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Please use this identifier to cite or link to this item: https://dspace.ctu.edu.vn/jspui/handle/123456789/4186
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dc.contributor.authorNelles, A.-
dc.contributor.authorBuitink, S.-
dc.contributor.authorCorstanje, A.-
dc.contributor.authorEnriquez, J. E.-
dc.contributor.authorFalcke, H.-
dc.contributor.authorHörandel, J. R.-
dc.contributor.authorRachen, J. P.-
dc.contributor.authorRossetto, L.-
dc.contributor.authorSchellart, P.-
dc.contributor.authorScholten, O.-
dc.contributor.authorVeen, S. ter-
dc.contributor.authorThoudam, S.-
dc.contributor.authorTrịnh, Thị Ngọc Gia-
dc.date.accessioned2018-09-14T07:17:39Z-
dc.date.available2018-09-14T07:17:39Z-
dc.date.issued2015-
dc.identifier.urihttp://dspace.ctu.edu.vn/jspui/handle/123456789/4186-
dc.description.abstractThe pattern of the radio emission of air showers is finely sampled with the Low-Frequency ARray (LOFAR). A set of 382 measured air showers is used to test a fast, analytic parameterization of the distribution of pulse powers. Using this parameterization we are able to reconstruct the shower axis and give estimators for the energy of the air shower as well as the distance to the shower maximum.vi_VN
dc.language.isoenvi_VN
dc.relation.ispartofseriesJournal of Cosmology and Astroparticle Physics;2015-
dc.subjectCosmic ray experimentsvi_VN
dc.titleThe radio emission pattern of air showers as measured with LOFAR—a tool for the reconstruction of the energy and the shower maximumvi_VN
dc.typeArticlevi_VN
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