5–9 Oct 2026
INPE
America/Sao_Paulo timezone

Cosmic Ray Muon Forbush Decrease and Its Relation with ICMEs

7 Oct 2026, 11:30
15m
IAI (INPE)

IAI

INPE

Oral Solar, Heliospheric and Magnetospheric Physics Oral Presentations | Apresetações Orais

Speaker

Marlos Rockenbach (INPE)

Description

Muons are secondary particles formed by the interaction of a primary Galactic Cosmic Ray with the Earth's atmosphere, whose primary proton is influenced by a solar magnetic structure that travels throughout the heliosphere. This interaction between the primary proton and solar structures is known as Heliospheric Modulation of cosmic rays. The solar structures that cause the most intense cosmic ray modulation are the Interplanetary Coronal Mass Ejections (ICMEs), whose magnetic structure called Magnetic Cloud, have a helical magnetic field, which hinders the entry of cosmic rays inside the ICME, causing a decrease on the cosmic ray observations when this structure intercepts the Earth. The Forbush Diminution of cosmic rays was first linked to solar structure by S. E. Forbush in 1937, who had this phenomenon named in his honor for his discovery. In this sense, a detailed analysis of cosmic ray Forbush decrease observed by muon detectors on the Earth's surface is necessary to understand whether the polarity of the helical structure of the magnetic cloud plays an important role in the size of the decay and its recovery time.

Authors

Marlos Rockenbach (INPE) Dr Alisson Dal Lago (INPE) Dr Rosemeire Oliveira (3Grupo de Pesquisa em Matemática Científica e Computacional) Dr Marcos Oliveira (IFSP) Mr Jesus Nuñez (INPE)

Presentation materials

There are no materials yet.