Solar cosmic rays: 75 years of research

被引:0
作者
Miroshnichenko, L. I. [1 ,2 ]
机构
[1] Russian Acad Sci, Ionosphere & Radio Wave Propagat IZMIRAN, Pushkov Inst Terr Magnetism, Kaluzhskoe Shosse 4, Moscow 108840, Russia
[2] Lomonosov Moscow State Univ, Skobeltsyn Inst Nucl Phys, Leninskie Gory 1, Moscow 119991, Russia
关键词
Sun; solar flares; particle acceleration; solar cosmic rays; GROUND-LEVEL ENHANCEMENT; CORONAL MASS EJECTIONS; 2000; JULY; 14; PARTICLE-ACCELERATION; PROTON EVENTS; GAMMA-RAY; ENERGETIC PARTICLES; SHOCK ACCELERATION; SEPTEMBER; 29; AD; 774-775;
D O I
10.3367/UFNe.2017.03.038091
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The 28th of February 2017 marked the 75th anniversary of the first confident detection of solar cosmic rays (SCRs), a term referring to accelerated solar particles with energies from about 10(6) to similar to 10(10)-10(11) eV. The present paper reviews the key observational and theoretical results on SCRs that have been accumulated over this period. The history of the discovery of SCRs is briefly described, together with SCR recording techniques and instruments, and some physical, methodical, and practical aspects of SCR generation are discussed in more detail. Special attention is given to mechanisms of charged particle acceleration at and near the Sun. Current ideas on the interaction of solar cosmic rays with the solar atmosphere, peculiarities of their transport in interplanetary magnetic fields, movements in Earth's magnetosphere, and their impact on Earth's atmosphere are reviewed. It is shown that this field of space physics has produced many results of fundamental interest for astrophysics, solar-terrestrial physics, geophysics, and practical cosmonautics (astronautics).
引用
收藏
页码:323 / 352
页数:30
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