Difference between revisions of "User:Tohline/Appendix/lsuPhys"

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   <li>purplebullet.gif</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 />
   <li>rmode.final.mpeg:  &nbsp;&nbsp; presumably the same as "rmode.waveshort.mpg" as described above under the "rmode" DIRECTORY<br />
<b><font color="maroon">YouTube:</font></b> &nbsp;[https://Youtu.be/i2zBvA7c7iB rmode.final.mpeg]
<b><font color="red">YouTube posting:</font></b> &nbsp;[https://Youtu.be/i2zBvA7c7iB rmode.final.mpeg]
   </li>
   </li>
   <li>saied.stream.gif</li>
   <li>saied.stream.gif</li>
Line 353: Line 353:
The files in these directories primarily contain (circa 2006) XML-formatted attempts to present instructional material that contains many nontrivial mathematical expressions.
The files in these directories primarily contain (circa 2006) XML-formatted attempts to present instructional material that contains many nontrivial mathematical expressions.
<ul>
<ul>
  <li>COLLADA/&nbsp; &nbsp; <-- ''circa 2021''</li>
   <li>Gifs/</li>
   <li>Gifs/</li>
   <li>HBook/</li>
   <li>HBook/</li>
Line 362: Line 363:
<ul>
<ul>
   <li>LSUAEI.movies.html</li>
   <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.pdf</li>
   <li>LSUAEI.talk.ppt</li>
   <li>LSUAEI.talk.ppt</li>
Line 373: Line 385:
<ul>
<ul>
   <li>"Model A" Classic, two-armed spiral: &nbsp;&nbsp; www.phys.lsu.edu/astro/nap98/movies/movie1.mov (5,907K)<br />
   <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">BhRUqZe0Ly4</font></b>
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>
   </li>
</ul>
</ul>
Line 380: Line 395:
COMPRESSIBLE ANALOGS OF RIEMANN ELLIPSOIDS
COMPRESSIBLE ANALOGS OF RIEMANN ELLIPSOIDS
<ul>
<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 />
   <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">yggbz9z8JQ4</font></b>
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>
   </li>
</ul>
</ul>




FISSION
COOLING + FISSION (?)
<ul>
<ul>
   <li>Cooling evolution:  &nbsp;&nbsp; www.phys.lsu.edu/astro/barmode/movies/binary.form.mov (8,514K)<br />
   <li>Cooling evolution:  &nbsp;&nbsp; www.phys.lsu.edu/astro/barmode/movies/binary.form.mov (8,514K)<br />
YouTube id = <b><font color="darkgreen">erYWHgaKYyc</font></b>
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>
   </li>
</ul>
</ul>
Line 397: Line 439:
<ul>
<ul>
   <li>Nonlinear development of r-mode instability in a neutron star: Mac &hellip; TransitionPC_V01/Videos/YouTube/rmode.final.mpeg (1.9M)<br />
   <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">i2zBvA7c7i8</font></b>
YouTube id = <b><font color="darkgreen">[https://youtu.be/i2zBvA7c7i8 i2zBvA7c7i8]</font></b>
   </li>
   </li>
</ul>
</ul>
Line 405: Line 447:
<ul>
<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 />
   <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">Fi8Fp26uc-g</font></b>
YouTube id = <b><font color="darkgreen">[https://youtu.be/Fi8Fp26uc-g Fi8Fp26uc-g]</font></b>
   </li>
   </li>
</ul>
</ul>
Line 413: Line 455:
<ul>
<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 />
   <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">lFR5S_Fc-9w</font></b><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.
<b><font color="red">EXCELLENT!</font></b> This movie shows nonlinear-amplitude pumping of m = 3, 4, 5 modes on the accretor.


   </li>
   </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 />
   <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">pxjhuR0BsE0</font></b>
YouTube id = <b><font color="darkgreen">[https://youtu.be/pxjhuR0BsE0 pxjhuR0BsE0]</font></b>
   </li>
   </li>
</ul>
</ul>


==Movies to be Uploaded==
BAR-MODE INSTABILITY
<ul>
  <li>"Model B" Initially uniform vortensity: &nbsp;&nbsp; http://www.phys.lsu.edu/astro/barmode/movies/modelB.spiral.mov (10.8M)</li>
</ul>


FISSION
SETTLING DISK
<ul>
<ul>
   <li>Equatorial Flow:   &nbsp;&nbsp; http://www.phys.lsu.edu/astro/cazes/dodconf/movies/movie3.mov (4,712K)</li>
   <li>Paul Fisher's settling galaxy disk (circa 1999): &nbsp;&nbsp; www.phys.lsu.edu/astro/barmode/paul.mpg (69K)<br />
  <li>Meridional Flow:  &nbsp;&nbsp; http://www.phys.lsu.edu/astro/cazes/dodconf/movies/movie4.mov (3,375K)</li>
YouTube id = <b><font color="darkgreen">[https://youtu.be/yxOLu03T1yE yxOLu03T1yE]</font></b>
   <li>Andalib Model:  &nbsp;&nbsp; http://www.phys.lsu.edu/astro/barmode/movies/bin_sa.mov (5,725K)</li>
   </li>
</ul>
</ul>


COMPRESSIBLE ANALOGS OF RIEMANN ELLIPSOIDS
==Movies to be Uploaded==
<ul>
''None'' at the present time.
  <li>"Model A" Steady-state:  &nbsp;&nbsp; http://www.phys.lsu.edu/astro/barmode/movies/modelA.steady.mov (7,169K)</li>
  <li>"Model B" Steady-state:  &nbsp;&nbsp; http://www.phys.lsu.edu/astro/barmode/movies/modelB.steady.mov (14.1M)</li>
  <li>"Model A" Equatorial Flow:  &nbsp;&nbsp; http://www.phys.lsu.edu/astro/barmode/movies/movie2.mov (5.75M)</li>
  <li>"Andalib Model" Equatorial Flow:  &nbsp;&nbsp; http://www.phys.lsu.edu/astro/cip/movie2.mov (5,754K)</li>
  <li>"Model A" Meridional Flow:  &nbsp;&nbsp; http://www.phys.lsu.edu/astro/nap98/movies/movie3.mov (3,375K)</li>
</ul>




{{LSU_HBook_footer}}
{{LSU_HBook_footer}}

Latest revision as of 17:41, 27 January 2021

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

Whitworth's (1981) Isothermal Free-Energy Surface
|   Tiled Menu   |   Tables of Content   |  Banner Video   |  Tohline Home Page   |

Primary Web

public_html = /opt1/usrlocal/apache2/htdocs/graceland/faculty/tohline = http://www.phys.lsu.edu/faculty/tohline …

HOMEPAGE RELEVANT

  • index.html
  • indexhtv.html: Homepage prior to "accessibility statement" added by htv (Hortensia)
  • indexMarch2011.html
  • biosketch.html
  • courses.html: Also see "courses" directory, below
  • faculty.awards.html: explains what an Alumni Professorship is
  • features.html: lists featured work
  • publications.html: Older version of ref_ref.html
  • ref_index.html
  • ref_IPAM2005.html
  • ref_movies.html
  • ref_ref.html
  • research.html
  • resume.html
  • students.html
  • vision.html
  • resume0.html
  • ref0_index.html
  • ref0_ref.html
  • PDF-formatted …
    • resume.forpdf.html
    • resume01.forpdf.html
    • resume02.forpdf.html
    • resume08.forpdf.html
    • ref_ref.forpdf.html
    • ref_ref.forpdf06.html
    • ref_ref.forpdf07.html
    • ref_ref.forpdf08.html
    • research.forpdf.html
  • t.html: (circa 2006) Single-page statement of research interests an relevant publications
  • test.html: very early draft of homepage layout, including one of Andalib's binary vector flows
  • test2.html: very early draft of homepage layout


MOVIE ENSEMBLES

  • 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)


DIRECTORIES

  • aasvideo2006: Simply points to subdirectory … tohline/astroph/dmtf05/
  • Appendices
  • Applications
  • arribas: OBJ files prepared in effort to solicit "Micky Mouse" glass solid rectangle from Arribas
  • astr1102.04
  • astr4222
  • astroph
  • BPFest:
  • capital
  • CHEGA
  • CIP
  • cise: Fledgling effort to construct "astrophysics portal" for CISE magazine
  • CiSE
  • clayton
  • Context
  • courses
  • grbcollaboration
  • GRBcollaboration
  • GRsources
  • honors
  • idesk
  • Interim2001
  • Landolt
  • ligo
  • lisa6
  • lsulogos
  • movies
  • MRAC_2007
  • NAVO
  • NCSA
  • SDSC
  • NPACI98
  • NRAC98.proposal
  • NRAC99
  • NRAC_2000
  • NRAC_2001
  • NRAC_2002
  • NRAC_2004
  • NRAC_2005
  • NRC_rankings
  • NSF99
  • NSF02
  • NSF03
  • oldcommittees
  • oldpdfs
  • oldwebpages
  • papers
  • PHYS2411
  • phys4412
  • PHYS7412
  • phys7741
  • pullin
  • rmode/
  • sabbatical
  • Sci-Tech
  • sources
  • sph-grid
  • Talks
  • Talks_Additional
  • temp
  • vistrails
  • vita
  • webintro
  • whyOOP
  • www.cise.org
  • youtube


GRAD STUDENTS

  • barnes/
  • motl/
  • ou/
  • valencic.html


IMAGES

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


OTHER FILES

  • fission.movies.html: detailed overview of (primarily) dissertation work by John Cazes
  • HDmovies.html: (circa 2008) Explaining need to feed broadcast HDTV format
  • html.documents.html: list (prior to 2005) of talks/papers/proposals in HTML format
  • meaganISEF.html: A thank-you note from Meagan Messina dated 5/16/2000
  • out01
  • Quicktime.html: (circa 2005) detailed overview of steps used to generate a Quicktime animation sequence
  • realtime.html (circa 2005) detailed estimate of feasibility of real-time analysis (e.g., inside CAVE) of 3D CFD flows
  • symbol.html: Early draft of H_Book page giving PGEs in spherical symmetry
  • T3E.timings.html: Points to same file name inside "SDSC" directory
  • TinsleyNotes1978.pdf
  • Tohline_Dissertation.pdf
  • valtech.html: (circa 1999) John Woodward's company?

Secondary Web

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

H_BOOK RELEVANT

  • H_Book.current/H_Book.html


MOVIE ENSEMBLES

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


DIRECTORIES

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


GRAD STUDENTS

  • cazes/
    • dodconf/hce.html: Heterogeous Computing Environment to …
    • LSU.at.SDSC.html:    Hydrocode timings in (circa 1996) proposal for T3E time at SDSC
    • tohline_NRAC98/ …     includes the following seven Andalib velocity maps
      Filename: vel05 vel12 vel14 vel20 vel30 vel36 vel43
      Thumbnail: Andalib.vel05 Andalib.vel05 Andalib.vel05 Andalib.vel05 Andalib.vel05 Andalib.vel05 Andalib.vel05
      Model. No. ?? ?? D13 D14 --- --- C13(?)
      Fig. No. ?? ?? 5.16 5.15 5.14 5.13 5.6(?)
    • LOTS! of other good stuff
  • fisher/
  • howie
  • motl/
  • paul/


IMAGES

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


OTHER FILES

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

Tertiary Web

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

DIRECTORIES:
The files in these directories primarily contain (circa 2006) XML-formatted attempts to present instructional material that contains many nontrivial mathematical expressions.

  • COLLADA/    <-- circa 2021
  • Gifs/
  • HBook/
  • IGERT/
  • New/

FILES

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

YouTube

Movies Already Uploaded

BAR-MODE INSTABILITY

  • "Model A" Classic, two-armed spiral:    www.phys.lsu.edu/astro/nap98/movies/movie1.mov (5,907K)
    YouTube id = BhRUqZe0Ly4
  • "Model B" Initially uniform vortensity:    www.phys.lsu.edu/astro/barmode/movies/modelB.spiral.mov (7.7M)
    YouTube id = Qh-bMto2e3k


COMPRESSIBLE ANALOGS OF RIEMANN ELLIPSOIDS

  • "Model A" Steady-state:    www.phys.lsu.edu/astro/barmode/movies/modelA.steady.mov (7,169K)
    YouTube id = z3RDthHnY3A
  • "Model A" Equatorial Flow:    www.phys.lsu.edu/astro/nap98/movies/movie2.mov (5.9M)
    YouTube id = fgjjzu3Nmo8 — Japan's National Astronomical Observatory poster mounted on the wall
  • "Model A" Meridional Flow:    www.phys.lsu.edu/astro/nap98/movies/movie3.mov (3.5M)
    YouTube id = _nXKv0k0h-Q — Japan's National Astronomical Observatory poster mounted on the wall
  • "Model B" Steady-state:    www.phys.lsu.edu/astro/barmode/movies/modelB.steady.mov (14.1M)
    YouTube id = Eyl81O9s62s
  • "Model B" Equatorial Flow:    www.phys.lsu.edu/astro/barmode/movies/bar_uv.mov (5,976K)
    YouTube id = yggbz9z8JQ4 — National Science Foundation wall poster
  • Andalib's Equatorial Flow:    www.phys.lsu.edu/astro/cip/movie2.mov (5.9M)
    YouTube id = p550IDP8h-s — Computers in Physics wall poster
  • Four Andalib Models:    www.phys.lsu.edu/astro/nap98/movies/movie4.mov (7.1M)
    YouTube id = cCfLmitM7bc — Japan's National Astronomical Observatory poster mounted on the wall


COOLING + FISSION (?)

  • Cooling evolution:    www.phys.lsu.edu/astro/barmode/movies/binary.form.mov (8,514K)
    YouTube id = erYWHgaKYyc
  • Equatorial "Binary" Flow:    www.phys.lsu.edu/astro/cazes/dodconf/movies/movie3.mov (4,712K)
    YouTube id = nC4adQzlXrI — MSRC wall poster
  • Meridional "Binary" Flow:    www.phys.lsu.edu/astro/cazes/dodconf/movies/movie4.mov (3,375K)
    YouTube id = S0tg2jURzGE — MSRC wall poster
  • Andalib "Binary" Model:    www.phys.lsu.edu/astro/barmode/movies/bin_sa.mov (5,725K)
    YouTube id = nkwRJh2tgos — MSRC wall poster


NEUTRON STAR r-MODE INSTABILITY

  • Nonlinear development of r-mode instability in a neutron star: Mac … TransitionPC_V01/Videos/YouTube/rmode.final.mpeg (1.9M)
    YouTube id = i2zBvA7c7i8


ELLIPTICAL INSTABILITY

  • 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 = Fi8Fp26uc-g


MASS-TRANSFERRING BINARY STAR SYSTEM

  • 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 = lFR5S_Fc-9w
    EXCELLENT! This movie shows nonlinear-amplitude pumping of m = 3, 4, 5 modes on the accretor.
  • 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 = pxjhuR0BsE0


SETTLING DISK

  • Paul Fisher's settling galaxy disk (circa 1999):    www.phys.lsu.edu/astro/barmode/paul.mpg (69K)
    YouTube id = yxOLu03T1yE

Movies to be Uploaded

None at the present time.


Whitworth's (1981) Isothermal Free-Energy Surface

© 2014 - 2021 by Joel E. Tohline
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Appendices: | Equations | Variables | References | Ramblings | Images | myphys.lsu | ADS |
Recommended citation:   Tohline, Joel E. (2021), The Structure, Stability, & Dynamics of Self-Gravitating Fluids, a (MediaWiki-based) Vistrails.org publication, https://www.vistrails.org/index.php/User:Tohline/citation

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