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

页码：761 / 766

页数：6

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