On the 15th of June 2006, the PAMELA (Payload for Antimatter Matter Exploration and Light-
nuclei Astrophysics) satellite-borne experiment was launched onboard the Russian Resurs …

This review paper commemorates a century of cosmic ray research, with emphasis on the
plasma physics aspects. Cosmic rays comprise only∼ 10− 9 of interstellar particles by …

We present a measurement of the atmospheric neutrino oscillation parameters using three
years of data from the IceCube Neutrino Observatory. The DeepCore infill array in the center …

IceTop, the surface component of the IceCube Neutrino Observatory at the South Pole, is an
air shower array with an area of 1km2. The detector allows a detailed exploration of the …

Weakly interacting massive particles (WIMPs) are a theoretical class of particles that are
excellent dark matter candidates. WIMP annihilation or decay may produce essentially …

A measurement of the atmospheric muon neutrino energy spectrum from 100 GeV to 400
TeV was performed using a data sample of about 18 000 up-going atmospheric muon …

Recent observations by PAMELA, Fermi-LAT, and AMS-02 have conclusively indicated a
rise in the cosmic-ray positron fraction above 10 GeV, a feature which is impossible to mimic …

Self-annihilating or decaying dark matter in the Galactic halo might produce high energy
neutrinos detectable with neutrino telescopes. We have conducted a search for such a …

In the last few decades, a number of experiments have provided long-term, statistically
significant evidence of a faint sidereal anisotropy in the cosmic-ray arrival direction …

Over the last three years, several satellite and balloon observatories have suggested
intriguing features in the cosmic ray lepton spectra. Most notably, the PAMELA satellite has …