Solar eclipse effects of 22 July, 2009 on the propagation of radio signals

被引:1
|
作者
Bhattacharya, R. [1 ]
Nag, A. [2 ]
Guha, R. [1 ]
Bhoumick, A. [1 ]
De, S. [2 ]
Bhattacharya, A. B. [2 ]
机构
[1] Univ Kalyani, Dept Environm Sci, Kalyani 741235, W Bengal, India
[2] Univ Kalyani, Dept Phys, Kalyani 741235, W Bengal, India
关键词
Solar eclipse; radio signals; ionospheric effects; VLF;
D O I
10.1007/s12648-010-0143-7
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The results of investigation of the variation of radio signal strengths during the solar eclipse on July 22, 2009 are reported in this paper. Observations of the radio signals transmitted from different radio stations at different frequencies and received at a particular observing site indicate a distinct change in signal strength around the time the eclipse umbra passes the propagation paths. The three types of variations in the eclipse day and particularly during its peak period are different from propagation under normal condition. The phenomena of signal variations, the noted "Inverted U-shape" at one of the frequencies before the occurrence of the eclipse and 13 to 15 minutes time difference between the enhancement of the signal strength and the onset of eclipse are some interesting characteristics. The results are interpreted by ionospheric D-layer behavior at such times.
引用
收藏
页码:1587 / 1595
页数:9
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