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<bibitem type="C">   <ARLID>0453742</ARLID> <utime>20240103211557.4</utime><mtime>20160112235959.9</mtime>   <SCOPUS>84984581019</SCOPUS> <WOS>000371804300197</WOS>  <DOI>10.1063/1.4938976</DOI>           <title language="eng" primary="1">Automated detection of meteors in observed image sequence</title>  <specification> <page_count>4 s.</page_count> <media_type>P</media_type> </specification>    <serial><ARLID>cav_un_epca*0453741</ARLID><ISBN>978-0-7354-1349-8</ISBN><ISSN>0094-243X</ISSN><title>International conference of computational methods in sciences and engineering 2015</title><part_num/><part_title/><publisher><place>Melville</place><name>American Institute of Physics</name><year>2015</year></publisher><editor><name1>Simos</name1><name2>T.E.</name2></editor></serial>    <keyword>meteor detection</keyword>   <keyword>statistical moments</keyword>   <keyword>Hough transformation</keyword>    <author primary="1"> <ARLID>cav_un_auth*0100099</ARLID> <full_dept language="cz">Sluneční oddělení</full_dept> <full_dept language="eng">Department of Solar Physics</full_dept> <full_dept>Department of Solar Physics - Team 1</full_dept>  <name1>Šimberová</name1> <name2>Stanislava</name2> <institution>ASU-R</institution> <fullinstit>Astronomický ústav AV ČR, v. v. i.</fullinstit> </author> <author primary="0"> <ARLID>cav_un_auth*0101203</ARLID> <full_dept language="cz">Zpracování obrazové informace</full_dept> <full_dept>Department of Image Processing</full_dept> <department language="cz">ZOI</department> <department>ZOI</department> <full_dept>Department of Image Processing</full_dept>  <name1>Suk</name1> <name2>Tomáš</name2> <institution>UTIA-B</institution> <fullinstit>Ústav teorie informace a automatizace AV ČR, v. v. i.</fullinstit> </author>        <cas_special> <project> <ARLID>cav_un_auth*0314467</ARLID> <project_id>GA15-16928S</project_id> <agency>GA ČR</agency> </project>  <abstract language="eng" primary="1">We propose a new detection technique based on statistical characteristics of images in the video sequence. These  characteristics displayed in time enable to catch any bright track during the whole sequence. We applied our method to the  image datacubes that are created from camera pictures of the night sky. Meteor flying through the Earth’s atmosphere leaves a  light trail lasting a few seconds on the sky background. We developed a special technique to recognize this event automatically  in the complete observed video sequence. For further analysis leading to the precise recognition of object we suggest to apply  Fourier and Hough transformations.</abstract>    <action target="WRD"> <ARLID>cav_un_auth*0325124</ARLID> <name>International conference of computational methods in sciences and engineering 2015</name> <dates>20150320</dates> <place>Athens</place> <country>GR</country>  <unknown tag="mrcbC20-s">20150323</unknown> </action>  <RIV>IN</RIV>    <reportyear>2016</reportyear>     <unknown tag="mrcbC55"> UTIA-B IN </unknown> <inst_support> RVO:67985815 </inst_support> <inst_support> RVO:67985556 </inst_support>  <permalink>http://hdl.handle.net/11104/0254470</permalink>   <confidential>S</confidential>  <unknown tag="mrcbC83"> RIV/67985815:_____/15:00453742!RIV16-AV0-67985815 191659448 oprava kódu vědeckého oboru RIV ASU-R </unknown>       <unknown tag="mrcbT16-s">0.160</unknown> <unknown tag="mrcbT16-E">Q4</unknown> <arlyear>2015</arlyear>       <unknown tag="mrcbU14"> 84984581019 SCOPUS </unknown> <unknown tag="mrcbU34"> 000371804300197 WOS </unknown> <unknown tag="mrcbU63"> cav_un_epca*0453741 International conference of computational methods in sciences and engineering 2015 American Institute of Physics 2015 Melville 978-0-7354-1349-8 AIP Conference proceedings 1702 0094-243X 190009/1-190009/4 </unknown> <unknown tag="mrcbU67"> 340 Simos T.E. </unknown> </cas_special> </bibitem>