Editing Appendix/lsuPhys

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=IT Help Requested in June 2023=
Over the past several decades I have created and stored hundreds of research-related files on web servers that have been supported/maintained by the LSU Physics &amp; Astronomy IT staff.  Currently the vast majority of these files cannot be accessed via standard web browsers; and currently I am unable to log into and/or edit any of the servers/files.

In the past I was able to access these servers/files as follows:
<ul>
  <li>I would log into "theory.phys.lsu.edu" then &hellip;</li>
  <ul>
  <li>I would "cd" into "public_html", which would take me to <font color="red">/opt1/usrlocal/apache2/htdocs/graceland/faculty/tohline</font></li>
  <li>Many of the files that used to reside under this directory are listed, below, under the heading "<b>[[#Primary_Web|Primary Web]]</b>"</li>
  <li>Files under this directory used to be accessible by browsers that pointed to the URL:  http://www.phys.lsu.edu/faculty/tohline</li>
  </ul>
</ul>

Or &hellip;
<ul>
  <li>I would log into "theory.phys.lsu.edu" then &hellip;</li>
  <ul>
  <li>I would "cd" into "public_html", as above, then &hellip;</li>
  <li>I would type "cd ../../projs/astro", which would take me to <font color="red">/opt1/usrlocal/apache2/htdocs/graceland/projs/astro</font></li>
  <li>Many of the files that used to reside under this directory are listed, below, under the heading "<b>[[#Secondary_Web|Secondary Web]]</b>"</li>
  <li>Files under this directory used to be accessible by browsers that pointed to the URL:  http://www.phys.lsu.edu/astro/</li>
  </ul>
</ul>

Or &hellip;
<ul>
  <li>I would log into "theory.phys.lsu.edu" then &hellip;</li>
  <ul>
  <li>I would "cd" into "public", which would take me to <font color="red">/opt1/usrlocal/apache2/htdocs/tohline</font></li>
  <li>Many of the files that used to reside under this directory are listed, below, under the heading "<b>[[#Tertiary_Web|Tertiary Web]]</b>"</li>
  <li>Files under this directory used to be accessible by browsers that pointed to the URL:  http://phys.lsu.edu/tohline/</li>
  </ul>
</ul>

=Key Directories and Files on xxxx.phys.lsu.edu=

===Primary Web===
public_html = /opt1/usrlocal/apache2/htdocs/graceland/faculty/tohline =
http://www.phys.lsu.edu/faculty/tohline &hellip;

HOMEPAGE RELEVANT
<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>vision.html</li>
  <li>resume0.html</li>
  <li>ref0_index.html</li>
  <li>ref0_ref.html</li>
  <li>PDF-formatted &hellip;</li>
  <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>t.html:  (circa 2006) Single-page statement of research interests an 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 ENSEMBLES
<ul>
  <li>image.ensemble:   <font color="red">TERRIFIC</font> image-mosaic pointing to more than "Astrophysics Movies"<br />
        (most links point to descriptions listed below on our <b>[[#Secondary_Web|Secondary Web]]</b> MOVIE ENSEMBLES category)
  </li>
</ul>


DIRECTORIES
<ul>
  <li>aasvideo2006:  Simply points to subdirectory &hellip; tohline/astroph/dmtf05/</li>
  <li>Appendices</li>
  <li>Applications</li>
  <li>arribas:  OBJ files prepared in effort to solicit "Micky Mouse" glass solid rectangle from Arribas</li>
  <li>astr1102.04</li>
  <li>astr4222</li>
  <li>astroph</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>pullin</li>
  <li>rmode/
  <ul>
    <li>Index explaining how r-mode movie was rendered: &nbsp;&nbsp; http://www.phys.lsu.edu/faculty/tohline/rmode/index.html</li>
    <li>FINAL 3D movie (circa 2000):   &nbsp;&nbsp; http://www.phys.lsu.edu/faculty/tohline/rmode/final.mov (6,848K)</li>
    <li>mpg-version of FINAL 3D movie:   &nbsp;&nbsp; http://www.phys.lsu.edu/faculty/tohline/rmode/rmode.waveshort.mpg (1,812K)</li>
    <li>zebraimaging/
    <ul>
      <li>Plan to enlist holographic-imaging capabilities offered by <b><font color="red">Zebra Imaging/</font></b>:   &nbsp;&nbsp; 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 rmode movie frame #290</li>
    </ul>
    </li>
  </ul>
  </li>
  <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>webintro</li>
  <li>whyOOP</li>
  <li>www.cise.org</li>
  <li>youtube</li>
</ul>


GRAD STUDENTS
<ul>
  <li>barnes/</li>
  <li>motl/</li>
  <li>ou/</li>
  <li>valencic.html</li>
</ul>


IMAGES
<ul>
  <li>ballgreen.gif</li>
  <li>greenbullet.gif</li>
  <li>horiz.line.gif</li>
  <li>merger.oneil.mpeg</li>
  <li>pics/</li>
  <li>purplebullet.gif</li>
  <li>rmode.final.mpeg:  &nbsp;&nbsp; presumably the same as "rmode.waveshort.mpg" as described above under the "rmode" DIRECTORY<br />
<b><font color="red">YouTube posting:</font></b> &nbsp;[https://Youtu.be/i2zBvA7c7iB 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 FILES
<ul>
  <li>fission.movies.html:  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 in HTML format</li>
  <li>meaganISEF.html:  A thank-you note from Meagan Messina dated 5/16/2000</li>
  <li>out01</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 CFD 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/ &hellip;

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


MOVIE ENSEMBLES
<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>equalmass.binary.html:  The Relative Stability of Close, Equal-Mass Binaries</li>
      </ul>
      </li>
</ul>
    </li>
</ul>


DIRECTORIES
<ul>
  <li>barmode/index.html: &nbsp; &nbsp; <font color="red">EXCELLENT</font> collection of 10 movies &#8212; along with short captions &#8212; of Cazes' simulations</li>
  <li>cip/: &nbsp; &nbsp; Contains "clickable map" for talk found below in cazes/dodconf/hce.html</li>
  <li>drexel/</li>
  <li>movies/: &nbsp; &nbsp; includes subdirectory with early "motl" movies</li>
  <li>nap98/bf.final.lasp.html: &nbsp; &nbsp; Contains movie (movie4 ?) showing Lagrangian particle motions in four of Andalib's models</li>
  <li>network_database/ &nbsp; &nbsp; Defunct attempt (circa 1998) to create an interactive database of physics department computers</li>
  <li>tohline/ &nbsp; &nbsp; Contains primarily java/perl/fortran scripts to support active elements of early H_Book effort (circa 1997 with, e.g., Sherfessee &amp; Muffoletto)</li>
</ul>



GRAD STUDENTS
<ul>
  <li>cazes/
  <ul>
    <li>dodconf/hce.html:  Heterogeous Computing Environment to &hellip;</li>
    <li>LSU.at.SDSC.html: &nbsp;&nbsp; Hydrocode timings in (circa 1996) proposal for T3E time at SDSC</li>
    <li>tohline_NRAC98/ &hellip; &nbsp; &nbsp; includes  the following seven [https://digitalcommons.lsu.edu/gradschool_disstheses/6650/ Andalib] velocity maps<br />
<table border="1" align="center">
<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">[[File:Andalib.vel05Small.jpeg|100px|Andalib.vel05]]</td>
<td align="center">[[File:Andalib.vel12Small.jpeg|100px|Andalib.vel12]]</td>
<td align="center">[[File:Andalib.vel14Small.jpeg|100px|Andalib.vel14]]</td>
<td align="center">[[File:Andalib.vel20Small.jpeg|100px|Andalib.vel20]]</td>
<td align="center">[[File:Andalib.vel30Small.jpeg|100px|Andalib.vel30]]</td>
<td align="center">[[File:Andalib.vel36Small.jpeg|100px|Andalib.vel36]]</td>
<td align="center">[[File:Andalib.vel43Small.jpeg|100px|Andalib.vel43]]</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><font color="red">LOTS!</font> of other good stuff</li>
  </ul>
  </li>
  <li>fisher/</li>
  <li>howie</li>
  <li>motl/</li>
  <li>paul/</li>
</ul>



IMAGES
<ul>
  <li>m = 2 instability in PP torus &hellip;
  <ul>
    <li>bar.mpg: &nbsp;&nbsp; Instability in PP torus</li>
    <li>joel.mpg: &nbsp; &nbsp; (same as bar.mpg)</li>
    <li>joelmov.gif:  (larger) animation of instability in PP torus</li>
    <li>barmov.gif:  animation of instability in PP torus</li>
  </ul>
  </li>
  <li>fig3.jpg:  key figure ensemble from Cazes' dissertation</li>
  <li>Flyby of tilted-ring, warped galaxy disk &hellip;
  <ul>
    <li>gal.mpg: &nbsp;&nbsp; Excellent flyby of "tilted disk" model</li>
    <li>galmov.gif:  Crude resolution "tilted disk" animation ???</li>
  </ul>
  </li>
  <li>icon.gif:  Crude resolution of bar instability (2D eq. plane)</li>
  <li>splash.mpg:  &nbsp;&nbsp; Neat animation of nonequilibrium binary</li>
  <li>Sample of binary-merger animations from Kim New's research &hellip;
  <ul>
    <li>hydro.mpg:  &nbsp;&nbsp; Early movie segment of WD mass-transfor & merger</li>
    <li>kimmov.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 &hellip;
  <ul>
    <li>paul.mpg</li>
    <li>paulmov.gif:  (small) animation of thin disk settling</li>
  </ul>
  </li>
</ul>



OTHER FILES
<ul>
  <li>home.html: &nbsp;&nbsp; Same as "index.html"</li>
  <li>home.old.html: &nbsp;&nbsp; <font color="red">TERRIFIC!</font> includes links to long-lost mpg movies; load in Chrome, rather than Safari</li>
  <li>index.html: &nbsp;&nbsp; Crude home page for "Astrophysics Theory Group at LSU</li>
  <li>tohline.html:  &nbsp; &nbsp; 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 &hellip;
  <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/] &hellip;<br />

DIRECTORIES:<br />
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/&nbsp; &nbsp; <-- ''circa 2021''</li>
  <li>Gifs/</li>
  <li>HBook/</li>
  <li>IGERT/</li>
  <li>New/</li>
</ul>

FILES
<ul>
  <li>LSUAEI.movies.html</li>
  <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>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: &nbsp;&nbsp; www.phys.lsu.edu/astro/nap98/movies/movie1.mov (5,907K)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/BhRUqZe0Ly4 BhRUqZe0Ly4]</font></b>
  </li>
  <li>"Model B" Initially uniform vortensity: &nbsp;&nbsp; www.phys.lsu.edu/astro/barmode/movies/modelB.spiral.mov (7.7M)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/Qh-bMto2e3k Qh-bMto2e3k]</font></b>
  </li>
</ul>


COMPRESSIBLE ANALOGS OF RIEMANN ELLIPSOIDS
<ul>
  <li>"Model A" Steady-state:  &nbsp;&nbsp; www.phys.lsu.edu/astro/barmode/movies/modelA.steady.mov (7,169K)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/z3RDthHnY3A z3RDthHnY3A]</font></b>
  </li>
  <li>"Model A" Equatorial Flow:  &nbsp;&nbsp; www.phys.lsu.edu/astro/nap98/movies/movie2.mov (5.9M)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/fgjjzu3Nmo8 fgjjzu3Nmo8]</font></b> &#8212; <font color="maroon">''Japan's National Astronomical Observatory''</font> poster mounted on the wall
  </li>
  <li>"Model A" Meridional Flow:  &nbsp;&nbsp; www.phys.lsu.edu/astro/nap98/movies/movie3.mov (3.5M)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/_nXKv0k0h-Q _nXKv0k0h-Q]</font></b> &#8212; <font color="maroon">''Japan's National Astronomical Observatory''</font> poster mounted on the wall
  </li>
  <li>"Model B" Steady-state:  &nbsp;&nbsp; www.phys.lsu.edu/astro/barmode/movies/modelB.steady.mov (14.1M)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/Eyl81O9s62s Eyl81O9s62s]</font></b>
  </li>
  <li>"Model B" Equatorial Flow:  &nbsp;&nbsp; www.phys.lsu.edu/astro/barmode/movies/bar_uv.mov (5,976K)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/yggbz9z8JQ4 yggbz9z8JQ4]</font></b> &#8212; <font color="maroon">''National Science Foundation''</font> wall poster
  </li>
  <li>Andalib's Equatorial Flow:  &nbsp;&nbsp; www.phys.lsu.edu/astro/cip/movie2.mov (5.9M)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/p550IDP8h-s p550IDP8h-s]</font></b> &#8212; <font color="maroon">''Computers in Physics''</font> wall poster
  </li>
  <li>Four Andalib Models:  &nbsp;&nbsp; www.phys.lsu.edu/astro/nap98/movies/movie4.mov (7.1M)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/cCfLmitM7bc cCfLmitM7bc]</font></b> &#8212; <font color="maroon">''Japan's National Astronomical Observatory''</font> poster mounted on the wall
  </li>
</ul>


COOLING + FISSION (?)
<ul>
  <li>Cooling evolution:  &nbsp;&nbsp; www.phys.lsu.edu/astro/barmode/movies/binary.form.mov (8,514K)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/erYWHgaKYyc erYWHgaKYyc]</font></b>
  </li>
  <li>Equatorial "Binary" Flow:   &nbsp;&nbsp; www.phys.lsu.edu/astro/cazes/dodconf/movies/movie3.mov (4,712K)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/nC4adQzlXrI nC4adQzlXrI]</font></b> &#8212; <font color="maroon">''MSRC''</font> wall poster
  </li>
  <li>Meridional "Binary" Flow:  &nbsp;&nbsp; www.phys.lsu.edu/astro/cazes/dodconf/movies/movie4.mov (3,375K)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/S0tg2jURzGE S0tg2jURzGE]</font></b> &#8212; <font color="maroon">''MSRC''</font> wall poster
  </li>
  <li>Andalib "Binary" Model:  &nbsp;&nbsp; www.phys.lsu.edu/astro/barmode/movies/bin_sa.mov (5,725K)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/nkwRJh2tgos nkwRJh2tgos]</font></b> &#8212; <font color="maroon">''MSRC''</font> wall poster
  </li>
</ul>


NEUTRON STAR r-MODE INSTABILITY
<ul>
  <li>Nonlinear development of r-mode instability in a neutron star: Mac &hellip; TransitionPC_V01/Videos/YouTube/rmode.final.mpeg (1.9M)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/i2zBvA7c7i8 i2zBvA7c7i8]</font></b>
  </li>
</ul>


ELLIPTICAL INSTABILITY
<ul>
  <li>Nonlinear development of an elliptical instability in a rotating bar: &nbsp;&nbsp; Mac &hellip; TransitionPC_V01/Videos/YouTube/fmode.b181.helix.gr_off.mov (9.8M)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/Fi8Fp26uc-g Fi8Fp26uc-g]</font></b>
  </li>
</ul>


MASS-TRANSFERRING BINARY STAR SYSTEM
<ul>
  <li>Example of mass-transferring binary star system, similar to a white-dwarf binary: &nbsp;&nbsp; Mac &hellip; TransitionPC_V01/Videos/YouTube/Q0.4D.mov (74.3M)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/lFR5S_Fc-9w lFR5S_Fc-9w]</font></b><br />
<b><font color="red">EXCELLENT!</font></b> 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: &nbsp;&nbsp; Mac &hellip; TransitionPC_V01/Videos/YouTube/q0.4_hires_donor.mov (5.6M)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/pxjhuR0BsE0 pxjhuR0BsE0]</font></b>
  </li>
</ul>


SETTLING DISK
<ul>
  <li>Paul Fisher's settling galaxy disk (circa 1999):  &nbsp;&nbsp; www.phys.lsu.edu/astro/barmode/paul.mpg (69K)<br />
YouTube id = <b><font color="darkgreen">[https://youtu.be/yxOLu03T1yE yxOLu03T1yE]</font></b>
  </li>
</ul>

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


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