English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

Calculations are presented to demonstrate the feasibility of Moon shadowobservations for mean primary energies in the region 0.5-1.5 TeV using a muondetector operating under the Pyramid of the Sun at Teotihuacan, Mexico. Due tothe small height of that monument (65 m), the experiment is capable ofproviding considerably high statistics, although with reduced angular accuracyfor primary particle direction reconstruction. Our estimates are based onsimulations of muon production and transport in the atmosphere by CORSIKA andalong the body of the pyramid by GEANT4. The deflection of primaries in theearth magnetic field is calculated using the IGRF model. The statistics for theMoon shadow observations, which depends on different factors affecting theaccuracy of the primary particle direction reconstruction, are analyzed indetail.

Feasibility for p+/p- flow-ratio evaluation in the 0.5 - 1.5 TeV primary  energy range, based on Moon-shadow muon measurements, to be carried out in  the Pyramid of the Sun, Teotihuacan, Experiment