<?xml version="1.0" encoding="UTF-8"?>
<xml>
  <records>
    <record>
       <contributors>
          <authors>
             <author>Parajuli, I.P.</author>
             <author>Ciovati, G.</author>
             <author>Delayen, J.R.</author>
             <author>Gurevich, A.V.</author>
          </authors>
       </contributors>
       <titles>
          <title>
             Magnetic Field Mapping of a Large-Grain 1.3 GHz Single-Cell Cavity
          </title>
       </titles>
       <publisher>JACoW Publishing</publisher>
       <pub-location>Geneva, Switzerland</pub-location>
		 <isbn>2673-5504</isbn>
		 <isbn>978-3-95450-234-9</isbn>
		 <electronic-resource-num>10.18429/JACoW-SRF2023-MOPMB036</electronic-resource-num>
		 <language>English</language>
		 <pages>172-177</pages>
       <keywords>
          <keyword>cavity</keyword>
          <keyword>radio-frequency</keyword>
          <keyword>niobium</keyword>
          <keyword>SRF</keyword>
          <keyword>cryogenics</keyword>
       </keywords>
       <work-type>Contribution to a conference proceedings</work-type>
       <dates>
          <year>2023</year>
          <pub-dates>
             <date>2023-09</date>
          </pub-dates>
       </dates>
       <urls>
          <related-urls>
              <url>https://doi.org/10.18429/JACoW-SRF2023-MOPMB036</url>
              <url>https://jacow.org/srf2023/papers/mopmb036.pdf</url>
          </related-urls>
       </urls>
       <abstract>
          A new magnetic field mapping system for 1.3 GHz single-cell cavities was developed in order to reveal the impact of ambient magnetic field and temperature gradients during cool-down on the flux trapping phenomenon. Measurements were done at 2 K for different cool-down conditions of a large-grain cavity before and after 120 °C bake. The fraction of applied magnetic field trapped in the cavity walls was ~ 50% after slow cool-down and ~20% after fast cool-down. The results showed a weak correlation between between trapped flux locations and hot-spots causing the high-field Q-slope. The results also showed an increase of the trapped flux at the quench location, after quenching, and a local redistribution of trapped flux with increasing RF field.
       </abstract>
    </record>
  </records>
</xml>
