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      <br>
      -------- Forwarded Message --------
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            <th nowrap="nowrap" valign="BASELINE" align="RIGHT">Subject:
            </th>
            <td>Plasma Theory/Nonlinear Dynamics Seminar: "Symplectic
              and Variational Integration" - John M. Finn</td>
          </tr>
          <tr>
            <th nowrap="nowrap" valign="BASELINE" align="RIGHT">Date: </th>
            <td>Thu, 5 Apr 2018 18:43:46 +0000</td>
          </tr>
          <tr>
            <th nowrap="nowrap" valign="BASELINE" align="RIGHT">From: </th>
            <td>Wilkinson, Ellie V <a class="moz-txt-link-rfc2396E" href="mailto:evwilk@wm.edu"><evwilk@wm.edu></a></td>
          </tr>
          <tr>
            <th nowrap="nowrap" valign="BASELINE" align="RIGHT">To: </th>
            <td><a class="moz-txt-link-abbreviated" href="mailto:physics2017@physics.wm.edu">physics2017@physics.wm.edu</a>
              <a class="moz-txt-link-rfc2396E" href="mailto:physics2017@physics.wm.edu"><physics2017@physics.wm.edu></a></td>
          </tr>
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            <th nowrap="nowrap" valign="BASELINE" align="RIGHT">CC: </th>
            <td><a class="moz-txt-link-abbreviated" href="mailto:undergrads2017@physics.wm.edu">undergrads2017@physics.wm.edu</a>
              <a class="moz-txt-link-rfc2396E" href="mailto:undergrads2017@physics.wm.edu"><undergrads2017@physics.wm.edu></a></td>
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            v:shapes="Picture_x0020_1" class="" align="left" hspace="12"
            height="242" width="191"><!--[endif]--><b><u><span
                style="font-size:12.0pt;font-family:"Times New
                Roman",serif;color:#00B050">Plasma Theory/Nonlinear
                Dynamics Seminar</span></u></b><span
            style="font-size:12.0pt"><o:p></o:p></span></p>
        <p class="MsoNormal"><span
            style="font-size:12.0pt;font-family:"Times New
            Roman",serif">Wednesday, April 11, 2018<o:p></o:p></span></p>
        <p class="MsoNormal"><span
            style="font-size:12.0pt;font-family:"Times New
            Roman",serif">12:00 PM
            <o:p></o:p></span></p>
        <p class="MsoNormal"><span
            style="font-size:12.0pt;font-family:"Times New
            Roman",serif">Small Hall, Room 235<o:p></o:p></span></p>
        <p class="MsoNormal"><span
            style="font-size:12.0pt;font-family:"Times New
            Roman",serif"> <o:p></o:p></span></p>
        <p class="MsoNormal"><b><span
              style="font-size:12.0pt;font-family:"Times New
              Roman",serif;color:#00B050">John M. Finn
            </span></b><span
            style="font-size:12.0pt;font-family:"Times New
            Roman",serif">[Host: E. Tracy]<b>
            </b><o:p></o:p></span></p>
        <p class="MsoNormal"><span
            style="font-size:12.0pt;font-family:"Times New
            Roman",serif">Tibbar Plasma Technologies; Los Alamos
            National Laboratory (retired)<o:p></o:p></span></p>
        <p class="MsoNormal"><span style="font-size:12.0pt"><o:p> </o:p></span></p>
        <p class="MsoNormal"><b><span
              style="font-size:12.0pt;font-family:"Times New
              Roman",serif"> Title of Talk:  </span></b><b><span
              style="font-size:14.0pt;font-family:"Times New
              Roman",serif;color:#00B050">“Symplectic and
              Variational Integration”</span></b><b><span
              style="font-size:12.0pt;font-family:"Times New
              Roman",serif"><o:p></o:p></span></b></p>
        <p class="MsoNormal"><b><span style="font-size:12.0pt"><o:p> </o:p></span></b></p>
        <p class="MsoNormal"><span
            style="font-size:12.0pt;font-family:"Times New
            Roman",serif"><br>
            <br>
            <br>
            <b><span style="color:#00B050">Abstract:</span></b> In the
            context of canonical Hamiltonian systems, variational
            integrators provide an alternative way of deriving
            symplectic integrators. Variational integrators can be
            formed by discretizing the action based on a conventional
            configuration space Lagrangian, or alternately based on
            discretizing a phase space action principle. A phase space
            action principle leads to an ODE system which is degenerate,
            producing the first order canonical Hamiltonian equations of
            motion. A haphazard discretization can lead to discrete
            equations that are higher order in time, allowing for
            parasitic modes, which can be unstable. More careful
            discretizations can lead to a system which is properly
            degenerate. I present a review of these concepts and extend
            them to two noncanonical systems of interest in plasma
            physics, namely magnetic field lines and the guiding center
            equations of motion. A major outcome of this work is that
            for the discrete system to be properly degenerate, there is
            a straightforward test, based on the discrete form of the
            Hessian.<o:p></o:p></span></p>
        <p class="MsoNormal"><span
            style="font-size:12.0pt;font-family:"Times New
            Roman",serif"><o:p> </o:p></span></p>
        <p class="MsoNormal"><b><span
              style="font-size:12.0pt;font-family:"Times New
              Roman",serif;color:#00B050">Speaker Bio:</span></b><span
            style="font-size:12.0pt;font-family:"Times New
            Roman",serif;color:#00B050">
          </span><span style="font-size:12.0pt;font-family:"Times
            New Roman",serif">John M. Finn received his PhD from
            the University of Maryland in 1974. He worked at the Naval
            Research Laboratory, at the University of Maryland and,
            since 1993, at Los ALamos National Laboratory. He retired
            from LANL in 2016 to form the startup Tibbar Plasma
            Technologies, Inc. His research has been in plasma physics,
            for application to magnetic fusion as well as solar and
            astrophysical problems, with a focus on the application of
            Dynamical Systems to plasmas.<o:p></o:p></span></p>
        <p class="MsoNormal"><span
            style="font-size:12.0pt;font-family:"Times New
            Roman",serif"><br>
            Everyone is invited.<o:p></o:p></span></p>
        <p class="MsoNormal"><span
            style="font-size:12.0pt;font-family:"Times New
            Roman",serif"><o:p> </o:p></span></p>
        <p class="MsoNormal"><o:p> </o:p></p>
        <p class="MsoNormal"><span
            style="font-size:10.0pt;font-family:"Times New
            Roman",serif;color:black">******</span><span
            style="color:black"><o:p></o:p></span></p>
        <p class="MsoNormal"><b><span
              style="font-size:12.0pt;font-family:"Monotype
              Corsiva";color:#1F497D">Eleonor V. Wilkinson</span></b><span
            style="color:black"><o:p></o:p></span></p>
        <p class="MsoNormal"><span
style="font-size:9.0pt;font-family:"Georgia",serif;color:black">Administrative
            & Office Specialist
          </span><span style="color:black"><o:p></o:p></span></p>
        <p class="MsoNormal"><span
style="font-size:9.0pt;font-family:"Georgia",serif;color:black">The
            College of William & Mary-Physics<br>
            Small Hall, Room 123<br>
            300 Ukrop Way<br>
            Williamsburg, VA 23185</span><span style="color:black"><o:p></o:p></span></p>
        <p class="MsoNormal"><span
            style="font-size:9.0pt;font-family:"Times New
            Roman",serif;color:black">Telephone: 757-221-3503</span><span
            style="color:black"><o:p></o:p></span></p>
        <p class="MsoNormal"><span
            style="font-size:9.0pt;font-family:"Times New
            Roman",serif;color:black">Fax: 757-221-3540</span><span
            style="color:black"><o:p></o:p></span></p>
        <p class="MsoPlainText"> <o:p></o:p></p>
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