Radio Detection of Cosmic Rays with Lopes

dc.contributor.authorHorneffer, A.
dc.contributor.authorApel, W. D.
dc.contributor.authorBadea, F.
dc.contributor.authorBahren, L.
dc.contributor.authorBekk, K.
dc.contributor.authorBercuci, A.
dc.contributor.authorBertaina, M.
dc.contributor.authorBiermann, P. L.
dc.contributor.authorBlumer, J.
dc.contributor.authorBozdog, H.
dc.contributor.authorButcher, Harvey
dc.date.accessioned2015-12-10T22:17:05Z
dc.date.issued2006
dc.date.updated2015-12-09T08:29:40Z
dc.description.abstractMeasuring radio pulses from cosmic ray air showers offers various new opportunities. New digital radio receivers allow measurements of these radio pulses even in environments that have lots of radio interference. With high bandwidth ADCs and fast data processing it is possible to store the whole waveform information in digital form and analyse transient events like air showers even after they have been recorded. Digital filtering and beam forming can be used to suppress the radio interference so that it is possible to measure the radio pulses even in radio loud environments. LOPES is a prototype station for the new digital radio interferometer LOFAR and is tailored to measure air showers. For this it is located at the site of the KASCADE-Grande air shower experiment. Already with the first phase of LOPES we have been able to measure radio pulses from air showers and show correlations between the radio pulse height and air shower parameters. The first part gives an introduction and presents the science results of LOPES, while the second part presents the hard- and software that enables LOPES to detect air short pulses.
dc.identifier.issn0217-751X
dc.identifier.urihttp://hdl.handle.net/1885/51246
dc.publisherWorld Scientific Publishing Company
dc.sourceInternational Journal of Modern Physics A (IJMPA)
dc.titleRadio Detection of Cosmic Rays with Lopes
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage181
local.bibliographicCitation.startpage168
local.contributor.affiliationHORNEFFER, A., Radboud University Nijmegen
local.contributor.affiliationApel, W D, Institut fur Kernphysik
local.contributor.affiliationBadea, F, Institut fur Kernphysik
local.contributor.affiliationBahren, L, ASTRON Dwingeloo
local.contributor.affiliationBekk, K, Institut fur Kernphysik
local.contributor.affiliationBercuci, A, NIPNE Bucharest
local.contributor.affiliationBertaina, M, University di Torino
local.contributor.affiliationBiermann, P L, Max Planck Institute for Radio Astronomy
local.contributor.affiliationBlumer, J, Institut fur Kernphysik
local.contributor.affiliationBozdog, H, Institut fur Kernphysik
local.contributor.affiliationButcher, Harvey, College of Physical and Mathematical Sciences, ANU
local.contributor.authoremailu4478121@anu.edu.au
local.contributor.authoruidButcher, Harvey, u4478121
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020106 - High Energy Astrophysics; Cosmic Rays
local.identifier.ariespublicationu3379551xPUB220
local.identifier.citationvolume21
local.identifier.doi10.1142/S0217751X0603357X
local.identifier.scopusID2-s2.0-33747655085
local.identifier.uidSubmittedByu3379551
local.type.statusPublished Version

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