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Development of a Simple Home-Brew Radio Telescope
Journal
Advances in Environmental Engineering and Green Technologies
Analyzing the Physics of Radio Telescopes and Radio Astronomy
ISSN
2326-9162
Date Issued
2020
Author(s)
DOI
10.4018/978-1-7998-2381-0.ch003
Abstract
In this chapter, the design and construction of a simple home-brew radio telescope are illustrated. The radio telescope is built essentially from commercial off-the-shelf components. The main components include an offset prime-focus Ku-band reflector antenna, RF detector circuit, Arduino microcontroller, and a computer. To demonstrate the viability of the telescope, a drift-scan of the sun was performed. From the measurement, it is observed that the radiation signal from the sun has a peak power of –34.3 dBm, half power of –35.4 dBm, and a beamwidth of 3.13o. The impact of rain on the signal from the sky was also investigated. The result shows that there was a noticeable degradation of the power received. A significant amount of energy is absorbed by the dense water vapour in the atmosphere.
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