Size Distribution of Forbush Effects


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The distribution of Forbush effect magnitude for cosmic rays with a rigidity of 10 GV observed in 1957–2016 is studied based on a large amount of experimental data from the IZMIRAN database of Forbush effects and interplanetary disturbances. It is demonstrated that the distribution for sufficiently strong Forbush effects follows a power law with an index close those determined earlier for coronal mass ejections. The obtained distributions are evidence that almost all Forbush effects with magnitudes exceeding 1.4% were included into the database. The majority of these effects are associated with interplanetary coronal mass ejections.

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A. Melkumyan

Gubkin Russian State University of Oil and Gas

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Email: amelkumyan6@gmail.com
俄罗斯联邦, Moscow, 119991

A. Belov

Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN),
Russian Academy of Sciences

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Email: abelov@izmiran.ru
俄罗斯联邦, MoscowTroitsk, 108840

M. Abunina

Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN),
Russian Academy of Sciences

Email: abelov@izmiran.ru
俄罗斯联邦, MoscowTroitsk, 108840

A. Abunin

Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN),
Russian Academy of Sciences

Email: abelov@izmiran.ru
俄罗斯联邦, MoscowTroitsk, 108840

E. Eroshenko

Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN),
Russian Academy of Sciences

Email: abelov@izmiran.ru
俄罗斯联邦, MoscowTroitsk, 108840

V. Oleneva

Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN),
Russian Academy of Sciences

Email: abelov@izmiran.ru
俄罗斯联邦, MoscowTroitsk, 108840

V. Yanke

Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN),
Russian Academy of Sciences

Email: abelov@izmiran.ru
俄罗斯联邦, MoscowTroitsk, 108840

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