https://www.vistrails.org//index.php?title=User:Tohline/IVAJ/Levels2and3&feed=atom&action=historyUser:Tohline/IVAJ/Levels2and3 - Revision history2024-03-28T12:48:28ZRevision history for this page on the wikiMediaWiki 1.36.2https://www.vistrails.org//index.php?title=User:Tohline/IVAJ/Levels2and3&diff=2875&oldid=prevTohline: /* Base Workflow */2010-03-10T03:06:59Z<p><span dir="auto"><span class="autocomment">Base Workflow</span></span></p>
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 03:06, 10 March 2010</td>
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<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><tr><td align="left"></div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><tr><td align="left"></div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><font size="+1" color="red"><b>Execute on my desktop</b></font>: </div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><font size="+1" color="red"><b>Execute on my desktop</b></font>: </div></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>[[Image:VisTrails_Install_icon.jpg|right|frameless|border|link=http://www.sci.utah.edu/~emanuele/movies/Stars.mov]] Clicking on Figure 2's red "Execute on my desktop" button will download the Figure 1 workflow to the reader's laptop/desktop system for local execution. In order for this to work, VisTrails (version 1.4.2 or higher) must be installed on the reader's local system. (For help installing VisTrails, click the icon shown here the right, or view [http://www.youtube.com/watch?v=4oDXEjtYWJk&fmt=22 this YouTube video].) Note that two data files totaling > 100 MBytes will also be transferred for analysis on the local system, so the entire download may take 10 or more minutes, depending on the network connection. </div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>[[Image:VisTrails_Install_icon.jpg|right|frameless|border|link=http://www.sci.utah.edu/~emanuele/movies/Stars.mov]] Clicking on Figure 2's red "Execute on my desktop" button will download the Figure 1 workflow to the reader's laptop/desktop system for local execution. In order for this to work, VisTrails (version 1.4.2 or higher) must be installed on the reader's local system. (For help installing VisTrails, click the icon shown here <ins style="font-weight: bold; text-decoration: none;">on </ins>the right, or view [http://www.youtube.com/watch?v=4oDXEjtYWJk&fmt=22 this YouTube video].) Note that two data files totaling > 100 MBytes will also be transferred for analysis on the local system, so the entire download may take 10 or more minutes, depending on the network connection. </div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div></td></tr></div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div></td></tr></div></td></tr>
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</table>Tohlinehttps://www.vistrails.org//index.php?title=User:Tohline/IVAJ/Levels2and3&diff=2874&oldid=prevTohline: /* Base Workflow */ Insert VisTrails_Install_icon2010-03-10T03:04:54Z<p><span dir="auto"><span class="autocomment">Base Workflow: </span> Insert VisTrails_Install_icon</span></p>
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<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><tr><td align="left"></div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><tr><td align="left"></div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><font size="+1" color="red"><b>Execute on my desktop</b></font>: </div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><font size="+1" color="red"><b>Execute on my desktop</b></font>: </div></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>Clicking on Figure 2's red "Execute on my desktop" button will download the Figure 1 workflow to the reader's laptop/desktop system for local execution. In order for this to work, VisTrails (version 1.4.2 or higher) must be installed on the reader's local system. (For help installing VisTrails, <del style="font-weight: bold; text-decoration: none;">download [http://www.sci.utah.edu/~emanuele/movies/Stars.mov this quicktime movie] </del>or view [http://www.youtube.com/watch?v=4oDXEjtYWJk&fmt=22 this YouTube video].) Note that two data files totaling > 100 MBytes will also be transferred for analysis on the local system, so the entire download may take 10 or more minutes, depending on the network connection. </div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">[[Image:VisTrails_Install_icon.jpg|right|frameless|border|link=http://www.sci.utah.edu/~emanuele/movies/Stars.mov]] </ins>Clicking on Figure 2's red "Execute on my desktop" button will download the Figure 1 workflow to the reader's laptop/desktop system for local execution. In order for this to work, VisTrails (version 1.4.2 or higher) must be installed on the reader's local system. (For help installing VisTrails, <ins style="font-weight: bold; text-decoration: none;">click the icon shown here the right, </ins>or view [http://www.youtube.com/watch?v=4oDXEjtYWJk&fmt=22 this YouTube video].) Note that two data files totaling > 100 MBytes will also be transferred for analysis on the local system, so the entire download may take 10 or more minutes, depending on the network connection. </div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div></td></tr></div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div></td></tr></div></td></tr>
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</table>Tohlinehttps://www.vistrails.org//index.php?title=User:Tohline/IVAJ/Levels2and3&diff=2872&oldid=prevTohline: /* Base Workflow */ Insert links to installation movies2010-03-08T20:01:43Z<p><span dir="auto"><span class="autocomment">Base Workflow: </span> Insert links to installation movies</span></p>
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<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><tr><td align="left"></div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><tr><td align="left"></div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><font size="+1" color="red"><b>Execute on my desktop</b></font>: </div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><font size="+1" color="red"><b>Execute on my desktop</b></font>: </div></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>Clicking on Figure 2's red "Execute on my desktop" button will download the Figure 1 workflow to the reader's laptop/desktop system for local execution. In order for this to work, VisTrails (version 1.4.2 or higher) must be installed on the reader's local system. Note that two data files totaling > 100 MBytes will also be transferred for analysis on the local system, so the entire download may take 10 or more minutes, depending on the network connection. </div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>Clicking on Figure 2's red "Execute on my desktop" button will download the Figure 1 workflow to the reader's laptop/desktop system for local execution. In order for this to work, VisTrails (version 1.4.2 or higher) must be installed on the reader's local system. <ins style="font-weight: bold; text-decoration: none;">(For help installing VisTrails, download [http://www.sci.utah.edu/~emanuele/movies/Stars.mov this quicktime movie] or view [http://www.youtube.com/watch?v=4oDXEjtYWJk&fmt=22 this YouTube video].) </ins>Note that two data files totaling > 100 MBytes will also be transferred for analysis on the local system, so the entire download may take 10 or more minutes, depending on the network connection. </div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div></td></tr></div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div></td></tr></div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr>
</table>Tohlinehttps://www.vistrails.org//index.php?title=User:Tohline/IVAJ/Levels2and3&diff=2865&oldid=prevTohline: User:Tohline/CPM/Levels2and3 moved to User:Tohline/IVAJ/Levels2and3: Adopt new name: IVAJ2010-03-03T17:17:19Z<p><a href="/index.php/User:Tohline/CPM/Levels2and3" class="mw-redirect" title="User:Tohline/CPM/Levels2and3">User:Tohline/CPM/Levels2and3</a> moved to <a href="/index.php/User:Tohline/IVAJ/Levels2and3" title="User:Tohline/IVAJ/Levels2and3">User:Tohline/IVAJ/Levels2and3</a>: Adopt new name: IVAJ</p>
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<td colspan="1" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 17:17, 3 March 2010</td>
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</td></tr></table>Tohlinehttps://www.vistrails.org//index.php?title=User:Tohline/IVAJ/Levels2and3&diff=2828&oldid=prevTohline: /* <font color="#0000DD">Base Workflow</font> */ Specify preferred VisTrails version#2010-02-27T18:56:48Z<p><span dir="auto"><span class="autocomment"><font color="#0000DD">Base Workflow</font>: </span> Specify preferred VisTrails version#</span></p>
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 18:56, 27 February 2010</td>
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<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><tr><td align="left"></div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><tr><td align="left"></div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><font size="+1" color="red"><b>Execute on my desktop</b></font>: </div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><font size="+1" color="red"><b>Execute on my desktop</b></font>: </div></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>Clicking on Figure 2's red "Execute on my desktop" button will download the Figure 1 workflow to the reader's laptop/desktop system for local execution. In order for this to work, VisTrails must be installed on the reader's local system<del style="font-weight: bold; text-decoration: none;">. The accompanying video sidebar explains how to acquire and install the VisTrails application</del>. Note that two data files totaling > 100 MBytes will also be transferred for analysis on the local system, so the entire download may take 10 or more minutes, depending on the network connection. </div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>Clicking on Figure 2's red "Execute on my desktop" button will download the Figure 1 workflow to the reader's laptop/desktop system for local execution. In order for this to work, VisTrails <ins style="font-weight: bold; text-decoration: none;">(version 1.4.2 or higher) </ins>must be installed on the reader's local system. Note that two data files totaling > 100 MBytes will also be transferred for analysis on the local system, so the entire download may take 10 or more minutes, depending on the network connection. </div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div></td></tr></div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div></td></tr></div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr>
</table>Tohlinehttps://www.vistrails.org//index.php?title=User:Tohline/IVAJ/Levels2and3&diff=2799&oldid=prevTohline: /* <font color="#0000DD">Base Workflow</font> */ Add caution regarding download time for desktop execution; and add suggested parameter ranges2010-02-22T17:56:27Z<p><span dir="auto"><span class="autocomment"><font color="#0000DD">Base Workflow</font>: </span> Add caution regarding download time for desktop execution; and add suggested parameter ranges</span></p>
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 17:56, 22 February 2010</td>
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<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><tr><td align="left"></div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><tr><td align="left"></div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><font size="+1" color="black"><b>Figure 2</b></font>: </div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><font size="+1" color="black"><b>Figure 2</b></font>: </div></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>An image generated by our customized [http://www.vistrails.org VisTrails] workflow using the indicated values of the three variable parameters, <font face="Courier">Omega_frame</font> <math>(= \Delta \Omega)</math>, <font face="Courier">rho_min</font>, and <font face="Courier">Propagation_time</font>. The 3D-rendered image displays eight equatorial-plane streamlines and a pair of isodensity surfaces (lower density surface colored blue; higher density surface colored red) that outline the structure of both stars as well as the connecting mass-transfer stream. The propagation time is the same for all eight streamlines; along six streamlines, [http://www.vistrails.org VisTrails] carries out the integration in both directions from the location marked by a small colored sphere. Streamlines are truncated prematurely if they enter a region in which the matter density drops below the value specified by <font face="Courier">rho_min</font>, measured as a fraction of the maximum density. A new image will be generated by the VisTrails Wiki server (in accordance with the workflow shown in Figure 1) if the reader selects a different set of parameters and clicks the green "Update" button. <del style="font-weight: bold; text-decoration: none;"> </del></div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>An image generated by our customized [http://www.vistrails.org VisTrails] workflow using the indicated values of the three variable parameters, <font face="Courier">Omega_frame</font> <math>(= \Delta \Omega)</math>, <font face="Courier">rho_min</font>, and <font face="Courier">Propagation_time</font>. The 3D-rendered image displays eight equatorial-plane streamlines and a pair of isodensity surfaces (lower density surface colored blue; higher density surface colored red) that outline the structure of both stars as well as the connecting mass-transfer stream. The propagation time is the same for all eight streamlines; along six streamlines, [http://www.vistrails.org VisTrails] carries out the integration in both directions from the location marked by a small colored sphere. Streamlines are truncated prematurely if they enter a region in which the matter density drops below the value specified by <font face="Courier">rho_min</font>, measured as a fraction of the maximum density. A new image will be generated by the VisTrails Wiki server (in accordance with the workflow shown in Figure 1) if the reader selects a different set of parameters and clicks the green "Update" button. <ins style="font-weight: bold; text-decoration: none;"> Recommended parameter ranges:<br /></ins></div></td></tr>
<tr><td colspan="2"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;"><div align="center"></ins></div></td></tr>
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<tr><td colspan="2"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;"><br /></ins></div></td></tr>
<tr><td colspan="2"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div> </div></td></tr>
<tr><td colspan="2"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">0.1 < <font face="courier">propagation_time</font> < 3.5</ins></div></td></tr>
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<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><tr><td align="left"></div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><tr><td align="left"></div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><font size="+1" color="red"><b>Execute on my desktop</b></font>: </div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div><font size="+1" color="red"><b>Execute on my desktop</b></font>: </div></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>Clicking on Figure 2's red "Execute on my desktop" button will download the Figure 1 workflow to the reader's laptop/desktop system for local execution. In order for this to work, VisTrails must be installed on the reader's local system. The accompanying video sidebar explains how to acquire and install the VisTrails application.</div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>Clicking on Figure 2's red "Execute on my desktop" button will download the Figure 1 workflow to the reader's laptop/desktop system for local execution. In order for this to work, VisTrails must be installed on the reader's local system. The accompanying video sidebar explains how to acquire and install the VisTrails application<ins style="font-weight: bold; text-decoration: none;">. Note that two data files totaling > 100 MBytes will also be transferred for analysis on the local system, so the entire download may take 10 or more minutes, depending on the network connection</ins>. </div></td></tr>
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</table>Tohlinehttps://www.vistrails.org//index.php?title=User:Tohline/IVAJ/Levels2and3&diff=2794&oldid=prevEmanuele: /* <font color="#0000DD">Base Workflow</font> */2010-02-17T07:19:14Z<p><span dir="auto"><span class="autocomment"><font color="#0000DD">Base Workflow</font></span></span></p>
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 07:19, 17 February 2010</td>
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<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==<font color="#0000DD">Customized Python Module</font>==</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==<font color="#0000DD">Customized Python Module</font>==</div></td></tr>
</table>Emanuelehttps://www.vistrails.org//index.php?title=User:Tohline/IVAJ/Levels2and3&diff=2768&oldid=prevTohline: Couple of minor wording changes in "Interpretation of Results" subsection2010-02-11T21:30:52Z<p>Couple of minor wording changes in "Interpretation of Results" subsection</p>
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 21:30, 11 February 2010</td>
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<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==<font color="#0000DD">Interpretation of Results</font>==</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==<font color="#0000DD">Interpretation of Results</font>==</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>Figure 2 displays a 3D rendering of the flow from one of our binary mass-transfer simulations as generated by our customized [http://www.vistrails.org VisTrails] workflow using the parameter values indicated beside the image. In particular, the streamlines shown in the default image were generated assuming a frame rotation frequency given by Omega_frame = <math>\Delta\Omega = -0.041.</math> Using the Figure 2 VisMashup App, images can be generated assuming four other values of the frame rotation frequency in the range <math> +0.02 \ge \Delta\Omega \ge -0.06.</math> By downloading and executing this workflow on a local laptop/desktop system (click the red "Execute on my desktop" button shown in Figure 2), the reader can zoom, pan, and interactively rotate any of these 3D-rendered scenes and explore a wider range of model parameter values.</div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>Figure 2 displays a 3D rendering of the flow from one of our binary mass-transfer simulations as generated by our customized [http://www.vistrails.org VisTrails] workflow using the parameter values indicated beside the image. In particular, the streamlines shown in the default image were generated assuming a frame rotation frequency given by <ins style="font-weight: bold; text-decoration: none;"><font face="Courier"></ins>Omega_frame<ins style="font-weight: bold; text-decoration: none;"></font> </ins>= <math>\Delta\Omega = -0.041.</math> Using the Figure 2 VisMashup App, images can be generated assuming four other values of the frame rotation frequency in the range <math> +0.02 \ge \Delta\Omega \ge -0.06.</math> By downloading and executing this workflow on a local laptop/desktop system (click the red "Execute on my desktop" button shown in Figure 2), the reader can zoom, pan, and interactively rotate any of these 3D-rendered scenes and explore a wider range of model parameter values.</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>We'd like to determine which value of <math>\Delta\Omega</math> provides the best measure of the binary star system's true orbital period. For all five choices of <math>\Delta\Omega</math> identified by the Figure 2 VisMashup App, we found the highest velocities (marked by the longest streamlines) along the relatively low-density mass-transfer stream that connects the two stars. This was as expected. Material from the donor star (in the lower half of the rendered image in Figure 2) flows toward its stellar companion, reaching supersonic velocities before impacting the companion. An oblique shock front &#150; whose location is delineated by kinks in the pink, blue, and orange streamlines &#150; terminates the component of motion perpendicular to the companion's surface. Motion transverse to the shock becomes orbital motion in a thick, low-density disk that surrounds the companion star.</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>We'd like to determine which value of <math>\Delta\Omega</math> provides the best measure of the binary star system's true orbital period. For all five choices of <math>\Delta\Omega</math> identified by the Figure 2 VisMashup App, we found the highest velocities (marked by the longest streamlines) along the relatively low-density mass-transfer stream that connects the two stars. This was as expected. Material from the donor star (in the lower half of the rendered image in Figure 2) flows toward its stellar companion, reaching supersonic velocities before impacting the companion. An oblique shock front &#150; whose location is delineated by kinks in the pink, blue, and orange streamlines &#150; terminates the component of motion perpendicular to the companion's surface. Motion transverse to the shock becomes orbital motion in a thick, low-density disk that surrounds the companion star.</div></td></tr>
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<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>Each star's center of mass should lie near the center of the highest density region inside each star (outlined by the nearly spherical, red isodensity surfaces in Figure 2). When we've assigned <math>\Delta\Omega</math> a value that properly identifies the frequency at which the centers of mass of the two stars are orbiting one another, we should see very little residual motion near the donor star's center &#150; that is, streamlines rendered in white and green in Figure 2 should be quite short. Furthermore, we expect that this residual motion should translate into concave streamline segments, mapping out simple circular motion around the center of the donor star. When we've identified the correct value of <math>\Delta\Omega</math>, we also should expect the returning streamline nearest the mass-transfer stream (colored yellow) to remain inside the donor. With these ideas in mind, we judge <math>\Delta\Omega = - 0.041</math>.</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>Each star's center of mass should lie near the center of the highest density region inside each star (outlined by the nearly spherical, red isodensity surfaces in Figure 2). When we've assigned <math>\Delta\Omega</math> a value that properly identifies the frequency at which the centers of mass of the two stars are orbiting one another, we should see very little residual motion near the donor star's center &#150; that is, streamlines rendered in white and green in Figure 2 should be quite short. Furthermore, we expect that this residual motion should translate into concave streamline segments, mapping out simple circular motion around the center of the donor star. When we've identified the correct value of <math>\Delta\Omega</math>, we also should expect the returning streamline nearest the mass-transfer stream (colored yellow) to remain inside the donor. With these ideas in mind, we judge <math>\Delta\Omega = - 0.041</math>.</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>Finally, we note that as the pink and blue streamlines curve around the companion star, they extend outside the companion's disk (as outlined by the blue isodensity surface) in the rendered images with the most negative specified values of <math>\Delta\Omega</math>. These two streamlines appear to align most neatly with the distribution of material in the disk <del style="font-weight: bold; text-decoration: none;">in Figure 2a, that is, </del>for <math>\Delta\Omega = + 0.02</math>. This suggests that there's a characteristic frequency associated with motion in the companion's disk that's different from the binary orbital frequency.</div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>Finally, we note that as the pink and blue streamlines curve around the companion star, they extend outside the companion's disk (as outlined by the blue isodensity surface) in the rendered images with the most negative specified values of <math>\Delta\Omega</math>. These two streamlines appear to align most neatly with the distribution of material in the disk for <math>\Delta\Omega = + 0.02</math>. This suggests that there's a characteristic frequency associated with motion in the companion's disk that's different from the binary orbital frequency.</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>[[Image:Figure3_Tohline.jpg |border|center|600px|Figure 3. A magnified view of multiple streamlines in the region of the flow where the mass-transfer stream originates. (a = left panel) Reproduction of Figure 3 from the published work of Stephen Lubow and Frank Shu (used with permission). (b = right panel) A magnified segment of the flow depicted in Figure 2, image D (<math>\Delta\Omega = - 0.041</math>) from this work; we've numbered the colored streamlines to aid in our comparison with the Lubow and Shu image.]]</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>[[Image:Figure3_Tohline.jpg |border|center|600px|Figure 3. A magnified view of multiple streamlines in the region of the flow where the mass-transfer stream originates. (a = left panel) Reproduction of Figure 3 from the published work of Stephen Lubow and Frank Shu (used with permission). (b = right panel) A magnified segment of the flow depicted in Figure 2, image D (<math>\Delta\Omega = - 0.041</math>) from this work; we've numbered the colored streamlines to aid in our comparison with the Lubow and Shu image.]]</div></td></tr>
</table>Tohlinehttps://www.vistrails.org//index.php?title=User:Tohline/IVAJ/Levels2and3&diff=2767&oldid=prevTohline: /* <font color="#0000DD">Interpretation of Results</font> */ Modify first paragraph of this subsection to be consistent with Mashup App2010-02-11T21:22:33Z<p><span dir="auto"><span class="autocomment"><font color="#0000DD">Interpretation of Results</font>: </span> Modify first paragraph of this subsection to be consistent with Mashup App</span></p>
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<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==<font color="#0000DD">Interpretation of Results</font>==</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==<font color="#0000DD">Interpretation of Results</font>==</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>Figure 2 displays 3D <del style="font-weight: bold; text-decoration: none;">renderings </del>of the flow from one of our binary mass-transfer simulations as generated by our customized [http://www.vistrails.org VisTrails] workflow. <del style="font-weight: bold; text-decoration: none;">We have </del>generated <del style="font-weight: bold; text-decoration: none;">images </del>assuming <del style="font-weight: bold; text-decoration: none;">five different </del>frame rotation <del style="font-weight: bold; text-decoration: none;">frequencies, as specified </del>by <math>\Delta\Omega</math><del style="font-weight: bold; text-decoration: none;">. Aside from labeling </del><math>\Delta\Omega</math> <del style="font-weight: bold; text-decoration: none;">values under each image, we produced Figure 2 by simply taking </del>a <del style="font-weight: bold; text-decoration: none;">screenshot of </del>the <del style="font-weight: bold; text-decoration: none;">[http://www.vistrails.org VisTrails] interactive spreadsheet. The spreadsheet feature has proven to be extremely useful </del>in <del style="font-weight: bold; text-decoration: none;">this analysis because it facilitates </del>the <del style="font-weight: bold; text-decoration: none;">side-by-side comparison of scenes that [http://www.vistrails.org VisTrails] has rendered using different parameter values. And, although we </del>can<del style="font-weight: bold; text-decoration: none;">'t demonstrate it here in print, [http://www.vistrails.org VisTrails] lets users </del>zoom, pan, and interactively rotate <del style="font-weight: bold; text-decoration: none;">all </del>3D-rendered scenes <del style="font-weight: bold; text-decoration: none;">simultaneously</del>.</div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>Figure 2 displays <ins style="font-weight: bold; text-decoration: none;">a </ins>3D <ins style="font-weight: bold; text-decoration: none;">rendering </ins>of the flow from one of our binary mass-transfer simulations as generated by our customized [http://www.vistrails.org VisTrails] workflow <ins style="font-weight: bold; text-decoration: none;">using the parameter values indicated beside the image</ins>. <ins style="font-weight: bold; text-decoration: none;">In particular, the streamlines shown in the default image were </ins>generated assuming <ins style="font-weight: bold; text-decoration: none;">a </ins>frame rotation <ins style="font-weight: bold; text-decoration: none;">frequency given </ins>by <ins style="font-weight: bold; text-decoration: none;">Omega_frame = </ins><math>\Delta\Omega <ins style="font-weight: bold; text-decoration: none;">= -0.041.</ins></math> <ins style="font-weight: bold; text-decoration: none;">Using the Figure 2 VisMashup App, images can be generated assuming four other values of the frame rotation frequency in the range </ins><math> <ins style="font-weight: bold; text-decoration: none;">+0.02 \ge </ins>\Delta\Omega <ins style="font-weight: bold; text-decoration: none;">\ge -0.06.</ins></math> <ins style="font-weight: bold; text-decoration: none;"> By downloading and executing this workflow on </ins>a <ins style="font-weight: bold; text-decoration: none;">local laptop/desktop system (click </ins>the <ins style="font-weight: bold; text-decoration: none;">red "Execute on my desktop" button shown </ins>in <ins style="font-weight: bold; text-decoration: none;">Figure 2), </ins>the <ins style="font-weight: bold; text-decoration: none;">reader </ins>can zoom, pan, and interactively rotate <ins style="font-weight: bold; text-decoration: none;">any of these </ins>3D-rendered scenes <ins style="font-weight: bold; text-decoration: none;">and explore a wider range of model parameter values</ins>.</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>We'd like to determine which value of <math>\Delta\Omega</math> provides the best measure of the binary star system's true orbital period. <del style="font-weight: bold; text-decoration: none;">As expected, for </del>all five choices of <math>\Delta\Omega</math>, we found the highest velocities (marked by the longest streamlines) along the relatively low-density mass-transfer stream that connects the two stars. Material from the donor star (in the lower half of <del style="font-weight: bold; text-decoration: none;">each </del>rendered image in Figure 2) flows toward its stellar companion, reaching supersonic velocities before impacting the companion. An oblique shock front &#150; whose location is delineated by kinks in the pink, blue, and orange streamlines &#150; terminates the component of motion perpendicular to the companion's surface. Motion transverse to the shock becomes orbital motion in a thick, low-density disk that surrounds the companion star.</div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>We'd like to determine which value of <math>\Delta\Omega</math> provides the best measure of the binary star system's true orbital period. <ins style="font-weight: bold; text-decoration: none;">For </ins>all five choices of <math>\Delta\Omega</math> <ins style="font-weight: bold; text-decoration: none;">identified by the Figure 2 VisMashup App</ins>, we found the highest velocities (marked by the longest streamlines) along the relatively low-density mass-transfer stream that connects the two stars<ins style="font-weight: bold; text-decoration: none;">. This was as expected</ins>. Material from the donor star (in the lower half of <ins style="font-weight: bold; text-decoration: none;">the </ins>rendered image in Figure 2) flows toward its stellar companion, reaching supersonic velocities before impacting the companion. An oblique shock front &#150; whose location is delineated by kinks in the pink, blue, and orange streamlines &#150; terminates the component of motion perpendicular to the companion's surface. Motion transverse to the shock becomes orbital motion in a thick, low-density disk that surrounds the companion star.</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>For all five choices of <math>\Delta\Omega</math>, the flow's behavior in the vicinity of the mass-transfer stream very closely resembles the behavior that Stephen Lubow and Frank Shu predicted more than 30 years ago. Figure 3b shows the magnified view of this region of the flow from our simulation assuming <math>\Delta\Omega = - 0.041</math>. We've reoriented this magnified image and numbered the streamlines to facilitate comparison with the Lubow and Shu illustration, which we've reprinted with permission here (see Figure 3a). Rather than conducting a fully self-consistent 3D simulation &#150; which was computationally impractical at the time &#150; Lubow and Shu used a mathematical perturbation analysis to estimate what the flow should look like in the vicinity of the "L1" Lagrange point, as viewed from a frame of reference rotating with the correct instantaneous orbital frequency, <math>\Omega_\mathrm{frame}</math>. The close resemblance between our 3D simulation results in the vicinity of the L1 Lagrange point, and the behavior that Lubow and Shu predicted provides a useful point of verification for our work.</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>For all five choices of <math>\Delta\Omega</math>, the flow's behavior in the vicinity of the mass-transfer stream very closely resembles the behavior that Stephen Lubow and Frank Shu predicted more than 30 years ago. Figure 3b shows the magnified view of this region of the flow from our simulation assuming <math>\Delta\Omega = - 0.041</math>. We've reoriented this magnified image and numbered the streamlines to facilitate comparison with the Lubow and Shu illustration, which we've reprinted with permission here (see Figure 3a). Rather than conducting a fully self-consistent 3D simulation &#150; which was computationally impractical at the time &#150; Lubow and Shu used a mathematical perturbation analysis to estimate what the flow should look like in the vicinity of the "L1" Lagrange point, as viewed from a frame of reference rotating with the correct instantaneous orbital frequency, <math>\Omega_\mathrm{frame}</math>. The close resemblance between our 3D simulation results in the vicinity of the L1 Lagrange point, and the behavior that Lubow and Shu predicted provides a useful point of verification for our work.</div></td></tr>
</table>Tohlinehttps://www.vistrails.org//index.php?title=User:Tohline/IVAJ/Levels2and3&diff=2766&oldid=prevTohline: remove excess lines and widen VisMashup "table" from 90% to 95%2010-02-11T21:01:35Z<p>remove excess lines and widen VisMashup "table" from 90% to 95%</p>
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</table>Tohline