J. K. Lee

TL;DR: In this paper, the first flight of the balloon-borne cosmic-ray experiment Cosmic-Ray Energetics and Mass (CREAM) was reported to provide the first high accuracy measurements of the relative abundances of elements from boron to oxygen up to energies around 1.

TL;DR: In this article, the authors evaluate the exposure during nadir observations with JEM-EUSO, the Extreme Universe Space Observatory, on-board the Japanese Experiment Module of the International Space Station.

TL;DR: The Cosmic Ray Energetics And Mass (CREAM) experiment is designed to investigate high-energy (10 12 ∼10 15 ǫ) cosmic rays over the elemental range from hydrogen to iron (1⩽ Z ⩽26), through a series of long balloon flights as mentioned in this paper.

TL;DR: In this article, the relative abundances of cosmic-ray nuclei in the energy range of 500-3980 GeV/nucleon from the second flight of the Cosmic Ray Energetics And Mass balloon-borne experiment were determined using a sampling tungsten/scintillating-fiber calorimeter, while particle charge was identified precisely with a dual-layer silicon charge detector installed for this flight.

TL;DR: TUS (Tracking Ultraviolet Set-up) as discussed by the authors, the first orbital EECR detector, was launched into orbit on April 28, 2016, as a part of the Lomonosov satellite scientific payload.