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    <p>Hi Shen,</p>
    <p>It is also my understanding that the k value is the momentum
      transfer.</p>
    <p>Sorry, I do not have the time to look into you problem now.</p>
    <p>best, Kim</p>
    <p><br>
    </p>
    <div class="moz-cite-prefix">On 2/7/19 4:53 PM, <a class="moz-txt-link-abbreviated" href="mailto:ls8vm@virginia.edu">ls8vm@virginia.edu</a>
      wrote:<br>
    </div>
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        <p class="MsoNormal"><span style="font-family:"Times New
            Roman",serif">Hi all,<o:p></o:p></span></p>
        <p class="MsoNormal"><span style="font-family:"Times New
            Roman",serif"><o:p> </o:p></span></p>
        <p class="MsoNormal"><span style="font-family:"Times New
            Roman",serif">            I checked the
            supermirror_m3.rfl file and it ranges from 0 to 0.09
            [Angs-1] so I’m really confused with the k value in the
            first column of reflectivity file. I thought it represent
            the total momentum transferred. Can you explain more on
            “better the k values in the reflectivity file to be around
            e.g. 1.0 Angs-1.” Does the guide_gravity component have a
            different definition on reflectivity file? My actual source
            wavelength ranges from 0 to 10 [Angs].<o:p></o:p></span></p>
        <p class="MsoNormal" style="text-indent:.5in"><span
            style="font-family:"Times New Roman",serif"><o:p> </o:p></span></p>
        <p class="MsoNormal" style="text-indent:.5in"><span
            style="font-family:"Times New Roman",serif">And
            also for Peter, my actual problem is to optimize a polarizer
            which is built by stack of supermirror. I’m trying to find a
            way to get the most transmission through that setup. So I
            want to calculate the ratio neutron_out/neutron_in. Now it
            seems that I should just divide the intensity instead of
            event numbers?<o:p></o:p></span></p>
        <p class="MsoNormal"><span style="font-family:"Times New
            Roman",serif"><o:p> </o:p></span></p>
        <p class="MsoNormal"><span style="font-family:"Times New
            Roman",serif"><o:p> </o:p></span></p>
        <p class="MsoNormal"><span style="font-family:"Times New
            Roman",serif">Happy Lunar New Year,<o:p></o:p></span></p>
        <p class="MsoNormal"><span style="font-family:"Times New
            Roman",serif">Lingnan Shen<o:p></o:p></span></p>
        <p class="MsoNormal"><o:p> </o:p></p>
        <div
          style="mso-element:para-border-div;border:none;border-top:solid
          #E1E1E1 1.0pt;padding:3.0pt 0in 0in 0in">
          <p class="MsoNormal" style="border:none;padding:0in"><b>From:
            </b><a href="mailto:pkwi@fysik.dtu.dk"
              moz-do-not-send="true">Peter Kjær Willendrup</a><br>
            <b>Sent: </b>Tuesday, February 5, 2019 4:20 AM<br>
            <b>To: </b><a href="mailto:ls8vm@virginia.edu"
              moz-do-not-send="true">Lingnan Shen</a><br>
            <b>Cc: </b><a href="mailto:farhi@ill.fr"
              moz-do-not-send="true">Emmanuel Farhi</a><br>
            <b>Subject: </b>Re: [mcstas-users] Guide_gravity Problem</p>
        </div>
        <p class="MsoNormal"><o:p> </o:p></p>
        <p class="MsoNormal">Hello again, <o:p></o:p></p>
        <div>
          <p class="MsoNormal"><o:p> </o:p></p>
        </div>
        <div>
          <p class="MsoNormal"><o:p> </o:p></p>
        </div>
        <div>
          <p class="MsoNormal">A better starting point for understanding
            Guide_gravity and reflectivity files may be the instrument
            file Test_Guides which is included with your McStas
            installation, in combination with one of the example
            reflectivity files from the data folder - e.g.
            supermirror_m3.rdl.<o:p></o:p></p>
        </div>
        <div>
          <p class="MsoNormal"><o:p> </o:p></p>
        </div>
        <div>
          <p class="MsoNormal">Also, for a pencil beam with controllable
            divergence, an option is to use Source_div.<o:p></o:p></p>
        </div>
        <div>
          <p class="MsoNormal"><o:p> </o:p></p>
        </div>
        <div>
          <p class="MsoNormal">Hope this helps - otherwise you are
            welcome to write again, preferably with a good description
            of what exact problem you are trying to solve. :-)<o:p></o:p></p>
        </div>
        <div>
          <p class="MsoNormal"><o:p> </o:p></p>
        </div>
        <div>
          <p class="MsoNormal">Best,<o:p></o:p></p>
        </div>
        <div>
          <p class="MsoNormal"><o:p> </o:p></p>
        </div>
        <div>
          <p class="MsoNormal">Peter<o:p></o:p></p>
          <div>
            <p class="MsoNormal"><br>
              <br>
              <o:p></o:p></p>
            <blockquote style="margin-top:5.0pt;margin-bottom:5.0pt">
              <div>
                <p class="MsoNormal">On 5 Feb 2019, at 10.12, Peter Kjær
                  Willendrup <<a href="mailto:pkwi@fysik.dtu.dk"
                    moz-do-not-send="true">pkwi@fysik.dtu.dk</a>>
                  wrote:<o:p></o:p></p>
              </div>
              <p class="MsoNormal"><o:p> </o:p></p>
              <div>
                <div>
                  <p class="MsoNormal">Hello Lingnan, <o:p></o:p></p>
                  <div>
                    <p class="MsoNormal"><o:p> </o:p></p>
                  </div>
                  <div>
                    <p class="MsoNormal"><o:p> </o:p></p>
                  </div>
                  <div>
                    <div>
                      <p class="MsoNormal">Agree with Emmanuel. <o:p></o:p></p>
                    </div>
                    <div>
                      <p class="MsoNormal"><o:p> </o:p></p>
                    </div>
                    <div>
                      <p class="MsoNormal">Further, the combination of a
                        pencil-beam, i.e. almost non-divergent source
                        and using 500 channels in a rotated
                        Guide_gravity means that transport through the
                        guide becomes close to impossible. <o:p></o:p></p>
                    </div>
                    <div>
                      <p class="MsoNormal"><o:p> </o:p></p>
                    </div>
                    <div>
                      <p class="MsoNormal">With regard to your second
                        question you should always consider the
                        transported intensity I. The event count is
                        simply a measure of statistics (of "neutron
                        rays", not “neutrons”).<o:p></o:p></p>
                    </div>
                    <div>
                      <p class="MsoNormal"><o:p> </o:p></p>
                    </div>
                    <div>
                      <p class="MsoNormal"><o:p> </o:p></p>
                    </div>
                    <div>
                      <p class="MsoNormal">Best,<o:p></o:p></p>
                    </div>
                    <div>
                      <p class="MsoNormal"><o:p> </o:p></p>
                    </div>
                    <div>
                      <p class="MsoNormal">Peter Willendrup<o:p></o:p></p>
                    </div>
                    <div>
                      <p class="MsoNormal"><o:p> </o:p></p>
                    </div>
                    <div>
                      <p class="MsoNormal"><o:p> </o:p></p>
                    </div>
                    <div>
                      <blockquote
                        style="margin-top:5.0pt;margin-bottom:5.0pt">
                        <div>
                          <p class="MsoNormal">On 5 Feb 2019, at 10.01,
                            Emmanuel FARHI <<a
                              href="mailto:farhi@ill.fr"
                              moz-do-not-send="true">farhi@ill.fr</a>>
                            wrote:<o:p></o:p></p>
                        </div>
                        <p class="MsoNormal"><o:p> </o:p></p>
                        <div>
                          <div>
                            <p class="MsoNormal"
                              style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto">Hello
                              Lingnan,</p>
                            <p class="MsoNormal"
                              style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto">Your
                              reflectivity file is given for k=0 to 0.14
                              Angs-1. This is very small and covers
                              neutrons around lambda=60 Angs, which are
                              not even created by your source. Change
                              either the lambda setting at the source,
                              or better the k values in the reflectivity
                              file to be around e.g. 1.0 Angs-1.</p>
                            <p class="MsoNormal"
                              style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto">Cheers,
                              Emmanuel.</p>
                            <p class="MsoNormal"
                              style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto"><o:p> </o:p></p>
                            <div>
                              <p class="MsoNormal">On 2/5/19 7:17 AM,
                                Lingnan Shen wrote:<o:p></o:p></p>
                            </div>
                            <blockquote
                              style="margin-top:5.0pt;margin-bottom:5.0pt">
                              <div>
                                <p class="MsoNormal">Hi all, <o:p></o:p></p>
                                <div>
                                  <p class="MsoNormal"><o:p> </o:p></p>
                                </div>
                                <div>
                                  <p class="MsoNormal">        I was
                                    trying to learn how to use the
                                    guide_gravity component. I tried to
                                    define the reflectivity curve but I
                                    get zero neutrons at the wavelength
                                    monitor in the end of guide. I have
                                    attached my .instr and .rfl file. I
                                    also found that even if the neutron
                                    beam just go through the guide. The
                                    detector at the end still see
                                    nothing.<o:p></o:p></p>
                                </div>
                                <div>
                                  <p class="MsoNormal">        Also
                                    another question about transmission
                                    of certain setup. To calculate the
                                    ratio of neutron_in / neutron_out. I
                                    want to know how much neutron
                                    remained after passing through that
                                    setup. Should I use the flux or the
                                    events count?<o:p></o:p></p>
                                </div>
                                <div>
                                  <p class="MsoNormal"><o:p> </o:p></p>
                                </div>
                                <div>
                                  <p class="MsoNormal">Sincerely,<o:p></o:p></p>
                                </div>
                                <div>
                                  <p class="MsoNormal">Lingnan Shen<o:p></o:p></p>
                                </div>
                              </div>
                              <p class="MsoNormal"><br>
                                <br>
                                <o:p></o:p></p>
                              <pre>_______________________________________________</pre>
                              <pre>mcstas-users mailing list</pre>
                              <pre><a href="mailto:mcstas-users@mcstas.org" moz-do-not-send="true">mcstas-users@mcstas.org</a></pre>
                              <pre><a href="https://mailman2.mcstas.org/mailman/listinfo/mcstas-users" moz-do-not-send="true">https://mailman2.mcstas.org/mailman/listinfo/mcstas-users</a></pre>
                            </blockquote>
                            <pre>-- </pre>
                            <pre>Emmanuel FARHI,                                           \|/ ____ \|/</pre>
                            <pre>Spectroscopy Group Institut Laue-Langevin (ILL) Grenoble  ~@-/ oO \-@~</pre>
                            <pre>71 av des Martyrs,CS 20156,38042 Grenoble Cedex 9,France  /_( \__/ )_\</pre>
                            <pre>Work :Tel (33/0) 4 76 20 71 35. Fax (33/0) 4 76 48 39 06     \__U_/ </pre>
                          </div>
                          <p class="MsoNormal">_______________________________________________<br>
                            mcstas-users mailing list<br>
                            <a href="mailto:mcstas-users@mcstas.org"
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                              moz-do-not-send="true">https://mailman2.mcstas.org/mailman/listinfo/mcstas-users</a><o:p></o:p></p>
                        </div>
                      </blockquote>
                    </div>
                    <p class="MsoNormal"><o:p> </o:p></p>
                    <div>
                      <div>
                        <p class="MsoNormal"
                          style="margin-bottom:12.0pt"><span
                            style="font-size:9.0pt;font-family:"Helvetica",sans-serif"><br>
                            Peter Kjær Willendrup<br>
                            Forskningsingeniør, Specialkonsulent<br>
                            Næstformand for DTU Fysik LSU<br>
                            <br>
                            DTU Physics<o:p></o:p></span></p>
                      </div>
                      <p class="MsoNormal"><span
                          style="font-size:9.0pt;font-family:"Helvetica",sans-serif"><br>
                          <image001.gif><br>
                          <br>
                          <br>
                          Technical University of Denmark<br>
                          <br>
                          <br>
                          <image002.gif><br>
                          <br>
                          <br>
                          <br>
                          Department of Physics<br>
                          Fysikvej<br>
                          Building 307<br>
                          DK-2800 Kongens Lyngby<br>
                          Direct +45 2125 4612<br>
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                            moz-do-not-send="true">pkwi@fysik.dtu.dk</a>
                        </span><o:p></o:p></p>
                    </div>
                    <p class="MsoNormal"><o:p> </o:p></p>
                  </div>
                </div>
              </div>
            </blockquote>
          </div>
          <p class="MsoNormal"><o:p> </o:p></p>
          <div>
            <div>
              <p class="MsoNormal" style="margin-bottom:12.0pt"><span
style="font-size:9.0pt;font-family:"Helvetica",sans-serif;color:black"><br>
                  Peter Kjær Willendrup<br>
                  Forskningsingeniør, Specialkonsulent<br>
                  Næstformand for DTU Fysik LSU<br>
                  <br>
                  DTU Physics<o:p></o:p></span></p>
            </div>
            <p class="MsoNormal"><span
style="font-size:9.0pt;font-family:"Helvetica",sans-serif;color:black"><br>
                <img style="width:4.1666in;height:.0104in"
                  id="_x0037_F2B9384-5B9D-4EB7-89FC-07916BD8CDEA"
                  src="cid:b6339554-7f28-441d-9f31-5944f811397c@win.dtu.dk"
alt="cid:b6339554-7f28-441d-9f31-5944f811397c@win.dtu.dk"
                  moz-do-not-send="true" width="400" height="1"
                  border="0"><br>
                <br>
                <br>
                Technical University of Denmark<br>
                <br>
                <br>
                <img style="width:.375in;height:.552in"
                  id="E6FBFD88-6E07-4AB2-AEDD-6E71B78B1972"
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alt="cid:e108e480-fcab-46e2-9531-b38165079572@win.dtu.dk"
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                Department of Physics<br>
                Fysikvej<br>
                Building 307<br>
                DK-2800 Kongens Lyngby<br>
                Direct +45 2125 4612<br>
                Mobil +45 2125 4612<br>
                Fax +45 4593 2399<br>
                <a href="mailto:pkwi@fysik.dtu.dk"
                  moz-do-not-send="true">pkwi@fysik.dtu.dk</a> </span><o:p></o:p></p>
          </div>
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        <p class="MsoNormal"><o:p> </o:p></p>
        <p class="MsoNormal"><o:p> </o:p></p>
      </div>
      <br>
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      <pre class="moz-quote-pre" wrap="">_______________________________________________
mcstas-users mailing list
<a class="moz-txt-link-abbreviated" href="mailto:mcstas-users@mcstas.org">mcstas-users@mcstas.org</a>
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</pre>
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