<div dir="ltr">Dear Latifa<br><div><br></div><div>I can launch the full decoding after 4013 to store on volatile, but I think the actual procedure to process such a large amount of data should be:</div><div>- decode a few set of runs</div><div>- cook those runs<br></div><div>- filter those runs keeping the dst on work</div><div><br></div><div>Best regards</div><div>FX</div></div><br><div class="gmail_quote"><div dir="ltr">On Sat, Jun 23, 2018 at 10:55 AM Latifa Elouadrhiri <<a href="mailto:latifa@jlab.org">latifa@jlab.org</a>> wrote:<br></div><blockquote class="gmail_quote" style="margin:0 0 0 .8ex;border-left:1px #ccc solid;padding-left:1ex">
  
    
  
  <div bgcolor="#FFFFFF" text="#000000">
    <p>Dear Francois,</p>
    <p>We need to go ahead and decode all the data after 4013 we need to
      be able to process as much statistics as possible, once the
      reconstruction code is ready. Some proposed abstracts to DNP need
      a lot of statistics to show something. However we need to make
      sure that there will be no changes to the code that would require
      decoding.<br>
    </p>
    <p>I don't know where the list that Will developed came from.</p>
    <p>Best regards,</p>
    <p>Latifa<br>
    </p>
    <br>
    <div class="m_-1625372750689416772moz-cite-prefix">On 6/23/18 3:56 PM, L Smith wrote:<br>
    </div>
    <blockquote type="cite">
      
      Francois,
      <div><br>
      </div>
      <div>Could you add a few later runs to your
        decode/cooking?  So I can extend my gain drift study.</div>
      <div><br>
      </div>
      <div>4177 (75 nA)</div>
      <div>4178 (50 nA)</div>
      <div>4264 (50 nA)</div>
      <div>4326 (50 nA)</div>
      <div><br>
      </div>
      <div>Thanks, Cole<br>
        <div><br>
          <blockquote type="cite">
            <div>On Jun 22, 2018, at 5:08 PM, Francois-Xavier
              Girod <<a href="mailto:fxgirod@jlab.org" target="_blank">fxgirod@jlab.org</a>> wrote:</div>
            <br class="m_-1625372750689416772Apple-interchange-newline">
            <div>
              <div dir="ltr">Dear all<br>
                <div><br>
                </div>
                <div>If we have a list of runs, we can already
                  launch decoding this weekend I think</div>
                <div><br>
                </div>
                <div>Best regards</div>
                <div>FX</div>
              </div>
              <br>
              <div class="gmail_quote">
                <div dir="ltr">On Fri, Jun 22, 2018 at 1:45 PM
                  Daniel Carman <<a href="mailto:carman@jlab.org" target="_blank">carman@jlab.org</a>>
                  wrote:<br>
                </div>
                <blockquote class="gmail_quote" style="margin:0 0 0 .8ex;border-left:1px #ccc solid;padding-left:1ex">
                  <div style="word-wrap:break-word;line-break:after-white-space">Folks,
                    <div><br>
                    </div>
                    <div>The pass-0 cooking for RG-A will
                      commence very shortly. Today at our weekly CALCOM </div>
                    <div>meeting we had an important discussion
                      on run-based monitoring. While we do not yet </div>
                    <div>have a fully realized service to
                      extract and present the relevant subsystem
                      quantities as</div>
                    <div>a function of run number to help us
                      determine the stability of the calibrations, we
                      are not</div>
                    <div>without at least a set of tools that
                      we will use for the time being.</div>
                    <div><br>
                    </div>
                    <div>This email is a call to action for all
                      system groups to complete a few things over the
                      next</div>
                    <div>several days in advance of the
                      availability of the output of the pass-0 cooking:</div>
                    <div><br>
                    </div>
                    <div>1). Review the list of quantities that
                      we would like to monitor for each subsystem. The</div>
                    <div>present list of these quantities is
                      located at:</div>
                    <div><a href="https://clasweb.jlab.org/wiki/images/2/27/Run-based-monitoring.pdf" target="_blank">https://clasweb.jlab.org/wiki/images/2/27/Run-based-monitoring.pdf</a></div>
                    <div>This list is based on what has been
                      provided from the subsystem groups earlier this
                      year.</div>
                    <div><br>
                    </div>
                    <div>2). Review the list of reconstruction
                      monitoring plots that have been defined. You can</div>
                    <div>find the current set of subsystem
                      plots at:</div>
                    <div><a href="https://clasweb.jlab.org/wiki/images/b/bf/Girod_Fri220618.pdf" target="_blank">https://clasweb.jlab.org/wiki/images/b/bf/Girod_Fri220618.pdf</a></div>
                    <div>Please review these plots to be sure
                      that the quantities listed in item 1) above can be</div>
                    <div>derived from these reconstruction
                      monitoring plots. It is also important that if you
                      need</div>
                    <div>specific histograms fit and parameters
                      extracted for run-by-run monitoring, that you</div>
                    <div>provide this information. Depending on
                      the complexity of the quantities, we will then</div>
                    <div>have to make a determination of
                      quantities can be extracted.</div>
                    <div><br>
                    </div>
                    <div>Note that for the time being we will
                      not have monitoring on a channel-by-channel basis.</div>
                    <div>We also need to keep the number of
                      plots and quantities to monitor finite for each
                      subsystem.</div>
                    <div><br>
                    </div>
                    <div>Please respond to this email by
                      Wednesday morning so that we can continue to
                      prepare</div>
                    <div>the monitoring tools for pass-0 and
                      test our system out. If you have questions, please
                      let</div>
                    <div>me know.</div>
                    <div><br>
                    </div>
                    <div>Regards,</div>
                    <div>Daniel</div>
                    <div>
                      <div>
                        <div style="font-family:Helvetica;font-size:14px;font-style:normal;font-variant-caps:normal;font-weight:normal;letter-spacing:normal;text-align:start;text-indent:0px;text-transform:none;white-space:normal;word-spacing:0px;text-decoration:none"><br class="m_-1625372750689416772m_-2806711546182164170Apple-interchange-newline">
***********************************************************************************<br>
                          *                                             
                                                                       
                                                *<br>
                          * Dr. Daniel S. Carman                  <a href="mailto:carman@jlab.org" target="_blank">e-mail :
                            carman@jlab.org</a>                     *  <br>
                          * Staff Scientist                           
                            office : (757)-269-5586                     
                             *<br>
                          * Jefferson Laboratory                   web: <a href="http://userweb.jlab.org/%7Ecarman" target="_blank">http://userweb.jlab.org/~carman</a>
                           *  <br>
                          *                                             
                                                                       
                                                *<br>
***********************************************************************************</div>
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