Solar Energetic Particles and Trapped Radiation in the Near-Earth Space: Space Experiments and Modelling

被引：3
作者：
Kalegaev, V [1 ]
Kaportseva, K. [1 ]
Nikolaeva, N. [1 ]
Shugay, Yu [1 ]
Vlasova, N. [1 ]
机构：
[1] Moscow MV Lomonosov State Univ, Skobeltsyn Inst Nucl Phys, Moscow, Russia
来源：
PHYSICS OF ATOMIC NUCLEI | 2021年 / 84卷 / 06期
基金：
俄罗斯基础研究基金会;
关键词：
CORONAL MASS EJECTIONS; PROTON EVENTS; TIME; PROPAGATION; FORECAST; STREAMS; CYCLE; CMES;
D O I：
10.1134/S1063778821130147
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
Among the factors of space weather, one of the most dangerous phenomena is radiation. Radiation in space exists due to the presence of charged particles of different nature and creates problems for the ''vitality'' of not only the spacecraft, but also of humans. The main radiation threats are solar and galactic cosmic rays, fluxes of precipitating magnetospheric particles and trapped particles of the Earth's radiation belts. They are as dangerous as other natural disasters: earthquakes, tsunamis, floods. Solar and geomagnetic activity, which determine space weather, can cause drastic changes in physical conditions in geospace, which affect technological systems located both in space and in polar regions on the surface of the Earth. To prevent emergencies associated with cosmic factors, it is necessary to constantly monitor the solar activity and the state of the space environment.
引用
收藏
页码：1105 / 1113
页数：9
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