5-9 October 2020
Online
Europe/Moscow timezone
The conference is over. We would like to thank all participants for their attendance!

Forbush decrease spectrum in a magnetic cloud in the 2004 July 27 event

5 Oct 2020, 19:45
15m
Poster Server (Discord)

Poster Server

Discord

Poster Astroparticle physics Poster session

Speaker

Anastasia Petukhova (Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy of SB RAS)

Description

Magnetic clouds affect the intensity of galactic cosmic rays. The diffusion mechanism is usually considered as the formation mechanism for Forbush decrease (FD) in a magnetic cloud. An FD is an observed decrease in the intensity of cosmic rays. There is a new theory of FD formation, in which the mechanism is the loss of particle energy in the electromagnetic field of a magnetic cloud. The shape of the FD spectrum is calculated for a wide range of particle energies in the 2004 July 27 event. According to the measurements of the global networks of ground-based neutron monitors and muon telescopes, synchronous changes in the FD amplitude in time indicate that the FD is formed in a magnetic cloud for all energies. However, the calculated FD spectrum differs from the obtained one from measurements. The reasons for the difference can be: 1) the mechanism of formation is the diffusion mechanism; 2) the method for determining the spectrum, using the notion of mean or median energy, needs additional studies.

Primary authors

Anastasia Petukhova (Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy of SB RAS) Dr. Ivan Petukhov (Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy of SB RAS) Dr. Stanislav Petukhov (1Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy of SB RAS)

Presentation Materials

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