3-7 noviembre 2025
Europe/Madrid timezone

Energy-dependent Orbital Compton-Getting Dipole with IceCube Cosmic-Ray Muons

5 nov. 2025 17:30
15m
Room 2.1+2.2 (ADEIT)

Room 2.1+2.2

ADEIT

Talk Cosmic Rays Cosmic Rays

Ponente

Juan Carlos Díaz Vélez (University of Wisconsin-Madison)

Descripción

The Compton-Getting effect — an apparent dipolar anisotropy of cosmic rays generated by Earth's orbital motion around the Sun — serves as a known calibration source for cosmic-ray anisotropy studies. The amplitude of the Compton-Getting dipole depends on both the orbital speed and the mean spectral index of the cosmic-ray flux. It therefore provides an indirect method for studying the energy spectrum of cosmic rays. This work will report on a study of the spectral index of cosmic-ray induced muons as a function of energy using data collected over 12 years by IceCube in the 10 TeV to 100 TeV range.

Autores primarios

Juan Carlos Díaz Vélez (University of Wisconsin-Madison) Paolo Desiati (University of Wisconsin-Madison) Thyra Eysselink (New Patlz State University of New York) Aylar Gayypova (Mercer University)

Materiales de la presentación

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