We present a computationally simple, theoretically based parameterization for the
broadband albedo of snow and ice that can accurately reproduce the theoretical broadband …

The interactions of electromagnetic radiation with ice, and with ice-containing media such as
snow and clouds, are determined by the refractive index and absorption coefficient (the …

The detection of high-energy cosmic neutrinos as cosmic messengers has been an
important goal of astroparticle physics. Being stable, electrically neutral particles, high …

A compilation of the spectral absorption coefficient of ice Ih is presented for temperatures
near the melting point, superseding the compilation of Warren (1984). Significant changes …

The IceCube neutrino observatory [1, 2] is a cubic kilometer photomultiplier (PMT) array
embedded in glacial ice at the geographic South Pole. The complete array is made of 5160 …

We have performed a search for muon neutrinos from dark matter annihilation in the center
of the Sun with the 79-string configuration of the IceCube neutrino telescope. For the first …

A measurement of the diffuse astrophysical neutrino spectrum is presented using IceCube
data collected from 2011–2022 (10.3 years). We developed novel detection techniques to …

The IceCube neutrino observatory in operation at the South Pole, Antarctica, comprises
three distinct components: a large buried array for ultrahigh energy neutrino detection, a …

The IceCube Neutrino Observatory, approximately 1km3 in size, is now complete with 86
strings deployed in the Antarctic ice. IceCube detects the Cherenkov radiation emitted by …

IceCube is a km-scale neutrino observatory under construction at the South Pole with
sensors both in the deep ice (InIce) and on the surface (IceTop). The sensors, called Digital …