Large-scale distribution of arrival directions of cosmic rays detected at the Pierre Auger Observatory and the Telescope Array above 1019 eV

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F16%3A00551702" target="_blank" >RIV/68378271:_____/16:00551702 - isvavai.cz</a>
Result on the web
<a href="https://pos.sissa.it/236/395/pdf" target="_blank" >https://pos.sissa.it/236/395/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.236.0395" target="_blank" >10.22323/1.236.0395</a>

Result language
angličtina
Original language name
Large-scale distribution of arrival directions of cosmic rays detected at the Pierre Auger Observatory and the Telescope Array above 1019 eV
Original language description
The large-scale distribution of arrival directions of high-energy cosmic rays is a key observable in attempts to understanding their origin. The dipole and quadrupole moments are of special interest in revealing potential anisotropies. An unambiguous measurement of these moments as well as 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 Pierre Auger Observatory and the Telescope Array above 1019 eV has been performed.
Czech name
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Czech description
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Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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