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Shigeru Yoshida (Chiba University)16/09/2025, 13:40
The Amundsen-Scott South Pole Station is an ideal location for studying the universe of high-energy particles by detecting neutrinos. The IceCube Neutrino Observatory measures neutrinos emitted from sources of cosmic rays, which are the most energetic background radiation in the universe. In this talk, we present our latest findings on the neutrino sky, covering a broad range of energies from...
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Aya Ishihara (Chiba University)16/09/2025, 14:00
The IceCube Neutrino Observatory at the geographic South Pole has achieved major milestones in neutrino astrophysics, including the discovery of a high-energy astrophysical neutrino flux and correlations with flaring blazars and Seyfert galaxies. Building on this success, the IceCube Upgrade is scheduled for completion during the 2025/26 Antarctic summer season. This upgrade will deploy seven...
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Vivian O'Dell (University of Wisconsin–Madison)16/09/2025, 14:20
Building on the success of IceCube, and the upcoming deployment of the IceCube Upgrade, the IceCube collaboration is planning for a next phase of upgrade of the detector, IceCube-Gen2. Over the past decade, the IceCube-Gen2 Collaboration has been designing a detector that would provide an order of magnitude greater sensitivity to high- and ultra-high-energy neutrinos, increasing the volume of...
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Achara Seripienlert17/09/2025, 09:00
Ground-based cosmic ray observations from polar regions are key to understanding the modulation of galactic cosmic rays and their interactions with Earth’s magnetic environment. In this study, we present results from a latitude survey using the Changvan neutron monitor aboard the South Korean icebreaker Araon, which traversed from Antarctic to Arctic latitudes during its 2023–24 voyages. The...
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