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__FORCETOC__ 

=Files on LSU P&A Servers=

==Primary Web==
public_html = /opt1/usrlocal/apache2/htdocs/graceland/faculty/tohline = [http://www.phys.lsuedu/faculty/tohline http://www.phys.lsu.edu/faculty/tohline] …

===HOMEPAGE RELEVANT1===
<ul>
<li>
index.html
</li>
<li>
indexhtv.html: Homepage prior to "accessibility statement" added by htv (Hortensia)
</li>
<li>
indexMarch2011.html
</li>
<li>
biosketch.html
</li>
<li>
courses.html: Also see "courses" directory, below
</li>
<li>
faculty.awards.html: explains what an Alumni Professorship is
</li>
<li>
features.html: lists featured work
</li>
<li>
publications.html: Older version of ref_ref.html
</li>
<li>
ref_index.html
</li>
<li>
ref_IPAM2005.html
</li>
<li>
ref_movies.html
</li>
<li>
ref_ref.html
</li>
<li>
research.html
</li>
<li>
resume.html
</li>
<li>
students.html
</li>
<li>
mission.html
</li>
<li>
resume0.html
</li>
<li>
ref0_index.html
</li>
<li>
ref0_ref.html
</li>
<li>
PDF-formatted …

<ul>
<li>
resume.forpdf.html
</li>
<li>
resume01.forpdf.html
</li>
<li>
resume02.forpdf.html
</li>
<li>
resume08.forpdf.html
</li>
<li>
ref_ref.forpdf.html
</li>
<li>
ref_ref.forpdf06.html
</li>
<li>
ref_ref.forpdf07.html
</li>
<li>
ref_ref.forpdf08.html
</li>
<li>
research.forpdf.html
</li>
</ul>
</li>
<li>
t.html: (circa 2006) Single-page statement of research interests and relevant publications
</li>
<li>
test.html: very early draft of homepage layout, including one of Andalib's binary vector flows
</li>
<li>
test2.html: very early draft of homepage layout
</li>
</ul>

===MOVIE ENSEMBLES1===
<ul>
<li>
image.ensemble: TERRIFIC image-mosaic pointing to more than "Astrophysics Movies" (most links point to descriptions listed below on our Secondary Web MOVIE ENSEMBLES category)
</li>
</ul>

===DIRECTORIES1===
<ul>
<li>
aasvideo2006: Simply points to subdirectory … tohline/astroph/dmtf05/
</li>
<li>
Appendices
</li>
<li>
Applications
arribas: OBJ files prepared in effort to solicit "Micky Mouse" glass solid rectangle from Arribas
</li>
<li>
astr1102.04
</li>
<li>
astr4222
</li>
<li>
astrophysics
</li>
<li>
BPFest:
</li>
<li>
capital
</li>
<li>
CHEGA
</li>
<li>
CIP
</li>
<li>
cise: Fledgling effort to construct "astrophysics portal" for CISE magazine
</li>
<li>
CISE
</li>
<li>
clayton
</li>
<li>
Context
</li>
<li>
courses
</li>
<li>
grbcollaboration
</li>
<li>
GRBcollaboration
</li>
<li>
GRsources
</li>
<li>
honors
</li>
<li>
idesk
</li>
<li>
Interim2001
</li>
<li>
Landolt
</li>
<li>
ligo
</li>
<li>
lisa6
</li>
<li>
lsulogos
</li>
<li>
movies
</li>
<li>
MRAC_2007
</li>
<li>
NAVO
</li>
<li>
NCSA
</li>
<li>
SDSC
</li>
<li>
NPACI98
</li>
<li>
NRAC98.proposal
</li>
<li>
NRAC99
</li>
<li>
NRAC_2000
</li>
<li>
NRAC_2001
</li>
<li>
NRAC_2002
</li>
<li>
NRAC_2004
</li>
<li>
NRAC_2005
</li>
<li>
NRC_rankings
</li>
<li>
NSF99
</li>
<li>
NSF02
</li>
<li>
NSF03
</li>
<li>
oldcommittees
</li>
<li>
oldpdfs
</li>
<li>
oldwebpages
</li>
<li>
papers
</li>
<li>
PHYS2411
</li>
<li>
phys4412
</li>
<li>
PHYS7412
</li>
<li>
phys7741
</li>
<li>
pulling
</li>
<li>
rmode/
<ul>
<li>
index explaining how r-mode movie was rendered: [http://www.phys.lsu.edu/faculty/tohline/rmode/index.html http://www.phys.lsu.edu/faculty/tohline/rmode/index.html]
</li>
<li>
FINAL 3D movie (circa 2000): [http://www.phys.lsu.edu/faculty/tohline/rmode/final.mov http://www.phys.lsu.edu/faculty/tohline/rmode/final.mov] (6,848K)
</li>
<li>
mpg-version of FINAL 3D movie: [http://www.phys.lsu.edu/faculty/tohline/rmode/rmode.waveshort.mpg http://www.phys.lsu.edu/faculty/tohline/rmode/rmode.waveshort.mpg] (1,812K)
</li>
<li>
zebra imaging/
<ul>
<li>Plan to enlist holographic-imaging capabilities offered by Zebra Imaging/: [http://www.phys.lsu.edu/faculty/tohline/rmode/zebraimaging/index.html http://www.phys.lsu.edu/faculty/tohline/rmode/zebraimaging/index.html]</li>
<li>(circa 2001) Four "sdl" files, along with a template sdl file, define four iso-density files from mode movie frame #290</li>
</ul>
</li>
</ul>
<li>
sabbatical
</li>
<li>
Sci-Tech
</li>
<li>
sources
</li>
<li>
sph-grid
</li>
<li>
Talks
</li>
<li>
Talks_Additional
</li>
<li>
temp
</li>
<li>
vistrails
</li>
<li>
vita
</li>
<li>
web intro
</li>
<li>
whyOOP
</li>
<li>
www.cise.org
</li>
<li>
youtube
</li>

</ul>

===GRAD STUDENTS1===
<ul>
<li>
barnes/
</li>
<li>
motl/
</li>
<li>
ou/
</li>
<li>
valencia.html
</li>
</ul>

===IMAGES1===
<ul>
<li>
ballgreen.gif
</li>
<li>
greenbullet.gif
</li>
<li>
horizon.line.gif
</li>
<li>
merger.oneil.mpeg
</li>
<li>
pics/
</li>
<li>
purplebullet.gif
</li>
<li>
rmode.final.mpeg: presumably the same as "mode.waveshort.mpg" as described above under the "mode" DIRECTORY YouTube posting: rmode.final.mpeg
</li>
<li>
saied.stream.gif
</li>
<li>
saied.vel1.gif
</li>
<li>
stable.gif
</li>
<li>
tohline.jpg
</li>
<li>
tohline.old.gif
</li>
<li>
rhoT.final.pdf: Figure for 2001 ARAA review article
</li>
<li>
rhoT.final.ps: Figure for 2001 ARAA review article
</li>
</ul>

===OTHER FILES1===
<ul>
<li>
fission.movies.htmls: detailed overview of (primarily) dissertation work by John Cazes
</li>
<li>
HDmovies.html: (circa 2008) Explaining need to feed broadcast HDTV format
</li>
<li>
html.documents.html: list (prior to 2005) of talks/papers/proposals inHTML format
</li>
<li>
meaganISEF.html: A thank-you note from Meagan Messina dated 5/16/2000
</li>
<li>
out1
</li>
<li>
Quicktime.html: (circa 2005) detailed overview of steps used to generate a Quicktime animation sequence
</li>
<li>
realtime.html (circa 2005) detailed estimate of feasibility of real-time analysis (e.g., inside CAVE) of 3D DFD flows
</li>
<li>
symbol.html: Early draft of H_Book page giving PGEs in spherical symmetry
</li>
<li>
T3E.timings.html: Points to same file name inside "SDSC" directory
</li>
<li>
TinsleyNotes1978.pdf
</li>
<li>
Tohline_Dissertation.pdf
</li>
<li>
valtech.html: (circa 1999) John Woodward's company?

</li>
</ul>

==Secondary Web==

/opt1/usrlocal/apache2/htdocs/graceland/projs/astro = [http://www.phys.lsu.edu/astro/ http://www.phys.lsu.edu/astro/] …

===H_BOOK RELEVANT===
<ul>
<li>
H_Book.current/H_Book.html
</li>
</ul>

===MOVIE ENSEMBLES2===
<ul>
<li>
movie.index.html:Movies produced by LSU's Astrophysics Theory Group
<ul>
<li>(see below) cazes/dodconf/hce.html</li>
<li>
movie_captions/
<ul>
<li>motl.binary.html: Dynamics of Mass-Transferring Binary Star Systems</li>
<li>fission.html: The Fission Mechanism for Binary Star Formation</li>
<li>cares.html: Compressible Analogs of Riemann Ellipsoids (CAREs)</li>
<li>two-armed_spiral.html: Two-Armed, Spiral-Mode Instability</li>
<li>Andalib.html: Nonaxisymmetric, Self-Gravitating Disks with Uniform Vortensity</li>
<li>pp_instability.html: Papaloizou-Pringle Instability</li>
<li>equal mass.binary.html: The Relative Stability of Close, Equal-Mass Binaries</li>
</ul>
</li>
</ul>
</li>
</ul>

===DIRECTORIES2===
<ul>
<li>
barmode/index.html: EXCELLENT collection of 10 movies — along with short captions — of Cazes' simulations
</li>
<li>
cip/: Contains "clickable map" for talk found below in Cazes/dodconf/hce.html
</li>
<li>
Drexel/
</li>
<li>
movies/: includes subdirectory with early "motl" movies
</li>
<li>
nap98/bf.final.lasp.html: Contains movie (movie4 ?) showing Lagrangian particle motions in four of Andalib's models
</li>
<li>
network_database/ Defunct attempt (circa 1998) to create an interactive database of physics department computers
</li>
<li>
tohline/ Contains primarily java/perl/fortran scripts to support active elements of early H_Book effort (circa 1997 with, e.g., Sherfessee & Muffoletto)

</li>
</ul>

===GRAD STUDENTS2===
<ul>
<li>
cazes/
<ul>
<li>dodconf/hce.html: Heterogeneous Computing Environment to …</li>
<li>LSU.at.SDSC.html: Hydrocode timings in (circa 1996) proposal for T3E time at SDSC</li>
<li>tohline_NRAC98/ … includes the following seven Andalib velocity maps
<table border="1" align="center" cellpadding="3">
<tr>
<td align="center">Filename</td>
<td align="center">vel05</td>
<td align="center">vel12</td>
<td align="center">vel14</td>
<td align="center">vel20</td>
<td align="center">vel30</td>
<td align="center">vel36</td>
<td align="center">vel43</td>
</tr>

<tr>
<td align="center">Thumbnail</td>
<td align="center"> </td>
<td align="center"> </td>
<td align="center"> </td>
<td align="center"> </td>
<td align="center"> </td>
<td align="center"> </td>
<td align="center"> </td>
</tr>

<tr>
<td align="center">Model No.</td>
<td align="center">??</td>
<td align="center">??</td>
<td align="center">D13</td>
<td align="center">D14</td>
<td align="center">—</td>
<td align="center">—</td>
<td align="center">C13(?)</td>
</tr>

<tr>
<td align="center">Fig. No. </td>
<td align="center">??</td>
<td align="center">??</td>
<td align="center">5.16</td>
<td align="center">5.15</td>
<td align="center">5.14</td>
<td align="center">5.13</td>
<td align="center">5.6(?)</td>
</tr>
</table>
</li>
<li>LOTS! of other good stuff</li>
</ul>
</li>
<li>
fisher/
</li>
<li>
howie/
</li>
<li>
motl/
</li>
<li>
paul/

</li>
</ul>

===IMAGES2===
<ul>
<li>
m = 2 instability in PP torus …
<ul>
<li>bar.mpg: Instability in PP torus</li>
<li>joel.mpg: (same as bar.mpg)</li>
<li>joelmov.gif: (larger) animation of instability in PP torus</li>
<li>barman.gif: animation of instability in PP torus</li>
</ul>
</li>
<li>
fig3.jpg: key figure ensemble from Cazes' dissertation
<li>
Flyby of tilted-ring, warped galaxy disk …
<ul>
<li>gal.mpg: Excellent flyby of "tilted disk" model</li>
<li>glamor.gif: Crude resolution "tilted disk" animation ???</li>
</ul>
</li>
<li>
icon.gif: Crude resolution of bar instability (2D eq. plane)
</li>
<li>
splash.mpg: Neat animation of non equilibrium binary
</li>
<li>
Sample of binary-merger animations from Kim New's research
<ul>
<li>hydro.mpg: Early movie segment of WD mass-transfer and merger</li>
<li>kimmo.gif: (medium) animation of detached binary</li>
<li>merger.mov</li>
<li>merger.mpg</li>
<li>merger.old.mpg</li>
<li>mergermov.gif: (medium) animation of (WD?) binary merger</li>
<li>ns.mergemov.gif</li>
<li>ns.mergemov.gs.gif</li>
<li>ns.merger.gs.mpg</li>
<li>ns.merger.mpg</li>
</ul>
</li>
<li>
Settling of thin galaxy disk from Paul Fisher's research …
<ul>
<li>paul.mpg</li>
<li>paulmov.gif: (small) animation of thin disk settling</li>
</ul>
</li>
</ul>

===OTHER FILES2===
<ul>
<li>
home.html: Same as "index.html"
</li>
<li>
home.old.html: TERRIFIC! includes links to long-lost mpg movies; load in Chrome rather than Safari
</li>
<li>
index.html: Crude home page for "Astrophysics Theory Group" at LSU
</li>
<li>
tohline.html: Old (circa 1996) home page
</li>
<li>
A (circa 1998) perl (?) script to search web documents; we attached this to an early version of H_Book …
<ul>
<li>websearch.footer.txt</li>
<li>websearch.header.txt</li>
<li>websearch.pl</li>
</ul>
</li>
</ul>

==Tertiary Web==

public = /opt1/usrlocal/apache2/htdocs/tohline = [http://phys.lsu.edu/tohline/ http://phys.lsu.edu/tohline/] …

===DIRECTORIES3===
The files in these directories primarily contain (circa 2006) XML-formatted attempts to present instructional material that contains many nontrivial mathematical expressions.
<ul>
<li>
COLLADA/    <-- ''circa'' 2021
</li>
<li>
Gifs/
</li>
<li>
HBook/
</li>
<li>
IGERT/
</li>
<li>
New/
</li>
</ul>

===FILES3===
<ul>
<li>
LSUAEI.movies.html
<ul>
<li>Two r-mode movies: Pt. 1 = www.phys.lsu.edu/faculty/tohline/rmode/surface.mov; and Pt. 2 = (same)/rmode/final.mov</li>
<li>Two "Ou" dynamical barmode movies. Neither accessible, as their addresses are paris.phys.lsu.edu/~ou</li>
<li>Four "D'Souza" binary mass-transfer movies. None accessible, as their addresses are paris.phys.lsu.edu/~mario</li>
</ul>
</li>
<li>
LSUAEI.talk.pdf
</li>
<li>
LSUAEI.talk.ppt
</li>
<li>
TalkSantaFe.ppt
</li>
</ul>

=YouTube=
==Movies Already Uploaded==
===BAR-MODE INSTABILITY===
<ul>
<li>
''Model A'' Classic, two-armed spiral: www.phys.lsu.edu/astro/nap98/movies/movie1.mov (5,907K) 
YouTube id = [https://www.youtube.com/watch?v=BhRUqZe0Ly4 BhRUqZe0Ly4]
</li>
<li>
''Model A'' Initially uniform vortensity: www.phys.lsu.edu/astro/barmode/movies/modelB.spiral.mov (7.7M) 
YouTube id = [https://www.youtube.com/watch?v=Qh-bMto2e3k Qh-bMto2e3k]
</li>
<li>

</li>
</ul>

===COMPRESSIBLE ANALOGS OF RIEMANN ELLIPSOIDS===
<ul>
<li>
''Model A'' Steady-state: www.phys.lsu.edu/astro/barmode/movies/modelA.steady.mov (7,169K) 
YouTube id = [https://www.youtube.com/watch?v=z3RDthHnY3A z3RDthHnY3A]
</li>
<li>
''Model A'' Equatorial Flow: www.phys.lsu.edu/astro/nap98/movies/movie2.mov (5.94M) 
YouTube id = [https://www.youtube.com/watch?v=fgjjzu3Nmo8 fgjjzu3Nmo8] — ''Japan's National Astronomical Observatory'' poster mounted on the wall
</li>
<li>
''Model A'' Meridional Flow: www.phys.lsu.edu/astro/nap98/movies/movie3.mov (3.5M) 
YouTube id = [https://www.youtube.com/watch?v=_nXKv0k0h-Q _nXKv0k0h-Q] — ''Japan's National Astronomical Observatory'' poster mounted on the wall
</li>
<li>
''Model B'' Steady-state: www.phys.lsu.edu/astro/barmode/movies/modelB.steady.mov (14.1M) 
YouTube id = [https://www.youtube.com/watch?v=Eyl81O9s62s Eyl81O9s62s]
</li>
<li>
''Model B'' Equatorial Flow: www.phys.lsu.edu/astro/barmode/movies/bar_uv.mov (5,976K) 
YouTube id = [https://www.youtube.com/watch?v=yggbz9z8JQ4 yggbz9z8JQ4] — ''U. S. National Science Foundation'' wall poster
</li>
<li>
''Andalib's'' Equatorial flow: www.phys.lsu.edu/astro/cip/movie2.mov (5.9M) 
YouTube id = [https://www.youtube.com/watch?v=p550IDP8h-s p550IDP8h-s] — ''Computers in Physics'' wall poster
</li>
<li>
''Four Andalib'' Models: www.phys.lsu.edu/astro/nap98/movies/movie4.mov (7.1M) 
YouTube id = [https://www.youtube.com/watch?v=cCfLmitM7bc cCfLmitM7bc] — ''Japan's National Astronomical Observatory'' poster mounted on the wall
</li>
</ul>

===COOLING + FISSION (?)===
<ul>
<li>
Cooling evolution: www.phys.lsu.edu/astro/barmode/movies/binary.form.mov (8,514K) 
YouTube id = [https://www.youtube.com/watch?v=erYWHgaKYyc erYWHgaKYyc]
</li>
<li>
Equatorial "Binary" Flow: www.phys.lsu.edu/astro/cazes/dodconf/movies/movie3.mov (4,712K) 
YouTube id = [https://www.youtube.com/watch?v=nC4adQzlXrI nC4adQzlXrI] — ''MSRC'' wall poster
</li>
<li>
Meridional "Binary" Flow: www.phys.lsu.edu/astro/cazes/dodconf/movies/movie4.mov (3,375K) 
YouTube id = [https://www.youtube.com/watch?v=S0tg2jURzGE S0tg2jURzGE] — ''MSRC'' wall poster
</li>
<li>
Andalib "Binary" Model: www.phys.lsu.edu/astro/barmode/movies/bin_sa.mov (5,725K) 
YouTube id = [https://www.youtube.com/watch?v=nkwRJh2tgos nkwRJh2tgos] — ''MSRC'' wall poster
</li>
</ul>

===NEUTRON STAR r-MODE INSTABILITY===
<ul>
<li>
Nonlinear development of r-mode instability in a neutron star: Mac … TransitionPC_V01/Videos/YouTube/rmode.final.mpeg (1.9M) 
YouTube id = [https://www.youtube.com/watch?v=i2zBvA7c7i8 i2zBvA7c7i8]
</li>
</ul>

===ELLIPTICAL INSTABILITY===
<ul>
<li>
Nonlinear development of an elliptical instability in a rotating bar: Mac … TransitionPC_V01/Videos/YouTube/fmode.b181.helix.gr_off.mov (9.8M) 
YouTube id = [https://www.youtube.com/watch?v=Fi8Fp26uc-g Fi8Fp26uc-g]
</li>
</ul>

===MASS-TRANSFERRING BINARY STAR SYSTEM===
<ul>
<li>
Example of mass-transferring binary star system, similar to a white-dwarf binary: Mac … TransitionPC_V01/Videos/YouTube/Q0.4D.mov (74.3M) 
YouTube id = [https://www.youtube.com/watch?v=lFR5S_Fc-9w&list=PLjCUvbPxed2S9vmjCl2tkol06_QF2So-T lFR5S_Fc-9w&list=PLjCUvbPxed2S9vmjCl2tkol06_QF2So-T] 
EXCELLENT! This movie shows nonlinear-amplitude pumping of m = 3, 4, 5 modes on the accretor. 
</li>
<li>
Same mass-transferring binary star system, but showing only the fluid from the donor star: Mac … TransitionPC_V01/Videos/YouTube/q0.4_hires_donor.mov (5.6M) 
YouTube id = [https://www.youtube.com/watch?v=pxjhuR0BsE0 pxjhuR0BsE0]
</li>
</ul>

===SETTLING DISK===
<ul>
<li>
Paul Fisher's settling galaxy disk (''circa'' 1999): www.phys.lsu.edu/astro/barmode/paul.mpg (69K) 
YouTube id = [https://www.youtube.com/watch?v=yxOLu03T1yE yxOLu03T1yE]
</li>
</ul>

==Movies to be Uploaded==
''None'' at the present time.

=See Also=

{{ SGFfooter }}

Appendix/Ramblings/myPhys - Revision history