Properties of a cosmic ray flux crossing the magnetic cloud-solar wind interface

Petukhov, I. S.; Petukhov, S. I.

doi:10.3103/s1062873815050354

Bull. Russ. Acad. Sci. Phys.

2015

DOI: 10.3103/s1062873815050354

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Properties of a cosmic ray flux crossing the magnetic cloud-solar wind interface

I. S. Petukhov

S. I. Petukhov

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2023

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Cited by 2 publications

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Efficiency of Mechanisms for the Formation of Sporadic Forbush Decreases

Petukhova,

Petukhov,

Petukhov

2023

Bull. Russ. Acad. Sci. Phys.

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Efficiency of Mechanisms for the Formation of Sporadic Forbush Decreases

Petukhova,

Petukhov,

Petukhov

2023

Bull. Russ. Acad. Sci. Phys.

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Efficiency of mechanisms for the formation of sporadic Forbush decreases

Petukhova,

Petukhov,

Petukhov

2023

Izvestiâ Akademii nauk SSSR. Seriâ fizičeskaâ

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From the measurements of the neutron monitors world network in the period 1996–2018, 31 strong Forbush decreases (5%) were identified that satisfy the accepted event selection criterion. The superposed epoch analyses is used to determine the consistent spatial distributions of the solar wind parameters and the decrease in cosmic ray density. It has been established that the contributions of the formation mechanisms of the Forbush decrease differ greatly in two groups of events. The difference may be since the formation of the Forbush depression in one group occurs in the frontal part, and in the other group in the peripheral part of the disturbance.

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Properties of a cosmic ray flux crossing the magnetic cloud-solar wind interface

Cited by 2 publications

References 5 publications

Efficiency of Mechanisms for the Formation of Sporadic Forbush Decreases

Efficiency of Mechanisms for the Formation of Sporadic Forbush Decreases

Efficiency of mechanisms for the formation of sporadic Forbush decreases

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