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Statements

Subject Item
n2:RIV%2F00216208%3A11320%2F14%3A10283734%21RIV15-MSM-11320___
rdf:type
skos:Concept n18:Vysledek
rdfs:seeAlso
http://dx.doi.org/10.1088/0004-637X/794/2/172
dcterms:description
Spherical harmonic moments are well-suited for capturing anisotropy at any scale in the flux of cosmic rays. An unambiguous measurement of the full set of spherical harmonic coefficients requires full-sky coverage. This can be achieved by combining data from observatories located in both the northern and southern hemispheres. To this end, a joint analysis using data recorded at the Telescope Array and the Pierre Auger Observatory above 10(19) eV is presented in this work. The resulting multipolar expansion of the flux of cosmic rays allows us to perform a series of anisotropy searches, and in particular to report on the angular power spectrum of cosmic rays above 10(19) eV. No significant deviation from isotropic expectations is found throughout the analyses performed. Upper limits on the amplitudes of the dipole and quadrupole moments are derived as a function of the direction in the sky, varying between 7% and 13% for the dipole and between 7% and 10% for a symmetric quadrupole. Spherical harmonic moments are well-suited for capturing anisotropy at any scale in the flux of cosmic rays. An unambiguous measurement of the full set of spherical harmonic coefficients requires full-sky coverage. This can be achieved by combining data from observatories located in both the northern and southern hemispheres. To this end, a joint analysis using data recorded at the Telescope Array and the Pierre Auger Observatory above 10(19) eV is presented in this work. The resulting multipolar expansion of the flux of cosmic rays allows us to perform a series of anisotropy searches, and in particular to report on the angular power spectrum of cosmic rays above 10(19) eV. No significant deviation from isotropic expectations is found throughout the analyses performed. Upper limits on the amplitudes of the dipole and quadrupole moments are derived as a function of the direction in the sky, varying between 7% and 13% for the dipole and between 7% and 10% for a symmetric quadrupole.
dcterms:title
SEARCHES FOR LARGE-SCALE ANISOTROPY IN THE ARRIVAL DIRECTIONS OF COSMIC RAYS DETECTED ABOVE ENERGY OF 10(19) eV AT THE PIERRE AUGER OBSERVATORY AND THE TELESCOPE ARRAY SEARCHES FOR LARGE-SCALE ANISOTROPY IN THE ARRIVAL DIRECTIONS OF COSMIC RAYS DETECTED ABOVE ENERGY OF 10(19) eV AT THE PIERRE AUGER OBSERVATORY AND THE TELESCOPE ARRAY
skos:prefLabel
SEARCHES FOR LARGE-SCALE ANISOTROPY IN THE ARRIVAL DIRECTIONS OF COSMIC RAYS DETECTED ABOVE ENERGY OF 10(19) eV AT THE PIERRE AUGER OBSERVATORY AND THE TELESCOPE ARRAY SEARCHES FOR LARGE-SCALE ANISOTROPY IN THE ARRIVAL DIRECTIONS OF COSMIC RAYS DETECTED ABOVE ENERGY OF 10(19) eV AT THE PIERRE AUGER OBSERVATORY AND THE TELESCOPE ARRAY
skos:notation
RIV/00216208:11320/14:10283734!RIV15-MSM-11320___
n5:aktivita
n17:P n17:I
n5:aktivity
I, P(7AMB14AR005), P(GA14-17501S), P(LG13007)
n5:cisloPeriodika
2
n5:dodaniDat
n7:2015
n5:domaciTvurceVysledku
n10:9906681 n10:7650736
n5:druhVysledku
n16:J
n5:duvernostUdaju
n20:S
n5:entitaPredkladatele
n13:predkladatel
n5:idSjednocenehoVysledku
44090
n5:idVysledku
RIV/00216208:11320/14:10283734
n5:jazykVysledku
n14:eng
n5:klicovaSlova
cosmic rays; astroparticle physics
n5:klicoveSlovo
n12:astroparticle%20physics n12:cosmic%20rays
n5:kodStatuVydavatele
US - Spojené státy americké
n5:kontrolniKodProRIV
[1E9776291376]
n5:nazevZdroje
Astrophysical Journal
n5:obor
n8:BF
n5:pocetDomacichTvurcuVysledku
2
n5:pocetTvurcuVysledku
607
n5:projekt
n11:LG13007 n11:GA14-17501S n11:7AMB14AR005
n5:rokUplatneniVysledku
n7:2014
n5:svazekPeriodika
794
n5:tvurceVysledku
Albuquerque, I. F. M. Alvarez-Muniz, J. Aublin, J. Aramo, C. Assis, P. Almela, A. Alvarez Castillo, J. Asorey, H. Allison, P. Badescu, A. M. Aab, A. Beatty, J. J. Allen, J. Al Samarai, I. Allekotte, I. Ave, M. Baus, C. Abreu, P. Andringa, S. Aminaei, A. Arqueros, F. Barber, K. B. Avila, G. Nosek, Dalibor Anchordoqui, L. Avenier, M. Novotný, Vladimír Ahn, E. J. Batista, R. Alves Baeuml, J. Ambrosio, M. Aglietta, M.
n5:wos
000343085800076
s:issn
0004-637X
s:numberOfPages
15
n19:doi
10.1088/0004-637X/794/2/172
n3:organizacniJednotka
11320