Development of a Magnetic Loop Antenna for the Detection of Jovian Radiowaves at 20.1 MHz

被引：1

作者：

Galvis Rodriguez, Hamilton David ^{[1
]}

Quintero Salazar, Edwin Andres ^{[1
]}

Cardona Torres, Luisa Fernanda ^{[1
]}

机构：

[1] Univ Tecnol Pereira, Pereira, Colombia

来源：

TECCIENCIA | 2016年 / 11卷 / 20期

关键词：

Synchrotron Emission; Jovian Radio Emissions; Magnetic Loop Antenna;

D O I：

10.18180/tecciencia.2016.20.6

中图分类号：

T [工业技术];

学科分类号：

08 ;

摘要：

Radio waves coming from the planet Jupiter are electromagnetic phenomena generated by synchrotron emission mechanism, due to the interaction of Jovian magnetic field with charged particles produced by the satellite Io. These radio waves fall directly upon the ionosphere affecting earth's radio communications. At the Astronomical Observatory of the University of Technology of Pereira (OAUTP) the research group in Astro-engineering Alfa Orion, developed a magnetic loop antenna designed to resonate at 20.1 MHz, which coupled with the receptor and the software from NASA's Radio Jove project enabled the observation of radio sources A, B, C, IoA, IoB and IoC from Jupiter, allowing the construction of a database for the study of the Jovian activity in radio waves.

引用

页码：41 / 46

页数：6

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