Variations of Geomagnetic Cosmic Ray Thresholds and Their Latitudinal Behavior in the Period of Solar Disturbance in September 2005
- 作者: Tyasto M.I.1, Danilova O.A.1, Sdobnov V.E.2
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隶属关系:
- St. Petersburg Branch of Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation
- Institute of Solar–Terrestrial Physics, Siberian Branch
- 期: 卷 58, 编号 1 (2018)
- 页面: 28-35
- 栏目: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/156623
- DOI: https://doi.org/10.1134/S0016793218010152
- ID: 156623
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详细
The period of interplanetary, geomagnetic and solar disturbances of September 7–15, 2005, is characterized by two sharp increases of solar wind velocity to 1000 km/s and great Dst variation of the geomagnetic field (~140 nT). The time variations of theoretical and experimental geomagnetic thresholds observed during this strong geomagnetic storm, their connection with solar wind parameters and the Dst index, and the features of latitudinal behavior of geomagnetic thresholds at particular times of the storm were studied. The theoretical geomagnetic thresholds were calculated with cosmic ray particle tracing in the magnetic field of the disturbed magnetosphere described by Ts01 model. The experimental geomagnetic thresholds were specified by spectrographic global survey according to the data of cosmic ray registration by the global station network.
作者简介
M. Tyasto
St. Petersburg Branch of Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation
编辑信件的主要联系方式.
Email: office@izmiran.spb.ru
俄罗斯联邦, St. Petersburg
O. Danilova
St. Petersburg Branch of Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation
Email: office@izmiran.spb.ru
俄罗斯联邦, St. Petersburg
V. Sdobnov
Institute of Solar–Terrestrial Physics, Siberian Branch
Email: office@izmiran.spb.ru
俄罗斯联邦, Irkutsk
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