Editing
ThreeDimensionalConfigurations/ChallengesPt4
(section)
Jump to navigation
Jump to search
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
==Reconcile ''Results'' Differences== <span id="Fig1">Before calling upon any of Riemann's model parameters</span>, from geometric considerations alone we should be able to determine exactly what the expression is for any off-center ellipse that results from slicing — at a tipped angle — the chosen ellipsoid. <table border="1" width="50%" cellpadding="8" align="center"> <tr> <td align="center" colspan="3"><b>Figure 1</b></td> </tr> <tr> <td align="left"> <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>~x' \, ,</math> </td> </tr> <tr> <td align="right"> <math>~y</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ y' \cos\theta - z'\sin\theta \, ,</math> </td> </tr> <tr> <td align="right"> <math>~(z - z_0)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ z' \cos\theta + y'\sin\theta \, .</math> </td> </tr> </table> </td> <td align="center">[[File:ExcelAxes02C.png|400px|Primed Coordinates]]</td> <td align="left"> <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>~x \, ,</math> </td> </tr> <tr> <td align="right"> <math>~y'</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ y \cos\theta + (z - z_0) \sin\theta \, ,</math> </td> </tr> <tr> <td align="right"> <math>~z'</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ (z-z_0) \cos\theta - y \sin\theta \, .</math> </td> </tr> </table> </td> </tr> </table> ===Body Frame=== As has been shown in [[ThreeDimensionalConfigurations/ChallengesPt2#Intersection_of_Tipped_Plane_With_Ellipsoid_Surface|our accompanying discussion]], we obtain the following, <table border="0" cellpadding="5" align="center"> <tr> <td align="center" colspan="3"><font color="maroon">'''Intersection Expression'''</font></td> </tr> <tr> <td align="right"> <math>~1 - \frac{x^2}{a^2} </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~y^2 \biggl[\frac{c^2 + b^2\tan^2\theta}{b^2c^2} \biggr] + y \biggl[ \frac{2z_0 \tan\theta}{c^2} \biggr] + \frac{z_0^2}{c^2} \, , </math> </td> </tr> </table> as long as z<sub>0</sub> lies within the range, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~z_0^2</math> </td> <td align="center"> <math>~\le</math> </td> <td align="left"> <math>~c^2 + b^2\tan^2\theta \, .</math> </td> </tr> </table> <table border="1" align="center" cellpadding="8" width="80%"><tr><td align="left"> Given the values of <math>~a, b, c, \theta, z_0</math>, we can immediately map this to the tipped plane to obtain the surface-intersection function, <math>~x'(y')</math>. Specifically we find, <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>~a \biggl\{ 1 - \biggl[ (y'\cos\theta - \cancelto{0}{z'} \sin\theta)^2 \biggl( \frac{c^2 + b^2\tan^2\theta}{b^2c^2} \biggr) + (y'\cos\theta - \cancelto{0}{z'} \sin\theta) \biggl( \frac{2z_0 \tan\theta}{c^2} \biggr) + \frac{z_0^2}{c^2} \biggr] \biggr\}^{1 / 2}</math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~a \biggl\{ 1 - \biggl[ (y'\cos\theta)^2 \biggl( \frac{c^2 + b^2\tan^2\theta}{b^2c^2} \biggr) + y'\cos\theta \biggl( \frac{2z_0 \tan\theta}{c^2} \biggr) + \frac{z_0^2}{c^2} \biggr] \biggr\}^{1 / 2}</math> </td> </tr> </table> </td></tr></table> Along the ''tipped'' <math>~y'</math> axis, two points will mark the ends of the x'-y' orbit; they are identified by the roots of this ''Intersection Expression'' when x = 0. That is, by the roots of, <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>~y^2 \biggl[\frac{\kappa^2}{\cos^2\theta} \biggr] + y \biggl[ \frac{2z_0 \tan\theta}{c^2} \biggr] + \biggl[\frac{z_0^2}{c^2} -1 \biggr] \, ,</math> </td> </tr> </table> where, <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>~ \frac{c^2 \cos^2\theta + b^2 \sin^2\theta}{b^2c^2} \, . </math> </td> </tr> </table> The roots are … <table border="1" align="center" cellpadding="8" width="80%"><tr><td align="left"> Scratch notes: <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~y_\mathrm{edge}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\frac{B}{2A} \biggl\{\pm \biggl[1 - \frac{4AC}{B^2} \biggr]^{1 / 2} -1 \biggr\}</math> </td> </tr> </table> where, <div align="center"> <math>~ \frac{4AC}{B^2} = \frac{4\kappa^2}{\cos^2\theta} \biggl[\frac{z_0^2}{c^2} -1 \biggr] \biggl[ \frac{2z_0 \tan\theta}{c^2} \biggr]^{-2} = \frac{\kappa^2}{\cos^2\theta} \biggl[ \frac{c^2(z_0^2 - c^2)}{z_0^2 \tan^2\theta} \biggr] = \biggl[ \frac{c^2 \kappa^2 (z_0^2 - c^2)}{z_0^2 \sin^2\theta} \biggr] </math> </div> </td></tr></table> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~y_\mathrm{edge}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\biggl[ \frac{z_0 \sin\theta \cos\theta}{c^2 \kappa^2} \biggr]\biggl\{\pm \biggl[1 - \frac{c^2 \kappa^2 (z_0^2 - c^2)}{z_0^2 \sin^2\theta} \biggr]^{1 / 2} -1 \biggr\}</math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\biggl[ \frac{\cos\theta}{c^2 \kappa^2} \biggr]\biggl\{\pm \biggl[z_0^2 \sin^2\theta + c^2 \kappa^2 (c^2 - z_0^2 ) \biggr]^{1 / 2} - z_0 \sin\theta \biggr\} \, .</math> </td> </tr> </table> Hereafter we will use <math>~y_p</math> to denote the "plus" root, and <math>~y_m</math> to denote the "minus" root; that is, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~y_p</math> </td> <td align="center"> <math>~\equiv</math> </td> <td align="left"> <math>~\biggl[ \frac{\cos\theta}{c^2 \kappa^2} \biggr]\biggl\{\biggl[z_0^2 \sin^2\theta + c^2 \kappa^2 (c^2 - z_0^2 ) \biggr]^{1 / 2} - z_0 \sin\theta \biggr\} \, ,</math> </td> </tr> <tr> <td align="right"> <math>~y_m</math> </td> <td align="center"> <math>~\equiv</math> </td> <td align="left"> <math>~- \biggl[ \frac{\cos\theta}{c^2 \kappa^2} \biggr]\biggl\{\biggl[z_0^2 \sin^2\theta + c^2 \kappa^2 (c^2 - z_0^2 ) \biggr]^{1 / 2} + z_0 \sin\theta \biggr\} \, .</math> </td> </tr> </table> <table border="1" align="center" cellpadding="8" width="80%"> <tr> <td align="left"> <ul> <li>If tanθ is positive … <ul> <li>Quadrant 1 ⇒ both sinθ and cosθ are positive.</li> <li>Quadrant 3 ⇒ both sinθ and cosθ are negative.</li> </ul> </li> </ul> <ul> <li>If tanθ is negative … <ul> <li>Quadrant 2 ⇒ sinθ is positive but cosθ is negative.</li> <li>Quadrant 4 ⇒ sinθ is negative while cosθ are positive.</li> </ul> </li> </ul> Taking numerical values from our [[#Riemann_Flow|chosen Example Model]] — and using z<sub>0</sub> = ± 0.25 as our 1<sup>st</sup> test cases — we have: <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\tan\theta</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ -\frac{\beta\Omega_2}{\gamma \Omega_3} = -0.344793 ~~~\Rightarrow~~~ \theta = -19.0238^\circ \, . </math> </td> </tr> <tr> <td align="right"> <math>~\kappa^2</math> </td> <td align="center"> <math>~\equiv</math> </td> <td align="left"> <math>~ \frac{c^2 \cos^2\theta + b^2 \sin^2\theta}{b^2c^2} = 1.05238\, . </math> </td> </tr> <tr> <td align="right"> <math>~\mathrm{TERM1}</math> </td> <td align="center"> <math>~\equiv</math> </td> <td align="left"> <math>~z_0^2 \sin^2\theta + c^2\kappa^2(c^2-z_0^2) =0.043577 </math> (for z<sub>0</sub> = ± 0.25). </td> </tr> </table> z<sub>0</sub> = +0.25 and θ in QUADRANT #4 (sinθ is negative while cosθ is positive): <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~y_p</math> </td> <td align="center"> <math>~\equiv</math> </td> <td align="left"> <math>~\biggl[ \frac{\cos\theta}{c^2 \kappa^2} \biggr]\biggl\{\biggl[ \mathrm{TERM1} \biggr]^{1 / 2} - z_0 \sin\theta \biggr\} = 1.1788 \, ,</math> </td> </tr> <tr> <td align="right"> <math>~y_m</math> </td> <td align="center"> <math>~\equiv</math> </td> <td align="left"> <math>~- \biggl[ \frac{\cos\theta}{c^2 \kappa^2} \biggr]\biggl\{\biggl[ \mathrm{TERM1} \biggr]^{1 / 2} + z_0 \sin\theta \biggr\} = - 0.5169 \, .</math> </td> </tr> <tr> <td align="right"> <math>~z_p</math> </td> <td align="center"> <math>~\equiv</math> </td> <td align="left"> <math>~-c \biggl[ 1 - \biggl( \frac{y_p}{b} \biggr)^2 \biggr]^{1 / 2} = -0.15645 \, ,</math> </td> </tr> <tr> <td align="right"> <math>~z_m</math> </td> <td align="center"> <math>~\equiv</math> </td> <td align="left"> <math>~c \biggl[ 1 - \biggl( \frac{y_m}{b} \biggr)^2 \biggr]^{1 / 2} = 0.42821 \, ,</math> </td> </tr> </table> </td> <td align="center"> <table border="1" align="center" cellpadding="5"> <tr> <td align="center" colspan="5"><math>~|z_0|_\mathrm{max} = 0.63792</math></td> </tr> <tr> <td align="center"><math>~z_0</math></td> <td align="center"><math>~y_p</math></td> <td align="center"><math>~z_p</math></td> <td align="center"><math>~y_m</math></td> <td align="center"><math>~z_m</math></td> </tr> <tr> <td align="right"><math>~+ 0.6379</math></td> <td align="right"><math>~+ 0.8511</math></td> <td align="right"><math>~+ 0.3444</math></td> <td align="right"><math>~+ 0.8379</math></td> <td align="right"><math>~+ 0.3490</math></td> </tr> <tr> <td align="right"><math>~+ 0.60</math></td> <td align="right"><math>~+ 1.1073</math></td> <td align="right"><math>~+ 0.2182</math></td> <td align="right"><math>~+ 0.4814</math></td> <td align="right"><math>~+ 0.4340</math></td> </tr> <tr> <td align="right"><math>~+ 0.55</math></td> <td align="right"><math>~+ 1.1950</math></td> <td align="right"><math>~+ 0.1380</math></td> <td align="right"><math>~+ 0.2613</math></td> <td align="right"><math>~+ 0.4599</math></td> </tr> <tr> <td align="right"><math>~+ 0.50</math></td> <td align="right"><math>~+ 1.2342</math></td> <td align="right"><math>~+ 0.0744</math></td> <td align="right"><math>~+ 0.0897</math></td> <td align="right"><math>~+ 0.4691</math></td> </tr> <tr> <td align="right"><math>~+ 0.45</math></td> <td align="right"><math>~+ 1.2489</math></td> <td align="right"><math>~- 0.0194</math></td> <td align="right"><math>~- 0.0574</math></td> <td align="right"><math>~+ 0.4698</math></td> </tr> <tr> <td align="right"><math>~+ 0.40</math></td> <td align="right"><math>~+ 1.2474</math></td> <td align="right"><math>~- 0.0301</math></td> <td align="right"><math>~- 0.1883</math></td> <td align="right"><math>~+ 0.4649</math></td> </tr> <tr> <td align="right"><math>~+ 0.35</math></td> <td align="right"><math>~+ 1.2338</math></td> <td align="right"><math>~- 0.0754</math></td> <td align="right"><math>~- 0.3071</math></td> <td align="right"><math>~+ 0.4559</math></td> </tr> <tr> <td align="right"><math>~+ 0.30</math></td> <td align="right"><math>~+ 1.2105</math></td> <td align="right"><math>~- 0.1174</math></td> <td align="right"><math>~- 0.4161</math></td> <td align="right"><math>~+ 0.4435</math></td> </tr> <tr> <td align="right" bgcolor="orange">+ 0.25</td> <td align="right" bgcolor="orange">+ 1.1788</td> <td align="right" bgcolor="orange">- 0.1564</td> <td align="right" bgcolor="orange">- 0.5169</td> <td align="right" bgcolor="orange">+ 0.4282</td> </tr> <tr> <td align="right"><math>~+ 0.20</math></td> <td align="right"><math>~+ 1.1399</math></td> <td align="right"><math>~- 0.1930</math></td> <td align="right"><math>~- 0.6103</math></td> <td align="right"><math>~+ 0.4104</math></td> </tr> <tr> <td align="right"><math>~+ 0.15</math></td> <td align="right"><math>~+ 1.0943</math></td> <td align="right"><math>~- 0.2273</math></td> <td align="right"><math>~- 0.6971</math></td> <td align="right"><math>~+ 0.3904</math></td> </tr> <tr> <td align="right"><math>~+ 0.10</math></td> <td align="right"><math>~+ 1.0426</math></td> <td align="right"><math>~- 0.2595</math></td> <td align="right"><math>~- 0.7778</math></td> <td align="right"><math>~+ 0.3682</math></td> </tr> <tr> <td align="right"><math>~+ 0.05</math></td> <td align="right"><math>~+ 0.9849</math></td> <td align="right"><math>~- 0.2896</math></td> <td align="right"><math>~- 0.8525</math></td> <td align="right"><math>~+ 0.3439</math></td> </tr> <tr> <td align="right"><math>~+ 0.00</math></td> <td align="right"><math>~+ 0.9216</math></td> <td align="right"><math>~- 0.3177</math></td> <td align="right"><math>~- 0.9216</math></td> <td align="right"><math>~+ 0.3177</math></td> </tr> <tr> <td align="right"><math>~- 0.05</math></td> <td align="right"><math>~+ 0.8525</math></td> <td align="right"><math>~- 0.3439</math></td> <td align="right"><math>~- 0.9849</math></td> <td align="right"><math>~+ 0.2895</math></td> </tr> <tr> <td align="right"><math>~- 0.10</math></td> <td align="right"><math>~+ 0.7778</math></td> <td align="right"><math>~- 0.3682</math></td> <td align="right"><math>~- 1.0426</math></td> <td align="right"><math>~+ 0.2595</math></td> </tr> <tr> <td align="center" colspan="5">''etc.'' </tr> <tr> <td align="right"><math>~- 0.6379</math></td> <td align="right"><math>~- 0.8379</math></td> <td align="right"><math>~- 0.3490</math></td> <td align="right"><math>~- 0.8511</math></td> <td align="right"><math>~- 0.3444</math></td> </tr> </table> </td> </tr> </table> The y-coordinate of the center of the orbit will lie halfway between these two "edges". That is (numerical example given for the case of z<sub>0</sub> = + 0.25), <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~y_\mathrm{center}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\frac{1}{2}\biggl[ y_p + y_m \biggr] = +0.3310 \, .</math> </td> </tr> </table> Correspondingly, the vertical (z) location of the orbit center in the ''body'' frame is given by the expression, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~z_\mathrm{center}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~y_\mathrm{center}\tan\theta + z_0 = +0.1359 \, .</math> </td> </tr> </table> The line that runs parallel to the x-axis — lies perpendicular to the y-z plane — and that passes through this "center" location intersects the surface of the ellipsoid at a value of x that is obtained by plugging <math>~y_\mathrm{center}</math> into the ''Intersection Expression''. That is, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\frac{x_\mathrm{surf}}{a}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\biggl\{ 1 - y^2_\mathrm{center} \biggl[\frac{\kappa^2}{\cos^2\theta} \biggr] - y_\mathrm{center} \biggl[ \frac{2z_0 \tan\theta}{c^2} \biggr] - \frac{z_0^2}{c^2} \biggr\}^{1 / 2} = 0.92001 \, ;</math> </td> </tr> </table> along the relevant orbit, this is also the maximum value of x. ===Tipped Plane=== We use the expressions in the right panel of [[#Fig1|Figure 1, above]] to transform (x, y, z) ''body'' coordinates to (x', y', z') ''tipped-frame'' coordiantes. Given that <math>~x' = x</math>, we appreciate that the x'-coordinate of the orbit center is zero, and the maximum value <math>~(x'_\mathrm{surf})</math> that is encountered along the relevant orbit is the same as the value of <math>~x_\mathrm{surf}</math> as determined in the ''body'' (unprimed) frame. The z'-coordinate of the orbit center is, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~z'_\mathrm{center}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ (z_\mathrm{center} - z_0)\cos\theta - y_\mathrm{center}\sin\theta </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ (y_\mathrm{center}\tan\theta) \cos\theta - y_\mathrm{center}\sin\theta </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ 0 \, . </math> </td> </tr> </table> Finally, in the ''tipped'' plane, the maximum (subscript_p) and minimum (subscript_m) values of y' are, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~y'_p</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ (z_p - z_0)\sin\theta + y_p\cos\theta = 1.2469 \, , </math> </td> </tr> <tr> <td align="right"> <math>~y'_m</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ (z_m - z_0)\sin\theta + y_m\cos\theta = -0.5467 \, , </math> </td> </tr> <tr> <td align="right"> <math>~\Rightarrow ~~~ y'_\mathrm{center}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \frac{1}{2}\biggl[ y_p' + y_m'\biggr] = 0.3501\, . </math> </td> </tr> <tr> <td align="right"> <math>~\Rightarrow ~~~ y'_\mathrm{surf}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ y'_p - y'_\mathrm{center} = 0.8968\, . </math> </td> </tr> </table> So, in the ''tipped'', x'-y' plane, the elliptical orbit that corresponds to z<sub>0</sub> = + 0.25 should be described by the expression, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~1</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \biggl[\frac{x'}{x_\mathrm{surf}} \biggr]^2 + \biggl[ \frac{(y' - y'_\mathrm{center} ) }{y'_\mathrm{surf}} \biggr]^2 \, . </math> </td> </tr> </table> NOTE: * <math>~y'_\mathrm{center}/z_0 = 0.350096/0.25 = 1.40038 \, .</math> * <math>~x_\mathrm{surf}/y'_\mathrm{surf} = 0.92001/0.896819 = 1.0259 \, .</math> At a minimum these numerical values should be compared to the Riemann model parameters [[ThreeDimensionalConfigurations/ChallengesPt2#Example_Equilibrium_Model|computed in our earlier (Pt. 2) examination]].
Summary:
Please note that all contributions to JETohlineWiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
JETohlineWiki:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Navigation menu
Personal tools
Not logged in
Talk
Contributions
Log in
Namespaces
Page
Discussion
English
Views
Read
Edit
View history
More
Search
Navigation
Main page
Tiled Menu
Table of Contents
Old (VisTrails) Cover
Appendices
Variables & Parameters
Key Equations
Special Functions
Permissions
Formats
References
lsuPhys
Ramblings
Uploaded Images
Originals
Recent changes
Random page
Help about MediaWiki
Tools
What links here
Related changes
Special pages
Page information