Vector anisotropy of cosmic rays in the beginning of Forbush effects


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We consider the behavior of anisotropy and density of galactic cosmic rays in the first hours of Forbush effects from 1957 to 2014 initiated by the arrival of a shock wave. It has been shown that, as early as the event commencement, the first harmonic of anisotropy tends to increase substantially and its direction changes significantly. The more is powerful the interplanetary disturbance, the greater are the changes. Based on changes in some parameters of anisotropy and density, we can estimate the heliolongitude of the disturbance source, as well as the further development of the Forbush effect and geomagnetic activity.

作者简介

A. Belov

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

编辑信件的主要联系方式.
Email: abelov@izmiran.ru
俄罗斯联邦, Kaluzhskoe shosse 4, Troitsk, Moscow, 108840

M. Abunina

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

Email: abelov@izmiran.ru
俄罗斯联邦, Kaluzhskoe shosse 4, Troitsk, Moscow, 108840

A. Abunin

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

Email: abelov@izmiran.ru
俄罗斯联邦, Kaluzhskoe shosse 4, Troitsk, Moscow, 108840

E. Eroshenko

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

Email: abelov@izmiran.ru
俄罗斯联邦, Kaluzhskoe shosse 4, Troitsk, Moscow, 108840

V. Oleneva

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

Email: abelov@izmiran.ru
俄罗斯联邦, Kaluzhskoe shosse 4, Troitsk, Moscow, 108840

V. Yanke

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

Email: abelov@izmiran.ru
俄罗斯联邦, Kaluzhskoe shosse 4, Troitsk, Moscow, 108840

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