Editing
Appendix/Ramblings/ToHadleyAndImamura
(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!
====His Derived Eigenfunction==== Via an analytic perturbation analysis, [http://adsabs.harvard.edu/abs/1985MNRAS.216..553B Blaes (1985)] shows that, in slender PP tori with uniform specific angular momentum, the spatial structure of unstable modes can be expressed as, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\frac{W(\eta,\theta)}{W_0} -1</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\biggl\{ f_m(\eta,\theta)e^{-i[m\phi + k\theta]} \biggr\} \, ,</math> </td> </tr> </table> </div> where (see his equation 1.10), <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~f_m(\eta,\theta)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math> ~\beta^2 m^2 \biggl[ 2\eta^2 \cos^2\theta - \frac{3\eta^2}{4(n+1)} - \frac{(4n+1)}{4(n+1)^2} \pm 4i\biggl(\frac{3}{2n+2}\biggr)^{1/2} \eta\cos\theta\biggr] + \mathcal{O}(\beta^3) \, . </math> </td> </tr> </table> </div> In this expression, <math>~n</math> is the polytropic index, and <math>~\beta</math> is a dimensionless parameter that specifies the relative thickness of the torus; specifically, in terms of the ratio of the inner-to-outer edge of the torus, <math>~r_-/r_+</math>, <div align="center"> <math>~\beta \equiv \frac{1- r_-/r_+}{1+ r_-/r_+} \, .</math> </div> Notice that this eigenfunction derived by [http://adsabs.harvard.edu/abs/1985MNRAS.216..553B Blaes (1985)] describes a spatial perturbation that is not confined to the equatorial plane of the torus. The parameter pair, <math>~(\eta,\theta)</math>, defines a two-dimensional, polar coordinate system in a plane lying perpendicular to the equatorial plane that contains the torus's (nearly circular) cross-section: <math>~\eta</math> is a dimensionless radial coordinate measuring distance from the center of the cross-section — <math>~\eta = 0</math> at the center of the cross-section and <math>~\eta = 1</math> at the surface of the torus; and <math>~\theta</math> is the polar-coordinate oriented such that <math>~\theta = 0</math> points toward the "inner" edge of the torus, <math>~\theta = \pi/2</math> points vertically, straight "up," and <math>~\theta = \pi</math> points toward the "outer" edge of the torus. Paralleling the [[#Generic_Formulation|generic formulation that has just been discussed]], this is a complex function having, to lowest order, the following real and imaginary parts: <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\mathcal{A}_\mathrm{Blaes}(\eta,\theta)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~(\beta m)^2\biggl[ 2\eta^2 \cos^2\theta - \frac{3\eta^2}{4(n+1)} - \frac{(4n+1)}{4(n+1)^2} \biggr] </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\frac{ (\beta m)^2}{4(n+1)^2}\biggl\{ ~[8(n+1)\cos^2\theta - 3]\eta^2 (n+1) - (4n+1) \biggr\} \, ; </math> </td> </tr> <tr> <td align="right"> <math>~\mathcal{B}_\mathrm{Blaes}(\eta,\theta)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ 4(\beta m)^2\biggl(\frac{3}{2n+2}\biggr)^{1/2} \eta\cos\theta </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\frac{(\beta m)^2}{4(n+1)^2}\biggl[2^7\cdot 3(n+1)^3 \eta^2\cos^2\theta \biggr]^{1/2}\, . </math> </td> </tr> </table> </div> We should therefore find that the amplitude (modulus) of the perturbation is, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\biggl|\frac{W}{W_0} -1\biggr|</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\sqrt{\mathcal{A}_\mathrm{Blaes}^2+ \mathcal{B}_\mathrm{Blaes}^2} \, ;</math> </td> </tr> </table> </div> and the associated "constant phase locus" should be identified by the function, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~m\phi_\mathrm{max}(\eta,\theta)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \tan^{-1}\biggl[ \frac{\mathcal{A}_\mathrm{Blaes}}{\mathcal{B}_\mathrm{Blaes}} \biggr] - k\theta \, .</math> </td> </tr> </table> </div> <!-- OLD, INCORRECT DESCRIPTION THAT IGNORES LEADING "1" IN DEFINITION OF REAL COMPONENT... <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~f_m(\eta,\theta)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math> ~\beta^2 m^2 \biggl[ 2\eta^2 \cos^2\theta - \frac{3\eta^2}{4(n+1)} - \frac{(4n+1)}{4(n+1)^2} \pm 4i\biggl(\frac{3}{2n+2}\biggr)^{1/2} \eta\cos\theta\biggr] + \mathcal{O}(\beta^3) \, . </math> </td> </tr> </table> </div> In this expression, <math>~n</math> is the polytropic index, and <math>~\beta</math> is a dimensionless parameter that specifies the relative thickness of the torus; specifically, in terms of the ratio of the inner-to-outer edge of the torus, <math>~r_-/r_+</math>, <div align="center"> <math>~\beta \equiv \frac{1- r_-/r_+}{1+ r_-/r_+} \, .</math> </div> Notice that this eigenfunction derived by [http://adsabs.harvard.edu/abs/1985MNRAS.216..553B Blaes (1985)] describes a spatial perturbation that is not confined to the equatorial plane of the torus. The parameter pair, <math>~(\eta,\theta)</math>, defines a two-dimensional, polar coordinate system in a plane lying perpendicular to the equatorial plane that contains the torus's (nearly circular) cross-section: <math>~\eta</math> is a dimensionless radial coordinate measuring distance from the center of the cross-section — <math>~\eta = 0</math> at the center of the cross-section and <math>~\eta = 1</math> at the surface of the torus; and <math>~\theta</math> is the polar-coordinate oriented such that <math>~\theta = 0</math> points toward the "inner" edge of the torus, <math>~\theta = \pi/2</math> points vertically, straight "up," and <math>~\theta = \pi</math> points toward the "outer" edge of the torus. Paralleling the [[#Generic_Formulation|generic formulation that has just been discussed]], this is a complex function having, to lowest order, the following real and imaginary parts: <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\mathcal{A}(\eta,\theta)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math> ~2\eta^2 \cos^2\theta - \frac{3\eta^2}{4(n+1)} - \frac{(4n+1)}{4(n+1)^2} </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\frac{1}{4(n+1)^2}\biggl\{ ~[8(n+1)\cos^2\theta - 3]\eta^2 (n+1) - (4n+1) \biggr\} \, ; </math> </td> </tr> <tr> <td align="right"> <math>~\mathcal{B}(\eta,\theta)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ 4\biggl(\frac{3}{2n+2}\biggr)^{1/2} \eta\cos\theta </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\frac{1}{4(n+1)^2}\biggl[2^7\cdot 3(n+1)^3 \eta^2\cos^2\theta \biggr]^{1/2}\, . </math> </td> </tr> </table> </div> We should therefore find that the amplitude (modulus) of the enthalpy perturbation is, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\frac{1}{(m\beta)^2}\biggl|\frac{\delta W}{W_0} \biggr|</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\sqrt{\mathcal{A}^2+ \mathcal{B}^2} \, ;</math> </td> </tr> </table> </div> and the associated "constant phase locus" should be identified by the function, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~m\phi_\mathrm{max}(\eta,\theta)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \tan^{-1}\biggl[ \frac{\mathcal{A}}{\mathcal{B}} \biggr] - k\theta \, .</math> </td> </tr> </table> </div> END OLD INCORRECT DESCRIPTION -->
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