D}^2}</math>
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| </td>
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| </tr>
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|
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| <tr>
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| <td align="right">
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| <math>~\Rightarrow~~~\frac{dy}{dx}</math>
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~- \frac{2x}{a_{2D}^2} \cdot \frac{b_{2D}^2}{2y} = - \frac{x}{q^2y} \, .</math>
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| </td>
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| </tr>
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|
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| <tr>
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| <td align="right">
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| <math>~\Rightarrow~~~\Delta y</math>
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~- \biggl( \frac{x}{q^2y} \biggr)\Delta x \, .</math>
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| </td>
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| </tr>
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| </table>
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|
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| The unit vector that lies tangent to any point on this elliptical curve will be described by the expression,
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| <table border="0" cellpadding="5" align="center">
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|
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| <tr>
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| <td align="right">
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| <math>~\hat{e}_2</math>
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~
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| \hat\imath~ \biggl\{ \frac{\Delta x}{[ (\Delta x)^2 + (\Delta y)^2 ]^{1 / 2}} \biggr\}
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| +
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| \hat\jmath~ \biggl\{ \frac{\Delta y}{[ (\Delta x)^2 + (\Delta y)^2 ]^{1 / 2}} \biggr\} </math>
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| </td>
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| </tr>
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|
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| <tr>
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| <td align="right">
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|
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~
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| \hat\imath~ \biggl\{ \frac{1}{[ 1 + x^2/(q^4y^2) ]^{1 / 2}} \biggr\}
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| -
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| \hat\jmath~ \biggl\{ \frac{x/(q^2y)}{[ 1 + x^2/(q^4y^2) ]^{1 / 2}} \biggr\} </math>
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| </td>
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| </tr>
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|
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| <tr>
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| <td align="right">
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|
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~
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| \hat\imath~ \biggl\{ \frac{q^2y}{[ x^2 + q^4y^2 ]^{1 / 2}} \biggr\}
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| -
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| \hat\jmath~ \biggl\{ \frac{x}{[ x^2 + q^4y^2 ]^{1 / 2}} \biggr\} \, .</math>
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| </td>
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| </tr>
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| </table>
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| As we have discovered, the coordinate that gives rise to this unit vector is,
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| <table border="0" cellpadding="5" align="center">
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|
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| <tr>
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| <td align="right">
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| <math>~\lambda_2</math>
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~\frac{x}{y^{1/q^2}} \, .</math>
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| </td>
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| </tr>
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| </table>
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|
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| Other properties that result from this definition of <math>~\lambda_2</math> are presented in the following table.
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|
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| <table border="1" cellpadding="8" align="center">
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| <tr>
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| <td align="center" colspan="9">'''Direction Cosine Components for T8 Coordinates'''</td>
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| </tr>
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| <tr>
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| <td align="center"><math>~n</math></td>
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| <td align="center"><math>~\lambda_n</math></td>
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| <td align="center"><math>~h_n</math></td>
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| <td align="center"><math>~\frac{\partial \lambda_n}{\partial x}</math></td>
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| <td align="center"><math>~\frac{\partial \lambda_n}{\partial y}</math></td>
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| <td align="center"><math>~\frac{\partial \lambda_n}{\partial z}</math></td>
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| <td align="center"><math>~\gamma_{n1}</math></td>
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| <td align="center"><math>~\gamma_{n2}</math></td>
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| <td align="center"><math>~\gamma_{n3}</math></td>
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| </tr>
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|
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| <tr>
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| <td align="center"><math>~1</math></td>
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| <td align="center"><math>~(x^2 + q^2 y^2 + p^2 z^2)^{1 / 2} </math></td>
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| <td align="center"><math>~\lambda_1 \ell_{3D}</math></td>
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| <td align="center"><math>~\frac{x}{\lambda_1}</math></td>
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| <td align="center"><math>~\frac{q^2 y}{\lambda_1}</math></td>
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| <td align="center"><math>~\frac{p^2 z}{\lambda_1}</math></td>
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| <td align="center"><math>~(x) \ell_{3D}</math></td>
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| <td align="center"><math>~(q^2 y)\ell_{3D}</math></td>
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| <td align="center"><math>~(p^2z) \ell_{3D}</math></td>
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| </tr>
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|
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| <tr>
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| <td align="center"><math>~2</math></td>
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| <td align="center"><math>~\frac{x}{ y^{1/q^2}}</math></td>
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| <td align="center"><math>~\frac{1}{\lambda_2}\biggl[\frac{x q^2 y }{(x^2 + q^4y^2)^{1 / 2}}\biggr] </math></td>
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| <td align="center"><math>~\frac{\lambda_2}{x}</math></td>
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| <td align="center"><math>~-\frac{\lambda_2}{q^2 y}</math></td>
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| <td align="center"><math>~0</math></td>
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| <td align="center"><math>~\frac{q^2 y }{(x^2 + q^4y^2)^{1 / 2}} </math></td>
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| <td align="center"><math>~- \frac{x }{(x^2 + q^4y^2)^{1 / 2}} </math></td>
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| <td align="center"><math>~0</math></td>
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| </tr>
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|
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| <tr>
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| <td align="center"><math>~3</math></td>
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| <td align="center">---</td>
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| <td align="center">---</td>
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| <td align="center">---</td>
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| <td align="center">---</td>
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| <td align="center">---</td>
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| <td align="center">---</td>
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| <td align="center">---</td>
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| <td align="center">---</td>
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| </tr>
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|
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| <tr>
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| <td align="left" colspan="9">
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| <table border="0" cellpadding="8" align="center">
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|
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| <tr>
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| <td align="right">
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| <math>~\ell_{3D}</math>
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| </td>
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| <td align="center">
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| <math>~\equiv</math>
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| </td>
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| <td align="left">
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| <math>~(x^2 + q^4y^2 + p^4 z^2 )^{- 1 / 2} </math>
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| </td>
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| </tr>
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|
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| </table>
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| </td>
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| </tr>
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| </table>
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|
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| The associated unit vector is, then,
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| <table border="0" cellpadding="5" align="center">
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|
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| <tr>
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| <td align="right">
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| <math>~\hat{e}_2</math>
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~
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| \hat\imath~\biggl[ \frac{q^2 y }{(x^2 + q^4y^2)^{1 / 2}} \biggr] - \hat\jmath~\biggl[ \frac{x }{(x^2 + q^4y^2)^{1 / 2}} \biggr] \, .
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| </math>
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| </td>
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| </tr>
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| </table>
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|
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| It is easy to see that <math>~\hat{e}_2 \cdot \hat{e}_2 = 1</math>. We also see that,
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| <table border="0" cellpadding="5" align="center">
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|
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| <tr>
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| <td align="right">
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| <math>~\hat{e}_1 \cdot \hat{e}_2</math>
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~
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| x \ell_{3D}\biggl[ \frac{q^2 y }{(x^2 + q^4y^2)^{1 / 2}} \biggr]
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| -
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| q^2y \ell_{3D} \biggl[ \frac{x }{(x^2 + q^4y^2)^{1 / 2}} \biggr] = 0 \, ,
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| </math>
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| </td>
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| </tr>
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| </table>
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| so it is clear that these first two unit vectors are orthogonal to one another.
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|
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| ==Search for the Third Coordinate==
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|
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| ===Cross Product of First Two Unit Vectors===
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|
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| The cross-product of these two unit vectors should give the third, namely,
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| <table border="0" cellpadding="5" align="center">
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|
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| <tr>
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| <td align="right">
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| <math>~\hat{e}_3 = \hat{e}_1 \times \hat{e}_2</math>
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~
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| \hat\imath~\biggl[ {e}_{1y}{e}_{2z} - {e}_{1z}{e}_{2y} \biggr]
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| +
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| \hat\jmath~\biggl[ {e}_{1z}{e}_{2x} - {e}_{1x}{e}_{2z} \biggr]
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| +
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| \hat{k}~\biggl[ {e}_{1x}{e}_{2y} - {e}_{1y}{e}_{2x} \biggr]
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| </math>
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| </td>
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| </tr>
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|
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| <tr>
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| <td align="right">
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|
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~
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| \hat\imath~\biggl[ \frac{x p^2z\ell_{3D}}{(x^2 + q^4y^2)^{1 / 2}} \biggr]
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| +
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| \hat\jmath~\biggl[ \frac{q^2 y p^2z \ell_{3D}}{(x^2 + q^4y^2)^{1 / 2}} \biggr]
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| -
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| \hat{k}~\biggl[ \frac{x^2\ell_{3D} }{(x^2 + q^4y^2)^{1 / 2}} ~+~ \frac{q^4 y^2\ell_{3D} }{(x^2 + q^4y^2)^{1 / 2}} \biggr]
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| </math>
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| </td>
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| </tr>
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|
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| <tr>
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| <td align="right">
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|
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| </td>
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| <td align="center">
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| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~ \frac{\ell_{3D}}{(x^2 + q^4y^2)^{1 / 2}} \biggl\{~
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| \hat\imath~( x p^2z )
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| +
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| \hat\jmath~(q^2 y p^2z )
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| -
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| \hat{k}~(x^2 + q^4y^2)
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| ~\biggr\} \, .
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| </math>
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| </td>
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| </tr>
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| </table>
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| Inserting these component expressions into the last row of the T8 Direction Cosine table gives …
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|
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| <table border="1" cellpadding="8" align="center">
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| <tr>
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| <td align="center" colspan="9">'''Direction Cosine Components for T8 Coordinates'''</td>
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| </tr>
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| <tr>
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| <td align="center"><math>~n</math></td>
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| <td align="center"><math>~\lambda_n</math></td>
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| <td align="center"><math>~h_n</math></td>
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| <td align="center"><math>~\frac{\partial \lambda_n}{\partial x}</math></td>
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| <td align="center"><math>~\frac{\partial \lambda_n}{\partial y}</math></td>
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| <td align="center"><math>~\frac{\partial \lambda_n}{\partial z}</math></td>
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| <td align="center"><math>~\gamma_{n1}</math></td>
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| <td align="center"><math>~\gamma_{n2}</math></td>
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| <td align="center"><math>~\gamma_{n3}</math></td>
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| </tr>
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|
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| <tr>
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| <td align="center"><math>~1</math></td>
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| <td align="center"><math>~(x^2 + q^2 y^2 + p^2 z^2)^{1 / 2} </math></td>
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| <td align="center"><math>~\lambda_1 \ell_{3D}</math></td>
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| <td align="center"><math>~\frac{x}{\lambda_1}</math></td>
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| <td align="center"><math>~\frac{q^2 y}{\lambda_1}</math></td>
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| <td align="center"><math>~\frac{p^2 z}{\lambda_1}</math></td>
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| <td align="center"><math>~(x) \ell_{3D}</math></td>
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| <td align="center"><math>~(q^2 y)\ell_{3D}</math></td>
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| <td align="center"><math>~(p^2z) \ell_{3D}</math></td>
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| </tr>
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|
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| <tr>
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| <td align="center"><math>~2</math></td>
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| <td align="center"><math>~\frac{x}{ y^{1/q^2}}</math></td>
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| <td align="center"><math>~\frac{1}{\lambda_2}\biggl[\frac{x q^2 y }{(x^2 + q^4y^2)^{1 / 2}}\biggr] </math></td>
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| <td align="center"><math>~\frac{\lambda_2}{x}</math></td>
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| <td align="center"><math>~-\frac{\lambda_2}{q^2 y}</math></td>
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| <td align="center"><math>~0</math></td>
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| <td align="center"><math>~\frac{q^2 y }{(x^2 + q^4y^2)^{1 / 2}} </math></td>
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| <td align="center"><math>~- \frac{x }{(x^2 + q^4y^2)^{1 / 2}} </math></td>
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| <td align="center"><math>~0</math></td>
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| </tr>
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|
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| <tr>
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| <td align="center"><math>~3</math></td>
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| <td align="center">---</td>
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| <td align="center">---</td>
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| <td align="center">---</td>
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| <td align="center">---</td>
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| <td align="center">---</td>
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| <td align="center"><math>~\frac{x p^2 z\ell_{3D}}{(x^2 + q^4y^2)^{1 / 2}} </math></td>
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| <td align="center"><math>~\frac{q^2 y p^2 z\ell_{3D}}{(x^2 + q^4y^2)^{1 / 2}} </math></td>
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| <td align="center"><math>~-\frac{(x^2 + q^4 y^2)\ell_{3D}}{(x^2 + q^4y^2)^{1 / 2}} </math></td>
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| </tr>
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|
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| <tr>
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| <td align="left" colspan="9">
| |
| <table border="0" cellpadding="8" align="center">
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|
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| <tr>
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| <td align="right">
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| <math>~\ell_{3D}</math>
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| </td>
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| <td align="center">
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| <math>~\equiv</math>
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| </td>
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| <td align="left">
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| <math>~(x^2 + q^4y^2 + p^4 z^2 )^{- 1 / 2} \, ,</math>
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| </td>
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| </tr>
| |
|
| |
| </table>
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| </td>
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| </tr>
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| </table>
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|
| |
|
| |
| ===Associated h<sub>3</sub> Scale Factor===
| |
| <table border="1" align="right" cellpadding="10"><tr><td align="center">
| |
| [[File:EUREKA 21Jan2021 sm.png|350px|Whiteboard EUREKA moment]]</td></tr></table>
| |
| After working through various scenarios on my whiteboard today (21 January 2021), I propose that,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{\partial \lambda_3}{\partial x}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\frac{xp^2z}{(x^2 + q^4y^2)} \, ;</math>
| |
| </td>
| |
| <td align="center> </td>
| |
| <td align="right">
| |
| <math>~\frac{\partial \lambda_3}{\partial y}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
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| </td>
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| <td align="left">
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| <math>~\frac{q^2 y p^2z}{(x^2 + q^4y^2)} \, ;</math>
| |
| </td>
| |
| <td align="center> and </td>
| |
| <td align="right">
| |
| <math>~\frac{\partial \lambda_3}{\partial z}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~-1 \, .</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| This means that,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~h_3^{-2}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\sum_{i=1}^3 \biggl( \frac{\partial \lambda_3}{\partial x_i}\biggr)^2</math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl[ \frac{xp^2z}{(x^2 + q^4y^2)} \biggr]^2
| |
| +
| |
| \biggl[ \frac{q^2 y p^2z}{(x^2 + q^4y^2)} \biggr]^2
| |
| +
| |
| \biggl[ -1 \biggr]^2
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{p^4z^2(x^2 + q^4y^2)}{(x^2 + q^4y^2)^2}
| |
| +
| |
| 1
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{(x^2 + q^4y^2 +p^4z^2)}{(x^2 + q^4y^2)}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{1}{\ell_{3D}^2 (x^2 + q^4y^2)}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow~~~ h_3</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \ell_{3D} (x^2 + q^4y^2)^{1 / 2} \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| This seems to work well because, when combined with the three separate expressions for <math>~\partial \lambda_3/\partial x_i</math>, this single expression for <math>~h_3</math> generates all three components of the third unit vector, that is, all three direction cosines, <math>~\gamma_{3i}</math>. All of the elements of this new "EUREKA moment" result have been entered into the following table.
| |
|
| |
|
| |
| <table border="1" cellpadding="8" align="center">
| |
| <tr>
| |
| <td align="center" colspan="9">'''Direction Cosine Components for T8 Coordinates'''</td>
| |
| </tr>
| |
| <tr>
| |
| <td align="center"><math>~n</math></td>
| |
| <td align="center"><math>~\lambda_n</math></td>
| |
| <td align="center"><math>~h_n</math></td>
| |
| <td align="center"><math>~\frac{\partial \lambda_n}{\partial x}</math></td>
| |
| <td align="center"><math>~\frac{\partial \lambda_n}{\partial y}</math></td>
| |
| <td align="center"><math>~\frac{\partial \lambda_n}{\partial z}</math></td>
| |
| <td align="center"><math>~\gamma_{n1}</math></td>
| |
| <td align="center"><math>~\gamma_{n2}</math></td>
| |
| <td align="center"><math>~\gamma_{n3}</math></td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="center"><math>~1</math></td>
| |
| <td align="center"><math>~(x^2 + q^2 y^2 + p^2 z^2)^{1 / 2} </math></td>
| |
| <td align="center"><math>~\lambda_1 \ell_{3D}</math></td>
| |
| <td align="center"><math>~\frac{x}{\lambda_1}</math></td>
| |
| <td align="center"><math>~\frac{q^2 y}{\lambda_1}</math></td>
| |
| <td align="center"><math>~\frac{p^2 z}{\lambda_1}</math></td>
| |
| <td align="center"><math>~(x) \ell_{3D}</math></td>
| |
| <td align="center"><math>~(q^2 y)\ell_{3D}</math></td>
| |
| <td align="center"><math>~(p^2z) \ell_{3D}</math></td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="center"><math>~2</math></td>
| |
| <td align="center"><math>~\frac{x}{ y^{1/q^2}}</math></td>
| |
| <td align="center"><math>~\frac{1}{\lambda_2}\biggl[\frac{x q^2 y }{(x^2 + q^4y^2)^{1 / 2}}\biggr] </math></td>
| |
| <td align="center"><math>~\frac{\lambda_2}{x}</math></td>
| |
| <td align="center"><math>~-\frac{\lambda_2}{q^2 y}</math></td>
| |
| <td align="center"><math>~0</math></td>
| |
| <td align="center"><math>~\frac{q^2 y }{(x^2 + q^4y^2)^{1 / 2}} </math></td>
| |
| <td align="center"><math>~- \frac{x }{(x^2 + q^4y^2)^{1 / 2}} </math></td>
| |
| <td align="center"><math>~0</math></td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="center"><math>~3</math></td>
| |
| <td align="center">---</td>
| |
| <td align="center"><math>~\ell_{3D}(x^2 + q^4 y^2)^{1 / 2}</math></td>
| |
| <td align="center"><math>~\frac{xp^2z}{(x^2 + q^4y^2)} </math></td>
| |
| <td align="center"><math>~\frac{q^2 y p^2z}{(x^2 + q^4y^2)}</math></td>
| |
| <td align="center"><math>~-1</math></td>
| |
| <td align="center"><math>~\frac{x p^2 z\ell_{3D}}{(x^2 + q^4y^2)^{1 / 2}} </math></td>
| |
| <td align="center"><math>~\frac{q^2 y p^2 z\ell_{3D}}{(x^2 + q^4y^2)^{1 / 2}} </math></td>
| |
| <td align="center"><math>~-\frac{(x^2 + q^4 y^2)\ell_{3D}}{(x^2 + q^4y^2)^{1 / 2}} </math></td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="left" colspan="9">
| |
| <table border="0" cellpadding="8" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\ell_{3D}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~\equiv</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~(x^2 + q^4y^2 + p^4 z^2 )^{- 1 / 2} </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| </table>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
|
| |
| ===What is the Third Coordinate Function, λ<sub>3</sub>===
| |
|
| |
| The remaining [https://en.wikipedia.org/wiki/The_$64,000_Question $64,000 question] is, "What is the actual expression for <math>~\lambda_3(x, y, z)</math> ? "
| |
|
| |
| Notice that the (partial) derivatives of <math>~\lambda_3</math> with respect to <math>~x</math> and <math>~y</math> may be rewritten, respectively, in the form
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\biggl( \frac{q^2 y}{p^2z} \biggr) \frac{\partial \lambda_3}{\partial x}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{q^2 y}{x(1 + \eta^2)}
| |
| =
| |
| \frac{\eta}{(1 + \eta^2)} \, ,
| |
| </math>
| |
| and,
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\biggl( \frac{x}{p^2z} \biggr) \frac{\partial \lambda_3}{\partial y}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{q^2y}{x(1 + \eta^2)}
| |
| =
| |
| \frac{\eta}{(1 + \eta^2)} \, ,
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| where,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\eta</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~\equiv</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{q^2y}{x} ~~~~\Rightarrow~~ \frac{\partial \ln\eta}{\partial \ln x} = -1 \, , ~~~~\frac{\partial \ln\eta}{\partial \ln y} = +1 \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| Then, after searching through the [[User:Tohline/Appendix/References#CRC|CRC Mathematical Handbook's]] pages of familiar derivative expressions, we appreciate that
| |
|
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{d}{dx_i} \biggl[\frac{1}{\cosh\gamma}\biggr]</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~- \biggl[ \frac{\tanh\gamma}{\cosh\gamma} \biggr] \frac{d\gamma}{dx_i} \, .</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| Hence, it will be useful to adopt the mapping,
| |
|
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\eta</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~~~\rightarrow~~~</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\sinh \gamma \, ,</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| because the right-hand side of both partial-derivative expressions becomes,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{\eta}{(1+\eta^2)}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~~~\rightarrow~~~</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\frac{\sinh\gamma}{\cosh^2\gamma} = \frac{\tanh\gamma}{\cosh\gamma} \, .</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| ====Guess A====
| |
| In particular, this suggests that we set,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\lambda_3</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\frac{A}{\cosh\gamma} \, ,</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| where,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\gamma</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~\equiv</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\sinh^{-1}\eta = \pm \cosh^{-1}[\eta^2 + 1]^{1 / 2} \, .</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| In other words,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\lambda_3</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~A[\eta^2 + 1]^{-1 / 2} \, .</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| Let's check the first and second partial derivatives.
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{\partial \lambda_3}{\partial x}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| - \frac{A}{2} \biggl[ \frac{2\eta}{(\eta^2 + 1)^{3 / 2}} \biggr] \frac{\partial \eta}{\partial x}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| ====Guess B====
| |
|
| |
| What if,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\lambda_3</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\frac{1}{2}\ln(1+\eta^2) \, .</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| Then,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{d\lambda_3}{d\eta}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{\eta}{(1+\eta^2)} \, ,
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| in which case we find,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{\partial\lambda_3}{\partial x_i} </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\frac{d\lambda_3}{d\eta} \cdot \frac{\partial\eta}{\partial x_i}</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| which means,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{\partial\lambda_3}{\partial x} </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{\eta}{(1+\eta^2)} \biggl[ - \frac{q^2 y}{x^2} \biggr]
| |
| =
| |
| - \frac{x}{(x^2 + q^4y^2)} \biggl[ \frac{q^4 y^2}{x^2} \biggr] \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| ====Guess C====
| |
|
| |
| What if,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\lambda_3</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\frac{1}{2} \ln(1+\eta^{-2}) \, .</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| Then,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{d\lambda_3}{d\eta}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~-
| |
| \frac{\eta^{-3}}{(1+\eta^{-2})}
| |
| =
| |
| -\frac{ \eta^{-1}}{(1+\eta^{2})}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| in which case we find,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{\partial\lambda_3}{\partial x_i} </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\frac{d\lambda_3}{d\eta} \cdot \frac{\partial\eta}{\partial x_i}</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| which means,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{\partial\lambda_3}{\partial x} </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| -\frac{\eta^{-1}}{(1+\eta^2)} \biggl[ - \frac{q^2 y}{x^2} \biggr]
| |
| =
| |
| \frac{x}{(x^2 + q^4y^2)} \, ;
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| and,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{\partial\lambda_3}{\partial y} </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| -\frac{\eta^{-1}}{(1+\eta^2)} \biggl[ \frac{q^2 }{x} \biggr]
| |
| =
| |
| -\frac{x^2}{y(x^2+ q^4y^2)}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| ==Inverting Coordinate Relations==
| |
|
| |
| ===In a Plane Perpendicular to the Z-Axis===
| |
| ====General Case====
| |
| At a fixed value of <math>~z = z_0</math>, let's invert the <math>~\lambda_1(x, y)</math> and <math>~\lambda_2(x, y)</math> relations to obtain expressions for <math>~x(\lambda_1, \lambda_2)</math> and <math>~y(\lambda_1, \lambda_2)</math>. Perhaps this will help us determine what the third coordinate expression should be.
| |
|
| |
| We start with,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\lambda_1</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~\equiv</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~(x^2 + q^2y^2 + p^2 z_0^2)^{1 / 2} \, ;</math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\lambda_2</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~\equiv</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\frac{x}{y^{1/q^2}} \, .</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| This means that,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\ln y</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~q^2(\ln x - \ln\lambda_2 ) \, ,</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| and,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~q^2 y^2</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~(\lambda_1^2 - p^2z_0^2) - x^2</math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow~~~2\ln y</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\ln\biggl\{ \frac{1}{q^2} \biggl[ (\lambda_1^2 - p^2z_0^2) - x^2 \biggr] \biggr\} \, .</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| Together, this gives,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\ln\biggl\{ \frac{1}{q^2} \biggl[ (\lambda_1^2 - p^2z_0^2) - x^2 \biggr] \biggr\} </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~2q^2(\ln x - \ln\lambda_2 ) </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\ln\biggl[\frac{x}{\lambda_2} \biggr]^{2q^2}</math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow~~~(\lambda_1^2 - p^2z_0^2) - x^2 </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~q^2\biggl[\frac{x}{\lambda_2} \biggr]^{2q^2} </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow~~~ x^2 +q^2\biggl[\frac{x}{\lambda_2} \biggr]^{2q^2} + (p^2z_0^2 - \lambda_1^2) </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~0 \, .</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| ====What if Axisymmetric (q<sup>2</sup> = 1)====
| |
|
| |
| In an axisymmetric configuration, <math>~q^2 = 1</math> and <math>~(\lambda_1^2 - p^2z_0^2) = \varpi^2</math>, so this general expression for <math>~x</math> becomes,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~0</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| x^2 + \biggl[\frac{x}{\lambda_2} \biggr]^{2} -\varpi^2
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| x^2\biggl[\frac{1 + \lambda_2^2}{\lambda_2^2}\biggr] -\varpi^2
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow~~~x</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \varpi \biggl[\frac{\lambda_2^2}{1 + \lambda_2^2}\biggr]^{1 / 2} \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| Given that, for axisymmetric systems,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~x</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\varpi \cos\varphi \, ,</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| we conclude that when <math>~q^2 = 1</math>,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\biggl[\frac{\lambda_2^2}{1 + \lambda_2^2}\biggr]^{1 / 2}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\cos\varphi </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow~~~\lambda_2^2</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\cot^2\varphi </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| ====What if q<sup>2</sup> = 2====
| |
| For example, if we choose <math>~q^2 = 2</math>, we have a quadratic expression for <math>~x^2</math>, namely,
| |
|
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~0 </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~x^2 + 2\biggl[\frac{x}{\lambda_2} \biggr]^{4} + (p^2z_0^2 - \lambda_1^2) </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow ~~~ 0 </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~x^{4} + \frac{1}{2} \lambda_2^4~ x^2 + \frac{1}{2}\lambda_2^4(p^2z_0^2 - \lambda_1^2) </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow ~~~ 2x^2 </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| - \frac{\lambda_2^4}{2} \pm \biggl[ \frac{\lambda_2^8}{4} - 2\lambda_2^4(p^2z_0^2 - \lambda_1^2) \biggr]^{1 / 2}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{\lambda_2^4}{2} \biggl\{ \biggl[ 1 - \frac{8(p^2z_0^2 - \lambda_1^2)}{\lambda_2^4} \biggr]^{1 / 2} - 1 \biggr\}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow ~~~ x^2 </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{\lambda_2^4}{4} \biggl\{ \biggl[ 1 - \frac{8(p^2z_0^2 - \lambda_1^2)}{\lambda_2^4} \biggr]^{1 / 2} - 1 \biggr\} \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| Given that, for <math>~q^2 = 2</math>, one of the two defining expression means, <math>~\lambda_2 = x/\sqrt{y}</math>, we also have,
| |
|
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~y </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{\lambda_2^2}{4} \biggl\{ \biggl[ 1 - \frac{8(p^2z_0^2 - \lambda_1^2)}{\lambda_2^4} \biggr]^{1 / 2} - 1 \biggr\} \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| ===New 2<sup>nd</sup> Coordinate===
| |
|
| |
| Apparently it will be cleaner to define a new "2<sup>nd</sup> coordinate," <math>~\kappa_2</math>, such that,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\kappa_2^{2q^2}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~\equiv</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| q^2\biggl[\frac{1}{\lambda_2} \biggr]^{2q^2}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow~~~\kappa_2</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~\equiv</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| q^{1/q^2}\biggl[\frac{1}{\lambda_2} \biggr]
| |
| =
| |
| q^{1/q^2}\biggl[\frac{y^{1/q^2}}{x} \biggr]
| |
| =
| |
| \frac{(qy)^{1/q^2}}{x} \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| (With this new definition, <math>~\kappa_2 \sim \tan\varphi</math>; it is exactly this when <math>~q^2 = 1</math>.) Then we can rewrite the last expression from the [[#General_Case|above general case]] as,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~x^2 +(\kappa_2 x)^{2q^2} - (\lambda_1^2 - p^2z_0^2 ) </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~0 \, .</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| When <math>~q=1</math> (the axisymmetric case), this gives,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~x^2(1+\kappa_2^2)</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~ (\lambda_1^2 - p^2z_0^2 ) </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow~~~\frac{x^2}{(\lambda_1^2 - p^2z_0^2 ) }</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~ \frac{1}{(1+\kappa_2^2)} \, ,</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| which means that <math>~\kappa_2 = \tan\varphi</math>. And, for the case of <math>~q^2 = 2</math>, after making the substitution,
| |
| <div align="center"><math>~\lambda_2 \rightarrow (q)^{1/q^2}\kappa_2^{-1} = \frac{2^{1 / 4}}{\kappa_2} \, ,</math></div>
| |
| we find,
| |
|
| |
| <table border="0" cellpadding="5" align="center">
| |
| <tr>
| |
| <td align="right">
| |
| <math>~x^2 </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{\lambda_2^4}{4} \biggl\{ \biggl[ 1 - \frac{8(p^2z_0^2 - \lambda_1^2)}{\lambda_2^4} \biggr]^{1 / 2} - 1 \biggr\} \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow~~~ x^2 </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{1}{2\kappa_2^4} \biggl\{ \biggl[ 1 + 4\kappa_2^4(\lambda_1^2 - p^2z_0^2 ) \biggr]^{1 / 2} - 1 \biggr\} \, ,
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| and,
| |
|
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~y = \biggl(\frac{\kappa_2^2}{2^{1 / 2}} \biggr) x^2 </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\biggl(\frac{\kappa_2^2}{2^{1 / 2}} \biggr)
| |
| \frac{1}{2\kappa_2^4} \biggl\{ \biggl[ 1 + 4\kappa_2^4(\lambda_1^2 - p^2z_0^2 ) \biggr]^{1 / 2} - 1 \biggr\}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{1}{2^{3 / 2}\kappa_2^2} \biggl\{ \biggl[ 1 + 4\kappa_2^4(\lambda_1^2 - p^2z_0^2 ) \biggr]^{1 / 2} - 1 \biggr\} \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| =Angle Between Unit Vectors=
| |
| We begin by restating that the coordinate, scale factor, and unit vector associated with the normal to our ellipsoidal surface are,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\lambda_1</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~\equiv</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~(x^2 + q^2y^2 + p^2z^2)^{1 / 2} \, ,</math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~h_1</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\lambda_1 \ell_{3D} \, ,</math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\hat{e}_1</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \hat\imath (x\ell_{3D} )
| |
| +
| |
| \hat\jmath (q^2 y\ell_{3D} )
| |
| +
| |
| \hat{k} (p^2z\ell_{3D} ) \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| In the [[#TableKappa8|Table below titled, "Direction Cosines Components for κ8 Coordinates"]], there are two fully-formed unit vectors that are each orthogonal to the (first) unit vector that is normal to the ellipsoid's surface. Here we will refer to the coordinates of these two fully-formed unit vectors as,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\lambda_2</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~\equiv</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\frac{xy^{1/q^2}}{z^{2/p^2}}</math>
| |
| </td>
| |
| <td align="center"> and, </td>
| |
| <td align="right">
| |
| <math>~\kappa_2</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~\equiv</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\frac{(qy)^{1/q^2}}{x} \, .</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| The associated scale factors and unit vectors are given by the following expressions:
| |
|
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~h_{\lambda_2}^{-2}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \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
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl(\frac{\lambda_2}{x} \biggr)^2
| |
| +
| |
| \biggl(\frac{\lambda_2}{q^2y} \biggr)^2
| |
| +
| |
| \biggl(- \frac{2\lambda_2}{p^2z} \biggr)^2
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~ \lambda_2^2 \biggl[
| |
| \frac{q^4y^2p^4z^2 + x^2p^4z^2 + 4x^2 q^4y^2}{x^2 q^4y^2 p^4z^2}
| |
| \biggr]
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow ~~~ h_{\lambda_2}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{x q^2y p^2z}{\lambda_2 \mathcal{D}}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow ~~~ \hat{e}_{\lambda_2}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \hat\imath \biggl[ h_{\lambda_2} \biggl(\frac{\partial \lambda_2}{\partial x}\biggr)\biggr]
| |
| +
| |
| \hat\jmath \biggl[ h_{\lambda_2} \biggl(\frac{\partial \lambda_2}{\partial y}\biggr)\biggr]
| |
| +
| |
| \hat{k} \biggl[ h_{\lambda_2} \biggl(\frac{\partial \lambda_2}{\partial z}\biggr)\biggr]
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \hat\imath \biggl[ \frac{q^2y p^2z}{\mathcal{D}} \biggr]
| |
| +
| |
| \hat\jmath \biggl[ \frac{xp^2z}{\mathcal{D}} \biggr]
| |
| -
| |
| \hat{k} \biggl[ \frac{2x q^2y }{\mathcal{D}} \biggr] \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
|
| |
| <table border="1" width="80%" align="center" cellpadding="8"><tr><td align="left">
| |
| With regard to orthogonality, note that,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\hat{e}_1 \cdot \hat{e}_{\lambda_2}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl[
| |
| \hat\imath (x\ell_{3D} )
| |
| +
| |
| \hat\jmath (q^2 y\ell_{3D} )
| |
| +
| |
| \hat{k} (p^2z\ell_{3D} )
| |
| \biggr] \cdot
| |
| \biggl\{
| |
| \hat\imath \biggl[ \frac{q^2y p^2z}{\mathcal{D}} \biggr]
| |
| +
| |
| \hat\jmath \biggl[ \frac{xp^2z}{\mathcal{D}} \biggr]
| |
| -
| |
| \hat{k} \biggl[ \frac{2x q^2y }{\mathcal{D}} \biggr]
| |
| \biggr\}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| (x\ell_{3D} )\biggl[ \frac{q^2y p^2z}{\mathcal{D}} \biggr]
| |
| +
| |
| (q^2 y\ell_{3D} )\biggl[ \frac{xp^2z}{\mathcal{D}} \biggr]
| |
| -
| |
| (p^2z\ell_{3D} )\biggl[ \frac{2x q^2y }{\mathcal{D}} \biggr]
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| 0 \, .</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| </td></tr></table>
| |
|
| |
|
| |
| And,
| |
|
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~h_{\kappa_2}^{-2}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl(\frac{\partial\kappa_2}{\partial x} \biggr)^2
| |
| +
| |
| \biggl(\frac{\partial\kappa_2}{\partial y} \biggr)^2
| |
| +
| |
| \biggl(\frac{\partial\kappa_2}{\partial z} \biggr)^2
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl(-\frac{\kappa_2}{x} \biggr)^2
| |
| +
| |
| \biggl(\frac{\kappa_2}{q^2 y} \biggr)^2
| |
| =
| |
| \frac{\kappa_2^2}{x^2q^4y^2}\biggl[x^2 + q^4y^2\biggr]
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow~~~h_{\kappa_2}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{xq^2y}{\kappa_2 (x^2 + q^4y^2)^{1 / 2}}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow~~~\hat{e}_{\kappa_2}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| -~\hat\imath \biggl[ \frac{q^2y}{(x^2 + q^4y^2)^{1 / 2}}\biggr]
| |
| +
| |
| \hat\jmath \biggl[ \frac{x}{(x^2 + q^4y^2)^{1 / 2}} \biggr]
| |
| +
| |
| \hat{k} \biggl[ 0 \biggr] \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
|
| |
| <table border="1" width="80%" align="center" cellpadding="8"><tr><td align="left">
| |
| Again, note that with regard to orthogonality,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\hat{e}_1 \cdot \hat{e}_{\kappa_2}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl[
| |
| \hat\imath (x\ell_{3D} )
| |
| +
| |
| \hat\jmath (q^2 y\ell_{3D} )
| |
| +
| |
| \hat{k} (p^2z\ell_{3D} )
| |
| \biggr] \cdot
| |
| \biggl\{
| |
| -\hat\imath \biggl[ \frac{q^2y}{(x^2 + q^4y^2)^{1 / 2}}\biggr]
| |
| +
| |
| \hat\jmath \biggl[ \frac{x}{(x^2 + q^4y^2)^{1 / 2}} \biggr]
| |
| \biggr\}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| -~(x\ell_{3D} )\biggl[ \frac{q^2y}{(x^2 + q^4y^2)^{1 / 2}} \biggr]
| |
| +
| |
| (q^2 y\ell_{3D} )\biggl[ \frac{x}{(x^2 + q^4y^2)^{1 / 2}} \biggr]
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| 0 \, .</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| </td></tr></table>
| |
|
| |
|
| |
| From this pair of orthogonality checks, we appreciate that both unit vectors always lie in the plane that is tangent to the surface of our ellipsoid. Next, let's determine the angle, <math>~\alpha</math>, between these two unit vectors as measured in the relevant tangent-plane.
| |
|
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\cos\alpha \equiv \hat{e}_{\lambda_2} \cdot \hat{e}_{\kappa_2}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl\{
| |
| \hat\imath \biggl[ \frac{q^2y p^2z}{\mathcal{D}} \biggr]
| |
| +
| |
| \hat\jmath \biggl[ \frac{xp^2z}{\mathcal{D}} \biggr]
| |
| -
| |
| \hat{k} \biggl[ \frac{2x q^2y }{\mathcal{D}} \biggr]
| |
| \biggr\}
| |
| \biggl\{
| |
| -\hat\imath \biggl[ \frac{q^2y}{(x^2 + q^4y^2)^{1 / 2}}\biggr]
| |
| +
| |
| \hat\jmath \biggl[ \frac{x}{(x^2 + q^4y^2)^{1 / 2}} \biggr]
| |
| +
| |
| \hat{k} \biggl[ 0 \biggr]
| |
| \biggr\}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| -\biggl[ \frac{q^2y}{(x^2 + q^4y^2)^{1 / 2}}\biggr]\biggl[ \frac{q^2y p^2z}{\mathcal{D}} \biggr]
| |
| +
| |
| \biggl[ \frac{x}{(x^2 + q^4y^2)^{1 / 2}} \biggr]\biggl[ \frac{xp^2z}{\mathcal{D}} \biggr]
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl[ \frac{p^2 z}{\mathcal{D} (x^2 + q^4y^2)^{1 / 2}} \biggr] \biggl[ x^2 - q^4y^2 \biggr] \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
|
| |
| ----
| |
|
| |
|
| |
| Let's again visit the unit vector that we know lies in the tangent-plane and is always orthogonal to <math>~\lambda_2</math>, namely,
| |
|
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\hat{e}_{\lambda_3}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| -~\hat\imath \biggl[ x(2q^4 y^2 + p^4z^2 )\biggr]\frac{\ell_{3D}}{\mathcal{D}}
| |
| +
| |
| \hat\jmath \biggl[q^2y(p^4z^2 + 2x^2) \biggr]\frac{\ell_{3D}}{\mathcal{D}}
| |
| +
| |
| \hat{k} \biggl[p^2z (x^2 - q^4y^2) \biggr]\frac{\ell_{3D}}{\mathcal{D}}
| |
| \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| We acknowledge that,
| |
|
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\hat{e}_{\lambda_2} \cdot \hat{e}_{\lambda_3}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl\{
| |
| \hat\imath \biggl[ \frac{q^2y p^2z}{\mathcal{D}} \biggr]
| |
| +
| |
| \hat\jmath \biggl[ \frac{xp^2z}{\mathcal{D}} \biggr]
| |
| -
| |
| \hat{k} \biggl[ \frac{2x q^2y }{\mathcal{D}} \biggr]
| |
| \biggr\}
| |
| \biggl\{
| |
| -~\hat\imath \biggl[ x(2q^4 y^2 + p^4z^2 )\biggr]\frac{\ell_{3D}}{\mathcal{D}}
| |
| +
| |
| \hat\jmath \biggl[q^2y(p^4z^2 + 2x^2) \biggr]\frac{\ell_{3D}}{\mathcal{D}}
| |
| +
| |
| \hat{k} \biggl[p^2z (x^2 - q^4y^2) \biggr]\frac{\ell_{3D}}{\mathcal{D}}
| |
| \biggr\}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| -~\biggl[ xq^2yp^2z(2q^4 y^2 + p^4z^2 )\biggr]\frac{\ell_{3D}}{\mathcal{D}^2}
| |
| +
| |
| \biggl[x q^2y p^2z(p^4z^2 + 2x^2) \biggr]\frac{\ell_{3D}}{\mathcal{D}^2}
| |
| -
| |
| \biggl[2xq^2y p^2z (x^2 - q^4y^2) \biggr]\frac{\ell_{3D}}{\mathcal{D}^2}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\biggl[
| |
| -(2q^4 y^2 + p^4z^2 )
| |
| +
| |
| (p^4z^2 + 2x^2)
| |
| -
| |
| 2 (x^2 - q^4y^2)
| |
| \biggr] \frac{(x q^2y p^2z) \ell_{3D}}{\mathcal{D}^2}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| 0 \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| =Kappa (κ8) Coordinates=
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\kappa_1</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~\equiv</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~(x^2 + q^2y^2 + p^2 z^2)^{1 / 2} \, ;</math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\kappa_3</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~\equiv</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\tan^{-1}\biggl[ \frac{(qy)^{1/q^2}}{x} \biggr] \, .</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{\partial\kappa_3}{\partial x}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl[1 + \frac{(qy)^{2/q^2}}{x^2} \biggr]^{-1} \biggl[- \frac{(qy)^{1/q^2}}{x^2} \biggr]
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| -\frac{\sin^2\kappa_3}{(qy)^{1/q^2}} = -\frac{\sin^2\kappa_3}{x\tan\kappa_3}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| -\frac{\sin\kappa_3 \cos\kappa_3}{x}\, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{\partial\kappa_3}{\partial y}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl[1 + \frac{(qy)^{2/q^2}}{x^2} \biggr]^{-1} \biggl[\frac{q^{1/q^2} y^{1/q^2}}{q^2 x y} \biggr]
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl[1 + \frac{(qy)^{2/q^2}}{x^2} \biggr]^{-1} \biggl[\frac{(qy)^{1/q^2}}{x } \biggr] \frac{1}{q^2y}
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{1}{q^2y}\biggl[\frac{\tan\kappa_3}{1 + \tan^2\kappa_3 }\biggr]
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| + \frac{\sin\kappa_3 \cos\kappa_3}{q^2y} \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| Therefore,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~h_3^{-2}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl[-\frac{\sin\kappa_3 \cos\kappa_3}{x} \biggr]^2
| |
| +
| |
| \biggl[\frac{\sin\kappa_3 \cos\kappa_3}{q^2y} \biggr]^2
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~(x^2 + q^4y^2)
| |
| \biggl[\frac{\sin\kappa_3 \cos\kappa_3}{xq^2y} \biggr]^2
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow~~~ h_3</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~(x^2 + q^4y^2)^{-1 / 2}
| |
| \biggl[\frac{xq^2y}{\sin\kappa_3 \cos\kappa_3} \biggr] \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
|
| |
| <span id="TableKappa8"> </span>
| |
| <table border="1" cellpadding="8" align="center">
| |
| <tr>
| |
| <td align="center" colspan="9">'''Direction Cosine Components for κ8 Coordinates'''</td>
| |
| </tr>
| |
| <tr>
| |
| <td align="center"><math>~n</math></td>
| |
| <td align="center"><math>~\kappa_n</math></td>
| |
| <td align="center"><math>~h_n</math></td>
| |
| <td align="center"><math>~\frac{\partial \kappa_n}{\partial x}</math></td>
| |
| <td align="center"><math>~\frac{\partial \kappa_n}{\partial y}</math></td>
| |
| <td align="center"><math>~\frac{\partial \kappa_n}{\partial z}</math></td>
| |
| <td align="center"><math>~\gamma_{n1}</math></td>
| |
| <td align="center"><math>~\gamma_{n2}</math></td>
| |
| <td align="center"><math>~\gamma_{n3}</math></td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="center"><math>~1</math></td>
| |
| <td align="center"><math>~(x^2 + q^2 y^2 + p^2 z^2)^{1 / 2} </math></td>
| |
| <td align="center"><math>~\kappa_1 \ell_{3D}</math></td>
| |
| <td align="center"><math>~\frac{x}{\kappa_1}</math></td>
| |
| <td align="center"><math>~\frac{q^2 y}{\kappa_1}</math></td>
| |
| <td align="center"><math>~\frac{p^2 z}{\kappa_1}</math></td>
| |
| <td align="center"><math>~(x) \ell_{3D}</math></td>
| |
| <td align="center"><math>~(q^2 y)\ell_{3D}</math></td>
| |
| <td align="center"><math>~(p^2z) \ell_{3D}</math></td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="center"><math>~2</math></td>
| |
| <td align="center">---</td>
| |
| <td align="center"><math>~\ell_{3D}(x^2 + q^4 y^2)^{1 / 2}</math></td>
| |
| <td align="center"><math>~\frac{xp^2z}{(x^2 + q^4y^2)} </math></td>
| |
| <td align="center"><math>~\frac{q^2 y p^2z}{(x^2 + q^4y^2)}</math></td>
| |
| <td align="center"><math>~-1</math></td>
| |
| <td align="center"><math>~\frac{x p^2 z\ell_{3D}}{(x^2 + q^4y^2)^{1 / 2}} </math></td>
| |
| <td align="center"><math>~\frac{q^2 y p^2 z\ell_{3D}}{(x^2 + q^4y^2)^{1 / 2}} </math></td>
| |
| <td align="center"><math>~-\frac{(x^2 + q^4 y^2)\ell_{3D}}{(x^2 + q^4y^2)^{1 / 2}} </math></td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="center"><math>~3</math></td>
| |
| <td align="center"><math>~\tan^{-1}\biggl[ \frac{(qy)^{1/q^2}}{x} \biggr]</math></td>
| |
| <td align="center"><math>~\frac{1}{\sin\kappa_3 \cos\kappa_3}\biggl[\frac{x q^2 y }{(x^2 + q^4y^2)^{1 / 2}}\biggr] </math></td>
| |
| <td align="center"><math>~-\frac{\sin\kappa_3 \cos\kappa_3}{x}</math></td>
| |
| <td align="center"><math>~\frac{\sin\kappa_3 \cos\kappa_3}{q^2 y}</math></td>
| |
| <td align="center"><math>~0</math></td>
| |
| <td align="center"><math>~- \frac{q^2 y }{(x^2 + q^4y^2)^{1 / 2}} </math></td>
| |
| <td align="center"><math>~\frac{x }{(x^2 + q^4y^2)^{1 / 2}} </math></td>
| |
| <td align="center"><math>~0</math></td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="left" colspan="9">
| |
| <table border="0" cellpadding="8" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\ell_{3D}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~\equiv</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~(x^2 + q^4y^2 + p^4 z^2 )^{- 1 / 2} </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| </table>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="center"><math>~4</math></td>
| |
| <td align="center"><math>~\frac{x y^{1/q^2}}{ z^{2/p^2}}</math></td>
| |
| <td align="center"><math>~\frac{1}{\kappa_4}\biggl[\frac{x q^2 y p^2 z}{ \mathcal{D}}\biggr] </math></td>
| |
| <td align="center"><math>~\frac{\kappa_4}{x}</math></td>
| |
| <td align="center"><math>~\frac{\kappa_4}{q^2 y}</math></td>
| |
| <td align="center"><math>~-\frac{2\kappa_4}{p^2 z}</math></td>
| |
| <td align="center"><math>~\frac{x q^2 y p^2 z}{\mathcal{D}} \biggl(\frac{1}{x}\biggr)</math></td>
| |
| <td align="center"><math>~ \frac{x q^2 y p^2 z}{\mathcal{D}} \biggl(\frac{1}{q^2y}\biggr)</math></td>
| |
| <td align="center"><math>~\frac{x q^2 y p^2 z}{\mathcal{D}} \biggl(-\frac{2}{p^2z}\biggr)</math></td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="center"><math>~5</math></td>
| |
| <td align="center">---</td>
| |
| <td align="center">---</td>
| |
| <td align="center">---</td>
| |
| <td align="center">---</td>
| |
| <td align="center">---</td>
| |
| <td align="center"><math>~-\frac{\ell_{3D}}{\mathcal{D}}\biggl[ x(2 q^4y^2 + p^4z^2 ) \biggl]</math></td>
| |
| <td align="center"><math>~\frac{\ell_{3D}}{\mathcal{D}}\biggl[ q^2 y(p^4z^2 + 2x^2 ) \biggl]</math></td>
| |
| <td align="center"><math>~\frac{\ell_{3D}}{\mathcal{D}}\biggl[ p^2z( x^2 - q^4y^2 ) \biggl]</math></td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="left" colspan="9">
| |
| <table border="0" cellpadding="8" 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>
| |
| Also note …
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~AB \equiv \biggl( \frac{\mathcal{D}}{\ell_{3D}} \biggr)^{2} </math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl[ x(2 q^4y^2 + p^4z^2 ) \biggl]^2
| |
| +
| |
| \biggl[ q^2 y(p^4z^2 + 2x^2 ) \biggl]^2
| |
| +
| |
| \biggl[ p^2z( x^2 - q^4y^2 ) \biggl]^2 \, ,
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| and the partial derivatives of <math>~A</math> and <math>~B</math> are detailed in [[User:Tohline/Appendix/Ramblings/ConcentricEllipsodalCoordinates#ABderivatives|an accompanying discussion]].
| |
| </td>
| |
| </tr>
| |
|
| |
| </table>
| |
|
| |
| The direction-cosines of the second unit vector — as has already been inserted into the "κ8 coordinates" table — should be obtainable from the first and third unit vectors via the cross product,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\hat{e}_2 = \hat{e}_3 \times \hat{e}_1</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \hat\imath \biggl[ e_{3y}e_{1z} - e_{3z} e_{1y} \biggr]
| |
| +
| |
| \hat\jmath \biggl[ e_{3z}e_{1x} - e_{3x} e_{1z} \biggr]
| |
| +
| |
| \hat{k} \biggl[ e_{3x}e_{1y} - e_{3y} e_{1x} \biggr]
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \hat\imath \biggl[ \frac{x (p^2z) \ell_{3D} }{(x^2 + q^4y^2)^{1 / 2}} \biggr]
| |
| +
| |
| \hat\jmath \biggl[ \frac{q^2 y (p^2z) \ell_{3D}}{(x^2 + q^4y^2)^{1 / 2}}\biggr]
| |
| -
| |
| \hat{k} \biggl[ \frac{(x^2 + q^4y^2) \ell_{3D} }{(x^2 + q^4y^2)^{1 / 2}} \biggr] \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
| The other boxes in the n = 2 row have been drawn from [[User:Tohline/Appendix/Ramblings/ConcentricEllipsodalT8Coordinates#Associated_h3_Scale_Factor|our accompanying EUREKA! moment]] and the n = 3 row of the table that details "Direction Cosine Components for T8 Coordinates."
| |
|
| |
| ==Attempt 1==
| |
| Let's try …
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\kappa_2</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~\equiv</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\tan^{-1}\biggl[ \frac{x(qy)^{1/q^2}}{(pz)^{1/p^2}} \biggr] \, ,</math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| which leads to,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{\partial\kappa_3}{\partial x}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl[1 + \frac{x^2(qy)^{2/q^2}}{(pz)^{2/p^2}} \biggr]^{-1} \biggl[ \frac{(qy)^{1/q^2}}{(pz)^{1/p^2}} \biggr]
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{1}{x}\biggl[1+\tan^2\kappa_2\biggr]^{-1} \tan\kappa_2 = \frac{\sin\kappa_2 \cos\kappa_2}{x} \, ;
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{\partial\kappa_3}{\partial y}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl[1 + \frac{x^2(qy)^{2/q^2}}{(pz)^{2/p^2}} \biggr]^{-1} \biggl[ \frac{xq^{1/q^2}(y)^{1/q^2}}{q^2 y(pz)^{1/p^2}} \biggr]
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \frac{1}{q^2y}\biggl[1+\tan^2\kappa_2\biggr]^{-1} \tan\kappa_2 = \frac{\sin\kappa_2 \cos\kappa_2}{q^2y} \, ;
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\frac{\partial\kappa_3}{\partial z}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| - \frac{\sin\kappa_2 \cos\kappa_2}{p^2z} \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| </table>
| |
| Hence,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~h_2^{-2}</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~\sin^2\kappa_2 \cos^2\kappa_2 \biggl[ \frac{1}{x^2} + \frac{1}{q^4y^2} + \frac{1}{p^4z^2} \biggr]</math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
|
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \sin^2\kappa_2 \cos^2\kappa_2 \biggl[ \frac{x^2 + q^4 y^2 + p^4 z^2}{x^2 q^4y^2 p^4 z^2} \biggr]
| |
| =
| |
| \biggl[ \frac{\sin^2\kappa_2 \cos^2\kappa_2 }{x^2 q^4y^2 p^4 z^2 \ell_{3D}^2} \biggr]
| |
| </math>
| |
| </td>
| |
| </tr>
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\Rightarrow~~~ h_2</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl[ \frac{x q^2y p^2 z \ell_{3D}}{\sin\kappa_2 \cos\kappa_2 } \biggr] \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
| The three direction-cosines are, then,
| |
| <table border="0" cellpadding="5" align="center">
| |
|
| |
| <tr>
| |
| <td align="right">
| |
| <math>~\gamma_{21} = h_2 \biggl(\frac{\partial \kappa_2}{\partial x}\biggr)</math>
| |
| </td>
| |
| <td align="center">
| |
| <math>~=</math>
| |
| </td>
| |
| <td align="left">
| |
| <math>~
| |
| \biggl[ \frac{x q^2y p^2 z \ell_{3D}}{\sin\kappa_2 \cos\kappa_2 } \biggr] \frac{\sin\kappa_2 \cos\kappa_2}{x}
| |
| =
| |
| q^2y p^2z \ell_{3D} \, .
| |
| </math>
| |
| </td>
| |
| </tr>
| |
| </table>
| |
|
| |
|
| =T9 Coordinates= | | =T9 Coordinates= |