Solar wind and geomagnetic activity

被引:0
|
作者
Costa, E., Jr. [1 ,3 ]
Simoes, F. J. R., Jr. [2 ,3 ]
Cardoso, F. R. [3 ]
Alves, M. V. [3 ]
机构
[1] Inst Fed Minas Gerais, Ouro Preto, MG, Brazil
[2] Fundacao Univ Fed Pelotas, Dept Fis, Pelotas, RS, Brazil
[3] Inst Nacl Pesquisas Espaciais, Lab Assoc Plasma, Sao Jose Dos Campos, SP, Brazil
来源
关键词
space physics; solar wind; geomagnetic activity; AURORAL KILOMETRIC RADIATION; PARAMETERS; INTENSITY; STORMS; AE;
D O I
10.1590/S1806-11172011000400001
中图分类号
G40 [教育学];
学科分类号
040101 ; 120403 ;
摘要
Nowadays, there are a lot of doubts about solar wind generation and most of what is known comes from observations. This is because its generation is too complex and the non-existence of observations in the regions where the wind is accelerated. However, near the Earth its features are well known and always measured. Solar wind interaction with the Earth magnetosphere leads to the formation of several magnetospheric regions. If the conditions are favorable such interaction leads also to geomagnetic activity. Studying geomagnetic activity variations caused by solar wind conditions is a main topic in space physics. For practical and technological aplications such variations can, for instance, damage ground and onbord satellites sistems because of the enhancement in atmospheric currents and levels of radiation, making this kind of research so important. This paper presents a brief revision about some of the main effects of solar wind and Earth's magnetosphere interaction.
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页数:8
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