19–21 Mar 2025
Physics Department
Europe/Athens timezone

High latitude muon and neutron observation of the Forbush decrease during the May 2024 solar storms

20 Mar 2025, 11:10
20m
Seminar Room (Physics Department )

Seminar Room

Physics Department

National and Kapodistrian University of Athens University Campus, Panepistimioupolis Zografos, 15784 Athens, GREECE

Speaker

Martin Schrön (Helmholtz Centre for Environmental Research GmbH - UFZ, Leipzig, Germany)

Description

A series of intense solar flares occurred in May 2024. Among other effects, a remarkable Forbush decrease in the cosmic ray flux was observed on the Earth. This event was observed by neutron and muon detectors installed at the Svalbard, in a high latitude site, characterized by a weak geomagnetic shielding. For this analysis we employed at Ny-Alesund three scintillator-based muon telescopes of the Extreme Energy Events (EEE) project, 14 channels of a Bonner Sphere neutron Spectrometer (BSS), thermal and epithermal neutron sensors used for hydrological monitoring, and data from NM Barentsburg.

Most sensors showed significant responses and correlation during the event. The observed relative magnitude of the Forbush decrease was estimated to be ≈ 9% for thermal neutrons, ≈ 8% for high-energy neutrons, and ≈ 3% for muons. A correlation analysis of the time series provided by all these detectors will be discussed in this contribution.

Session 2 - Intense Events of 2024

Primary author

Martin Schrön (Helmholtz Centre for Environmental Research GmbH - UFZ, Leipzig, Germany)

Co-authors

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