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

AMS-02 is a wide acceptance high-energy physics experiment installed on theInternational Space Station in May 2011 and it has been operating continuouslysince then. AMS-02 is able to separate cosmic rays light nuclei ($1\leq Z \leq8$) with contaminations less than $10^{-3}$. The ratio between the cosmic raysBoron and Carbon fluxes is known to be very sensitive to the properties of thepropagation of cosmic rays in the Galaxy, being Boron a secondary product ofspallation on the interstellar medium of heavier primary elements such asCarbon and Oxygen. A precise measurement reaching the TeV region cansignificantly help understanding cosmic rays propagation in the Galaxy and theamount of matter traversed before reaching Earth. The status of the measurementof the boron-to-carbon ratio based on 10 millions Boron and Carbon events ispresented.

Precision Measurement of Boron-to-Carbon ratio in Cosmic Rays from 2 GV  to 2 TV with the Alpha Magnetic Spectrometer on the International Space  Station