<xml>
  <records>
    <record>
       <contributors>
          <authors>
             <author>Kyle, B.S.</author>
             <author>Appleby, R.B.</author>
             <author>Pacey, T.H.</author>
             <author>Williams, P.H.</author>
             <author>Wolfenden, J.</author>
          </authors>
       </contributors>
       <titles>
          <title>
             Pyroelectric Detection of Coherent Radiation on the CLARA Phase 1 Beamline
          </title>
       </titles>
		 <publisher>JACoW Publishing</publisher>
       <pub-location>Geneva, Switzerland</pub-location>
		 <isbn>978-3-95450-184-7</isbn>
		 <electronic-resource-num>10.18429/JACoW-IPAC2018-THPAK140</electronic-resource-num>
		 <language>English</language>
		 <pages>3577-3580</pages>
       <pages>THPAK140</pages>
       <keywords>
       </keywords>
       <work-type>Contribution to a conference proceedings</work-type>
       <dates>
          <year>2018</year>
          <pub-dates>
             <date>2018-06</date>
          </pub-dates>
       </dates>
       <urls>
          <related-urls>
              <url>https://doi.org/10.18429/JACoW-IPAC2018-THPAK140</url>
              <url>http://jacow.org/ipac2018/papers/thpak140.pdf</url>
          </related-urls>
       </urls>
       <abstract>
          The impacts of coherent synchrotron radiation (CSR) and space charge in the bunch compressor section of the CLARA Free Electron Laser (FEL) are expected to be significant, given the relatively high charge and short bunch lengths expected. The General Particle Tracer (GPT) code allows for the modelling of these effects in tandem, presenting an opportunity to more reliably estimate their effects on the CLARA beam. To provide confidence in future studies using GPT, a benchmarking study on the CLARA Phase 1 beamline is presented alongside relevant simulations. This study will make use of pyroelectric detectors to measure the emitted coherent power of the CLARA beam as it passes through a dispersive section whilst varying the chirp imparted on the bunches longitudinal phase space (LPS). Simulations presented demonstrate the viability of such a study, with energies between ∼ 10-100 nJ per pulse expected to be incident upon the detector face.
       </abstract>
    </record>
  </records>
</xml>
