5th Congress of Balkan Geophysical Society 2009
DOI: 10.3997/2214-4609-pdb.126.6551
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Influence of Grid Density Gravity Surveys on Results in Hydrocarbon Exploration

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“…Instead of searching for such a localized excess, the neutrino arrival direction can be correlated with the arrival directions of UHECRs, as described in [15]. By obtaining the probability density function of the number of neutrino events within a specific angular distance from observed UHECRs, the number of neutrino events in the vicinity of observed UHECRs, necessary to claim a discovery with a chosen significance, can be calculated.…”
Section: Auger and Ultra-high-energy Cosmic Raysmentioning
confidence: 99%
“…Instead of searching for such a localized excess, the neutrino arrival direction can be correlated with the arrival directions of UHECRs, as described in [15]. By obtaining the probability density function of the number of neutrino events within a specific angular distance from observed UHECRs, the number of neutrino events in the vicinity of observed UHECRs, necessary to claim a discovery with a chosen significance, can be calculated.…”
Section: Auger and Ultra-high-energy Cosmic Raysmentioning
confidence: 99%