RADIO INVESTIGATION OF SOLAR PLASMA

被引：88

作者：

HEWISH, A

SYMONDS, MD

机构：

[1] Department of Physics, University of Cambridge, Cambridge, England

来源：

PLANETARY AND SPACE SCIENCE | 1969年 / 17卷 / 03期

关键词：

D O I：

10.1016/0032-0633(69)90064-6

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Observations of interplanetary scintillation and of the angular spectrum of radio waves scattered by the solar plasma are discussed. The scintillation index is found to vary as (distance)-1.6 in the range 0.1-1.5 a.u. and the scale of the plasma irregularities is derived in the range 0.1-1.0 a.u. Scintillation observed in the anti-solar direction gives no indication of a magnetospheric tail. Data obtained in 1967 show no enhancement of the solar wind at high heliocentric latitude. © 1969.

引用

页码：313 / &

共 8 条

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[5] LITTLE LT, 1968, PRIVATE COMMUNICATIO
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[7] IRREGULARITIES OF PLASMA DENSITY IN SOLAR NEIGHBOURHOOD
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HEWISH, A
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