Methods of local interstellar medium investigation

被引：0
|
作者：
Kurt, V. G. [1 ]
Mironova, E. N. [1 ]
机构：
[1] Russian Acad Sci, PN Lebedev Phys Inst, Astro Space Ctr, Moscow 119991, Russia
来源：
PHYSICS-USPEKHI | 2013年 / 56卷 / 09期
关键词：
HYDROGEN ABSORPTION CELL; INTER-PLANETARY EMISSION; ALPHA LINE-PROFILE; SOLAR-WIND; PICKUP IONS; INTERPLANETARY HYDROGEN; HELIUM PARAMETERS; ATOMIC-HYDROGEN; MAGNETIC-FIELD; HELIOSPHERE;
D O I：
10.3367/UFNe.0183.201309e.0963
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The question of the Sun's motion relative to the local interstellar medium (LISM) is examined. Results from Russian, US, and French satellites and space probes observing scattered solar radiation in hydrogen Lyman-alpha (lambda = 1215.7 angstrom) and helium (lambda = 584 angstrom) lines are presented. Data are briefly discussed on the direct registration inside the Solar System of neutral helium atoms, picked-up helium ions, and fast neutral hydrogen atoms entering from the LISM. The fast neutral hydrogen atoms arise in the region of solar wind-LISM interaction.
引用
收藏
页码：910 / 918
页数：9
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