Editing
Appendix/Ramblings/MyDoctoralStudents
(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!
===Years 1982 - 1988=== <!-- 1982 - 1988 --> <table border="0" align="center" width="100%" cellpadding="2"> <tr> <td align="center" width="91%" colspan="3"> </td> <td align="center">[http://www.phys.lsu.edu/~tohline/ref_ref.html Pubs.] <font color="red">(rank)</font></td> </tr> <tr> <td align="right" rowspan="3" width="2%"> </td> <td align="center" bgcolor="lightblue" width="4%"> </td> <td align="left" width="85%"> During his first half-a-dozen years on the faculty at LSU, Tohline continued to work closely with Richard Durisen (Indiana University) to examine the onset and nonlinear development of nonaxisymmetric instabilities in differentially rotating polytropes. <font color="red">Harold A. Williams</font> joined this effort as a graduate student in Tohline's group. He broadened the study to include configurations having a range of compressibility and different distributions of angular momentum; this became the central thrust of his doctoral dissertation. Williams also advanced the capabilities of the group's computational tools by implementing a second-order accurate finite-difference scheme to carry out integrations of the governing hydrodynamic equations. Over this time period, numerical simulations were carried out, to a large extent, on LSU's IBM main-frame computer. But, via [https://www.nsf.gov/awardsearch/showAward?AWD_ID=8818225&HistoricalAwards=false NSF funding], the group also was allocated time on Cray hardware at Minnesota's supercomputer center; Tohline and Williams both received training, for example, on Minnesota's newly acquired [https://en.wikipedia.org/wiki/Cray-2 Cray-2]. <font color="red">Izumi Hachisu</font> (Kyoto University, Japan) joined the group in a postdoctoral research position for a couple of years. Drawing from his own research background, Hachisu provided us with a blueprint for developing a very efficient numerical algorithm for constructing rapidly rotating equilibrium configurations with spheroidal, toroidal, or binary-star geometric shapes — see our [[AxisymmetricConfigurations/HSCF#Hachisu_Self-Consistent-Field_Technique|relevant chapter discussion]]. Over the past several decades, this ''Hachisu Self-Consistent-Field'' technique has allowed us to construct a wide range of different self-gravitation configurations as initial states for stability analyses and for examining the nonlinear growth of unstable modes using computational fluid techniques. </td> <td align="center" rowspan="3"> <p><br /></p> <b>[</b>[https://ui.adsabs.harvard.edu/abs/1985ApJ...298..220T/abstract 19]<b>]</b> <font color="red">(22<sup>nd</sup>)</font><br /> <b>[</b>[https://ui.adsabs.harvard.edu/abs/1987ApJ...315..594W/abstract 22]<b>]</b><br /> <b>[</b>[https://digitalcommons.lsu.edu/gradschool_disstheses/4549/ <math>~\odot</math>]<b>]</b><br /> <p><br /></p> <b>[</b>[https://ui.adsabs.harvard.edu/abs/1987ApJ...323..592H/abstract 25]<b>]</b><br /> <b>[</b>[https://ui.adsabs.harvard.edu/abs/1988ApJS...66..315H/abstract 27]<b>]</b><br /> <b>[</b>[https://ui.adsabs.harvard.edu/abs/1990ApJ...361..394T/abstract 33]<b>]</b> <font color="red">(20<sup>th</sup>)</font><br /> <p><br /></p> <p><br /></p> <b>[</b>[https://ui.adsabs.harvard.edu/abs/1986ApJ...305..281D/abstract 20]<b>]</b> <font color="red">(2<sup>nd</sup>)</font><br /> <p><br /></p> <p><br /></p> <p><br /></p> <p><br /></p> <b>[</b>[http://www.phys.lsu.edu/faculty/tohline/CiSE/CiSE2007.Vol9No6.pdf Viz]<b>]</b><br /> </td> </tr> <tr> <td align="left" bgcolor="yellow"> </td> <td align="left"> A quantitative comparison was made between the results obtained from simulations carried out with two different "finite-difference" CFD codes and one "smoothed particle hydrodynamics" algorithm. </td> </tr> <tr> <td align="left" bgcolor="pink"> </td> <td align="left"> We obtained the Fortran source code of a volume-rendering algorithm that had been developed by [https://www.gc.cuny.edu/Page-Elements/Academics-Research-Centers-Initiatives/Doctoral-Programs/Computer-Science/Faculty-Bios/Gabor-T-Herman?gclid=Cj0KCQjwxMjnBRCtARIsAGwWnBNa_Gr9qORMGErvo8fpEmKvVnTthkpPFZF5mI9RALHtufJ-o6fnUX0aAuUKEALw_wcB Gabor T. Herman] who, at the time, was in the University of Pennsylvania's radiology department. With significant assistance from <font color="red">Monika Lee</font> — our computer systems manager — the code was tuned to execute on the astronomy group's VAX 11/750 and its attached International Imaging System. A string of individual digital images was pieced together to generate animation sequences showing the behavior of our time-evolving fluid systems; this was accomplished by operating in tandem: a Lenco Color Encoder, a Lyon Lamb Mini-VAS animation controller, and a 3/4-inch broadcast-quality Sony U-matic video recorder. <font color="red">Jeffrey E. Anderson</font> — an undergraduate student at LSU (1985-89) — played a key role in operating this set of tools to assist in our analysis of the results of our CFD simulations. </td> </tr> </table>
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