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dc.contributor.advisor김항배-
dc.contributor.author박경윤-
dc.date.accessioned2020-03-18T17:00:35Z-
dc.date.available2020-03-18T17:00:35Z-
dc.date.issued2011-08-
dc.identifier.urihttps://repository.hanyang.ac.kr/handle/20.500.11754/138845-
dc.identifier.urihttp://hanyang.dcollection.net/common/orgView/200000417851en_US
dc.description.abstractWe studied about cosmic-ray how to propagate in the galaxy and what is the source of it. In addition, we briefly discussed some results from two cosmic-ray xperiments, which are PAMELA and FERMI. Explaining for these results, we consider the two pulsar, the Geminga and B0656+14, and these pulsars generate electrons and positron. Hence, these electrons and positrons can explain the strange phenomenon.-
dc.publisher한양대학교-
dc.title은하내에서 우주선의 전파과정-
dc.title.alternativePropagation of cosmic-ray in the galaxy-
dc.typeTheses-
dc.contributor.googleauthor박경윤-
dc.contributor.alternativeauthorPark, Kyeongyun-
dc.sector.campusS-
dc.sector.daehak대학원-
dc.sector.department물리학과-
dc.description.degreeMaster-
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GRADUATE SCHOOL[S](대학원) > PHYSICS(물리학과) > Theses (Master)
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