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   <subfield code="a">10.1007/BF02507849</subfield>
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   <subfield code="a">Rule-guided identification of cosmic-ray patterns in PLASTEX</subfield>
   <subfield code="h">[Elektronische Daten]</subfield>
   <subfield code="c">[O. Catalano, B. Lenzitti, J. Linsley, A. Machì, L. Scarsi]</subfield>
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   <subfield code="a">Summary: Some techniques devised in the computer science fields of pattern recognition and expert systems are being applied to the interpretation of EAS responses in the PLASTEX experiment. An attempt is made to codity in a set of rules the expertise of trained researchers who are able to recognize and classify different hit patterns even in the presence of noisy background, and in spite of imperfections in the detector response. The patterns expected to be useful include, but are not limited to, track patterns. The software described here, as a progress report, automatically finds patterns corresponding to isolated tracks, and patterns composed of tracks that connect with each other in a layer of dense material. Tracks are reconstructed iteratively, using both geometrical and internal consistency arguments. Multihits, geometrical inefficiency, mechanical imperfection and track bending are taken into account. Data preprocessing is applied to multihits according to a theoretical model of the particle-detector interaction, and the presence of tracks in dead detector areas is inferred by probabilistic arguments. Finally, particle scattering is allowed for using a variable-size tolerance cone during the track reconstruction procedure. Examples are given of application of the method to recognition of nearly straight tracks, such as those expected to be made by high-energy muons, and of more complicated patterns made of connected straight tracks.</subfield>
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   <subfield code="a">Società Italiana di Fisica, 1992</subfield>
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   <subfield code="a">Cosmic-rays</subfield>
   <subfield code="2">nationallicence</subfield>
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  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">PACS 94.40.My</subfield>
   <subfield code="2">nationallicence</subfield>
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  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">Extensive air showers</subfield>
   <subfield code="2">nationallicence</subfield>
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  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">Computation techniques</subfield>
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   <subfield code="a">Catalano</subfield>
   <subfield code="D">O.</subfield>
   <subfield code="u">Instituto di Fisica Cosmica ed Applicazioni dell'Informatica del CNR, Palermo, Italia</subfield>
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   <subfield code="a">Lenzitti</subfield>
   <subfield code="D">B.</subfield>
   <subfield code="u">Instituto di Fisica Cosmica ed Applicazioni dell'Informatica del CNR, Palermo, Italia</subfield>
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   <subfield code="u">Instituto di Fisica Cosmica ed Applicazioni dell'Informatica del CNR, Palermo, Italia</subfield>
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   <subfield code="a">Machì</subfield>
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   <subfield code="u">Instituto di Fisica Cosmica ed Applicazioni dell'Informatica del CNR, Palermo, Italia</subfield>
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   <subfield code="a">Scarsi</subfield>
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   <subfield code="u">Instituto di Fisica Cosmica ed Applicazioni dell'Informatica del CNR, Palermo, Italia</subfield>
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   <subfield code="t">Il Nuovo Cimento C</subfield>
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   <subfield code="g">15/5(1992-09-01), 763-769</subfield>
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