WIND STRUCTURE FROM AMPLITUDE FLUCTUATIONS IN PERSISTENT RADIO METEOR ECHOES

被引：6

作者：

PHILLIPS, E

机构：

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

来源：

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

关键词：

D O I：

10.1016/0032-0633(69)90084-1

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The amplitude fluctuations which are almost always present in persistent radio echoes from meteor trains can be interpreted in terms of the wind structure in the meteor region of the atmosphere. Measurement of parameters describing the onset of the fluctuations are in agreement with a horizontal wind velocity profile which is a sinusoidal function of height, the amplitude of the sinusoid increasing exponentially with height. © 1969.

引用

页码：553 / &

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