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 Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Cosmic ray (CR) nuclei are accelerated particles which move randomly through the interstellar medium (ISM), where they suffer scattering, reacceleration and energy loss processes before reaching Earth. Spallation processes also take place forming secondary nuclei by fragmentation of heavier ones. Due to the impossibility of observing directly their original direction, the determination of possible sources where these particles originated requires the use of codes to simulate the propagation of CR within the Galaxy. This consists of a spiral disk with a thickness of 2h ~ 200 pc, where CR are created, and a halo with a height H, where they diffuse.

The Effect of the Galactic Gas Distribution on the Expected Cosmic Rays Spectrum