<?xml version="1.0" encoding="UTF-8"?>
<collection xmlns="http://www.loc.gov/MARC21/slim">
 <record>
  <leader>     caa a22        4500</leader>
  <controlfield tag="001">469077220</controlfield>
  <controlfield tag="003">CHVBK</controlfield>
  <controlfield tag="005">20180323132938.0</controlfield>
  <controlfield tag="007">cr unu---uuuuu</controlfield>
  <controlfield tag="008">170328e19920901xx      s     000 0 eng  </controlfield>
  <datafield tag="024" ind1="7" ind2="0">
   <subfield code="a">10.1007/BF02507846</subfield>
   <subfield code="2">doi</subfield>
  </datafield>
  <datafield tag="035" ind1=" " ind2=" ">
   <subfield code="a">(NATIONALLICENCE)springer-10.1007/BF02507846</subfield>
  </datafield>
  <datafield tag="100" ind1="1" ind2=" ">
   <subfield code="a">Linsley</subfield>
   <subfield code="D">J.</subfield>
   <subfield code="u">Istituto di Fisica Cosmica ed Applicazioni dell'Informatica del CNR, Palermo, Italia</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="245" ind1="1" ind2="0">
   <subfield code="a">Interpretation of EAS observations by time-track complementarity (TTC)</subfield>
   <subfield code="h">[Elektronische Daten]</subfield>
   <subfield code="c">[J. Linsley]</subfield>
  </datafield>
  <datafield tag="520" ind1="3" ind2=" ">
   <subfield code="a">Summary: Attention is called to a time-track complementarity principle, which is shown to underlie the experimental methods used in a large class of extensive air shower (EAS) observations. A description is given of the Utah Fly's Eye, an important existing device which records both time and track information from individual EAS. In view of contemplated changes that would enable simultaneous recording of time and track information for individual EAS secondary particles in the Palermo-Leeds STAR CLUSTER array, a discussion is given, based on the TTC principle, of phenomena expected to be observed in case of small, nearby showers such as those which trigger the neighbouring GREX scintillator array. Finally, an application of small arrays made of time-track detectors is described, in a mode resembling operation of the Fly's Eye, suggesting that such arrays may have better performance at lower cost than existing alternatives, for the purpose of studying &lt;&lt;giant&gt;&gt; EAS, with energy &gt;(1018÷1019) eV.</subfield>
  </datafield>
  <datafield tag="540" ind1=" " ind2=" ">
   <subfield code="a">Società Italiana di Fisica, 1992</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">Cascade studies ( e.g. , extensive air showers)</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">Cosmic-ray interactions</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="773" ind1="0" ind2=" ">
   <subfield code="t">Il Nuovo Cimento C</subfield>
   <subfield code="d">Kluwer Academic Publishers</subfield>
   <subfield code="g">15/5(1992-09-01), 743-749</subfield>
   <subfield code="x">0390-5551</subfield>
   <subfield code="q">15:5&lt;743</subfield>
   <subfield code="1">1992</subfield>
   <subfield code="2">15</subfield>
   <subfield code="o">11543</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2="0">
   <subfield code="u">https://doi.org/10.1007/BF02507846</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/BF02507846</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">100</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Linsley</subfield>
   <subfield code="D">J.</subfield>
   <subfield code="u">Istituto di Fisica Cosmica ed Applicazioni dell'Informatica del CNR, Palermo, Italia</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">Il Nuovo Cimento C</subfield>
   <subfield code="d">Kluwer Academic Publishers</subfield>
   <subfield code="g">15/5(1992-09-01), 743-749</subfield>
   <subfield code="x">0390-5551</subfield>
   <subfield code="q">15:5&lt;743</subfield>
   <subfield code="1">1992</subfield>
   <subfield code="2">15</subfield>
   <subfield code="o">11543</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>
