Vector anisotropy of cosmic rays in the beginning of Forbush effects


Дәйексөз келтіру

Толық мәтін

Ашық рұқсат Ашық рұқсат
Рұқсат жабық Рұқсат берілді
Рұқсат жабық Тек жазылушылар үшін

Аннотация

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.

Авторлар туралы

A. Belov

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

Хат алмасуға жауапты Автор.
Email: abelov@izmiran.ru
Ресей, Kaluzhskoe shosse 4, Troitsk, Moscow, 108840

M. Abunina

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

Email: abelov@izmiran.ru
Ресей, Kaluzhskoe shosse 4, Troitsk, Moscow, 108840

A. Abunin

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

Email: abelov@izmiran.ru
Ресей, Kaluzhskoe shosse 4, Troitsk, Moscow, 108840

E. Eroshenko

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

Email: abelov@izmiran.ru
Ресей, Kaluzhskoe shosse 4, Troitsk, Moscow, 108840

V. Oleneva

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

Email: abelov@izmiran.ru
Ресей, Kaluzhskoe shosse 4, Troitsk, Moscow, 108840

V. Yanke

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

Email: abelov@izmiran.ru
Ресей, Kaluzhskoe shosse 4, Troitsk, Moscow, 108840

Қосымша файлдар

Қосымша файлдар
Әрекет
1. JATS XML

© Pleiades Publishing, Ltd., 2017