<?xml version="1.0" encoding="UTF-8"?>
<collection xmlns="http://www.loc.gov/MARC21/slim">
 <record>
  <leader>     caa a22        4500</leader>
  <controlfield tag="001">445830379</controlfield>
  <controlfield tag="003">CHVBK</controlfield>
  <controlfield tag="005">20180317145313.0</controlfield>
  <controlfield tag="007">cr unu---uuuuu</controlfield>
  <controlfield tag="008">170323e20110401xx      s     000 0 eng  </controlfield>
  <datafield tag="024" ind1="7" ind2="0">
   <subfield code="a">10.1007/s10686-010-9211-4</subfield>
   <subfield code="2">doi</subfield>
  </datafield>
  <datafield tag="035" ind1=" " ind2=" ">
   <subfield code="a">(NATIONALLICENCE)springer-10.1007/s10686-010-9211-4</subfield>
  </datafield>
  <datafield tag="245" ind1="0" ind2="0">
   <subfield code="a">Similarity model of feed support system for FAST</subfield>
   <subfield code="h">[Elektronische Daten]</subfield>
   <subfield code="c">[XiaoQiang Tang, WenBai Zhu, CaiHong Sun, Rui Yao]</subfield>
  </datafield>
  <datafield tag="520" ind1="3" ind2=" ">
   <subfield code="a">A new design of feed support system for Five hundred meter Aperture Spherical Telescope (FAST) is proposed in this paper. According to the similarity theory, a 1:15 scale model of feed support system has been built to make systemic research on the feasibility of the system. Then the control system and hardware structure of the feed support system are illustrated. A complete astronomical observation track is run by the scale model and the experiments results demonstrate that the new feed support system can satisfy the observation accuracy requirement of FAST.</subfield>
  </datafield>
  <datafield tag="540" ind1=" " ind2=" ">
   <subfield code="a">Springer Science+Business Media B.V., 2011</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">Feed support system</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">Similarity model</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">Large radio telescope</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">FAST</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Tang</subfield>
   <subfield code="D">XiaoQiang</subfield>
   <subfield code="u">Department of Precision Instrument &amp; Mechanology, Tsinghua University, 100084, Beijing, People's Republic of China</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Zhu</subfield>
   <subfield code="D">WenBai</subfield>
   <subfield code="u">National Astronomical Observatories, CAS, 100012, Beijing, People's Republic of China</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Sun</subfield>
   <subfield code="D">CaiHong</subfield>
   <subfield code="u">National Astronomical Observatories, CAS, 100012, Beijing, People's Republic of China</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Yao</subfield>
   <subfield code="D">Rui</subfield>
   <subfield code="u">National Astronomical Observatories, CAS, 100012, Beijing, People's Republic of China</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="773" ind1="0" ind2=" ">
   <subfield code="t">Experimental Astronomy</subfield>
   <subfield code="d">Springer Netherlands</subfield>
   <subfield code="g">29/3(2011-04-01), 177-187</subfield>
   <subfield code="x">0922-6435</subfield>
   <subfield code="q">29:3&lt;177</subfield>
   <subfield code="1">2011</subfield>
   <subfield code="2">29</subfield>
   <subfield code="o">10686</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2="0">
   <subfield code="u">https://doi.org/10.1007/s10686-010-9211-4</subfield>
   <subfield code="q">text/html</subfield>
   <subfield code="z">Onlinezugriff via DOI</subfield>
  </datafield>
  <datafield tag="908" ind1=" " ind2=" ">
   <subfield code="D">1</subfield>
   <subfield code="a">research-article</subfield>
   <subfield code="2">jats</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">856</subfield>
   <subfield code="E">40</subfield>
   <subfield code="u">https://doi.org/10.1007/s10686-010-9211-4</subfield>
   <subfield code="q">text/html</subfield>
   <subfield code="z">Onlinezugriff via DOI</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Tang</subfield>
   <subfield code="D">XiaoQiang</subfield>
   <subfield code="u">Department of Precision Instrument &amp; Mechanology, Tsinghua University, 100084, Beijing, People's Republic of China</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Zhu</subfield>
   <subfield code="D">WenBai</subfield>
   <subfield code="u">National Astronomical Observatories, CAS, 100012, Beijing, People's Republic of China</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Sun</subfield>
   <subfield code="D">CaiHong</subfield>
   <subfield code="u">National Astronomical Observatories, CAS, 100012, Beijing, People's Republic of China</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Yao</subfield>
   <subfield code="D">Rui</subfield>
   <subfield code="u">National Astronomical Observatories, CAS, 100012, Beijing, People's Republic of China</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">773</subfield>
   <subfield code="E">0-</subfield>
   <subfield code="t">Experimental Astronomy</subfield>
   <subfield code="d">Springer Netherlands</subfield>
   <subfield code="g">29/3(2011-04-01), 177-187</subfield>
   <subfield code="x">0922-6435</subfield>
   <subfield code="q">29:3&lt;177</subfield>
   <subfield code="1">2011</subfield>
   <subfield code="2">29</subfield>
   <subfield code="o">10686</subfield>
  </datafield>
  <datafield tag="900" ind1=" " ind2="7">
   <subfield code="a">Metadata rights reserved</subfield>
   <subfield code="b">Springer special CC-BY-NC licence</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="898" ind1=" " ind2=" ">
   <subfield code="a">BK010053</subfield>
   <subfield code="b">XK010053</subfield>
   <subfield code="c">XK010000</subfield>
  </datafield>
  <datafield tag="949" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="F">NATIONALLICENCE</subfield>
   <subfield code="b">NL-springer</subfield>
  </datafield>
 </record>
</collection>
