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  <titleInfo>
    <title>2D image processing for DSO astrophotography</title>
  </titleInfo>
  <name type="personal">
    <namePart>SUSZYŃSKI, Robert.</namePart>
    <namePart type="termsOfAddress">Politechnika Koszalińska - Wydział Elektroniki i Informatyki, Katedra Systemów Cyfrowego Przetwarzania Sygnałów</namePart>
    <namePart type="date">1996 -</namePart>
    <role>
      <roleTerm authority="marcrelator" type="text">creator</roleTerm>
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  <name type="personal">
    <namePart>WAWRYN, Krzysztof.</namePart>
    <namePart type="termsOfAddress">Politechnika Koszalińska - Wydział Elektroniki i Informatyki, Katedra Systemów Cyfrowego Przetwarzania Sygnałów</namePart>
    <namePart type="date">1996 -</namePart>
  </name>
  <name type="personal">
    <namePart>WIRSKI, Robert.</namePart>
    <namePart type="termsOfAddress">Politechnika Koszalińska - Wydział Elektroniki i Informatyki, Katedra Systemów Cyfrowego Przetwarzania Sygnałów</namePart>
    <namePart type="date">1996 -</namePart>
  </name>
  <name type="conference">
    <namePart>World Academy of Science, Engineering and Technology (2010 ; Tokio, Japan).</namePart>
  </name>
  <typeOfResource>text</typeOfResource>
  <genre authority="marc">conference publication</genre>
  <originInfo>
    <place>
      <placeTerm type="code" authority="marccountry">jp</placeTerm>
    </place>
    <dateIssued encoding="marc">2010</dateIssued>
    <issuance>continuing</issuance>
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    <languageTerm authority="iso639-2b" type="code">eng</languageTerm>
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  <abstract>The new concept of two–dimensional (2D) image processing implementation for auto-guiding system is shown in this paper. It is dedicated to astrophotography and operates with astronomy CCD guide cameras or with self-guided dual-detector CCD cameras and ST4 compatible equatorial mounts. This idea was verified by MATLAB model, which was used to test all procedures and data conversions. Next the circuit prototype was implemented at Altera MAX II CPLD device and tested for real astronomical object images. The digital processing speed of CPLD prototype board was sufficient for correct equatorial mount guiding in real-time system.</abstract>
  <note type="statement of responsibility">Robert Suszyński, Krzysztof Wawryn, Robert Wirski.</note>
  <subject>
    <topic>DSO astrophotography|en</topic>
  </subject>
  <subject>
    <topic>image processing|en</topic>
  </subject>
  <subject>
    <topic>twodimensional convolution method|en</topic>
  </subject>
  <subject>
    <topic>two-dimensional filtering|en</topic>
  </subject>
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    <titleInfo>
      <title>International Journal of Environmental, Earth Science and Engineering. -</title>
    </titleInfo>
    <identifier type="issn">1307-6892</identifier>
    <part>
      <text>2010, nr 4(5), s. 633-637</text>
    </part>
  </relatedItem>
  <identifier type="uri">http://scholar.waset.org/1999.0/2656</identifier>
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    <url>http://scholar.waset.org/1999.0/2656</url>
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