Design a radio receiver for solar activity observation in VLF band

A. A. Al- Banna
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Abstract

Solar activity monitoring is important in our life because of its direct or indirect influence on our life, not only on ionospheric communications. To study solar activity, researchers need measuring and monitoring instruments, these instruments are mostly expensive and are not available in all universities. In this paper, a very low frequency radio receiver had been designed and implemented with components available in most markets to support the researchers, college students, and radio astronomy amateurs with a minimum input voltage less than 100µV, an output voltage less than 135 m V with no distortion and an overall gain of 34dB. A comparison had been done between two circuit structures using a workbench software program and experimentally done in the lab. Two antennas were experimentally tested and a loop antenna was chosen. The whole system was connected and tested to receive signals in the Lab and monitored on computer using HDSDR software program. Another experiment done outside the lab (at home), and the result was not good because of many high level interference noises.  
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设计了一种用于VLF波段太阳活动观测的无线电接收机
太阳活动监测不仅对电离层通信有直接或间接的影响,而且对我们的生活也有重要意义。为了研究太阳活动,研究人员需要测量和监测仪器,这些仪器大多是昂贵的,并不是所有的大学都有。本文设计并实现了一种极低频无线电接收机,使用大多数市场上可用的组件,以支持研究人员,大学生和射电天文学业余爱好者,最小输入电压小于100 μ V,输出电压小于135 m V,无失真,总增益为34dB。利用工作台软件程序和实验室实验对两种电路结构进行了比较。对两种天线进行了实验测试,选择了一种环形天线。整个系统在实验室进行了连接和测试,并在计算机上使用HDSDR软件程序进行了监控。在实验室外(家里)做了另一个实验,由于有很多高水平的干扰噪声,结果并不好。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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