The turbulent structure of the solar wind from observations in the decameter radio wavelength range

被引:0
|
作者
Braude, SY [1 ]
Galanin, VV [1 ]
Inyutin, GA [1 ]
Men, AV [1 ]
Mori, K [1 ]
Rashkovskii, SL [1 ]
Sinitsyn, VG [1 ]
Sharykin, NK [1 ]
机构
[1] TOKYO COMMUN RES LAB,TOKYO,JAPAN
来源
ASTRONOMICHESKII ZHURNAL | 1995年 / 72卷 / 05期
关键词
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Results of observations of scattering of the decameter radio emission of a compact object in the source 3C 144 on inhomogeneities in the electron density of the solar wind plasma over a wide range of elongation on the URAN-1 and URAN-4 radio interferometers with baselines 42.3 and 613 km are presented. The experimental relationships obtained are compared with calculations made for a power law inhomogeneity spectrum. Dependences of the results of the calculations on a number of solar wind plasma parameters are presented, and probable values for these parameters are estimated.
引用
收藏
页码:761 / 766
页数:6
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