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 high school project on astrophysics research with cosmics (HiSPARC)employs a large number of small detection stations that sample the footprint ofextensive cosmic ray air showers. The majority of these stations has two 0.5\si{\meter\squared} scintillation detectors. A new method is presented whichenables probing the cosmic ray flux with a single two-scintillator station infive energy decades at $10^{12}$, $10^{13}$, $10^{14}$, $10^{15}$ and $10^{16}$eV. The method is based on the energy dependence of the distribution of thenumber of particles passing through a single detector. A relatively short datataking period of approximately one month is sufficient to probe this energyrange. The flux values agree well with measurements by other experiments. Forthe first time, the cosmic ray flux at $10^{12}$ and $10^{13}$ eV is derived atsea level.

Probing the cosmic ray energy spectrum at $10^{12}$--$10^{16}$ eV with two HiSPARC scintillators