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Please use this identifier to cite or link to this item: http://cmuir.cmu.ac.th/jspui/handle/6653943832/57895
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dc.contributor.authorK. Kasonsuwanen_US
dc.contributor.authorS. Wannawichianen_US
dc.contributor.authorT. Kirdkaoen_US
dc.date.accessioned2018-09-05T03:52:42Z-
dc.date.available2018-09-05T03:52:42Z-
dc.date.issued2017-10-20en_US
dc.identifier.issn17426596en_US
dc.identifier.issn17426588en_US
dc.identifier.other2-s2.0-85034107120en_US
dc.identifier.other10.1088/1742-6596/901/1/012009en_US
dc.identifier.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85034107120&origin=inwarden_US
dc.identifier.urihttp://cmuir.cmu.ac.th/jspui/handle/6653943832/57895-
dc.description.abstract© Published under licence by IOP Publishing Ltd. The direct observations of Geostationary Orbit (GEO) satellites above Thailand's sky by 0.7-meters telescope were proceeded at Inthanon Mt., Chiang Mai, Thailand. The observation took place at night with Sidereal Stare Mode (SSM). With this observing mode, the moving object will appear as a streak. The star identification for image calibration is based on (1) a star catalogue, (2) the streak detection of the satellite using the software and (3) the extraction of the celestial coordinate of the satellite as a predicted position. Finally, the orbital elements for GEO satellites were calculated.en_US
dc.subjectPhysics and Astronomyen_US
dc.titleObservation of GEO Satellite above Thailand's Skyen_US
dc.typeConference Proceedingen_US
article.title.sourcetitleJournal of Physics: Conference Seriesen_US
article.volume901en_US
article.stream.affiliationsChiang Mai Universityen_US
article.stream.affiliationsNational Astronomical Research Institute of Thailanden_US
article.stream.affiliationsLearning Center for Earth Science and Astronomy (LESA)en_US
article.stream.affiliationsRoyal Thai Air Forceen_US
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