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

The HiSCORE experiment is an array of wide-angle, non-imaging detectors of atmospheric Cherenkov component of EAS operating in the ultra high energy range. Whereas arrays of particle detectors use shower front of secondary particles that reach the observation level, HiSCORE deals with the shower light front, i.e. temporal and spatial distributions of Cherenkov photons generated in EAS. The temporal difference between light fronts of gamma and proton induced EAS is analyzed using Monte Carlo simulations. A gamma-hadron separation possibility based on this difference is studied taking into account realistic detector resolutions of event reconstruction.

A study of the EAS Cherenkov light time profile with the HiSCORE experiment