activity
20242026
collaborators

5 papers

astro-ph.HE2026

Observation of the Forbush decrease on 2024 May 10, using the ALPAQUITA air-shower array at the 70-1000 GV rigidity range

M. Anzorena, E. de la Fuente, K. Fujita +49

The Andes Large area PArticle detector for Cosmic ray and Astronomy (ALPACA) is a new air-shower array experiment under construction in the Bolivian Andes, and its prototype ALPAQU…

astro-ph.HE2025

A new air shower array in the Southern Hemisphere looking for the origins of Cosmic rays: the ALPACA experiment

M. Anzorena, E. de la Fuente, K. Fujita +53

The Tibet AS experiment successfully detected sub-PeV -rays from the Crab nebula using a Surface Array and underground muon detector. Considering this, we are building in B…

astro-ph.HE2025

Precision spectral measurements of Chromium and Titanium from 10 to 250 GeV and sub-Iron to Iron ratio with the Calorimetric Electron Telescope on the ISS

O. Adriani, Y. Akaike, K. Asano +77

The Calorimetric Electron Telescope (CALET), in operation on the International Space Station since 2015, collected a large sample of cosmic-ray (CR) iron and sub-iron events over a…

astro-ph.HE2025

Ground-based Observations of Temporal Variation of Cosmic Ray Spectrum during Forbush Decreases

W. Mitthumsiri, D. Ruffolo, K. Munakata +29

Observations of temporary Forbush decreases (FDs) in the Galactic cosmic ray (GCR) flux due to passage of solar storms are useful for space weather studies and alerts. Here we intr…

astro-ph.SR2024

Cosmic ray north-south anisotropy: rigidity spectrum and solar cycle variations observed by ground-based muon detectors

M. Kozai, Y. Hayashi, K. Fujii +9

The north-south (NS) anisotropy of galactic cosmic rays (GCRs) is dominated by a diamagnetic drift flow of GCRs in the interplanetary magnetic field (IMF), allowing us to derive ke…