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<xml>
  <records>
    <record>
       <contributors>
          <authors>
             <author>Leemann, S.C.</author>
             <author>Byrne, W.E.</author>
             <author>Cuneo, D.P.</author>
             <author>Ehrlichman, M.P.</author>
             <author>Hellert, T.</author>
             <author>Hexemer, A.</author>
             <author>Lu, Y.</author>
             <author>Marcus, M.</author>
             <author>Melton, C.N.</author>
             <author>Nishimura, H.</author>
             <author>Penn, G.</author>
             <author>Sannibale, F.</author>
             <author>Shapiro, D.A.</author>
             <author>Sun, C.</author>
             <author>Ushizima, D.</author>
             <author>Venturini, M.</author>
             <author>Wallén, E.J.</author>
          </authors>
       </contributors>
       <titles>
          <title>
             Applying Machine Learning to Stabilize the Source Size in the ALS Storage Ring
          </title>
       </titles>
       <publisher>JACoW Publishing</publisher>
       <pub-location>Geneva, Switzerland</pub-location>
       <abstract>
          In state-of-the-art synchrotron light sources the overall source stability is presently limited by the achievable level of electron beam size stability. This source size stability is presently on the few-percent level, which is still 1–2 orders of magnitude larger than already demonstrated stability of source position/angle (slow/fast orbit feedbacks) and current (top-off injection). Until now source size stabilization has been achieved through corrections based on a combination of static predetermined physics models and lengthy calibration measurements (feed-forward tables), periodically repeated to counteract drift in the accelerator and instrumentation. We now demonstrate for the first time* how application of machine learning allows for a physics- and model-independent stabilization of source size relying only on previously existing instrumentation in ALS. Such feed-forward correction based on neural networks that can be continuously online-retrained achieves source size stability as low as 0.2 microns rms (0.4%) which results in overall source stability approaching the sub-percent noise floor of the most sensitive experiments.
       </abstract>
    </record>
  </records>
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