Development of a Simple Home-Brew Radio Telescope

Author:

Yeap Kim Ho1ORCID,Lim Wei Gie1,Tang Tee2,Dakulagi Veerendra3ORCID

Affiliation:

1. Universiti Tunku Abdul Rahman, Malaysia

2. Queensland University of Technology, Australia

3. Lincoln University College, Malaysia

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.

Publisher

IGI Global

Reference10 articles.

1. Investigation of radio astronomical windows between 1MHz and 2060MHz in Universiti Malaya, Malaysia

2. Adnan, S. B. R. B. S. (2010). The study of radio frequency interference (RFI) for radio astronomy in some remote locations in peninsular Malaysia. Master Dissertation. University of Malaya.

3. A Simple Radio Telescope Operating at Ku Band for Educational Purposes

4. Design and simulation of Ku-Band Low-Noise Block Down-Converter in 0.18 micrometer CMOS technology

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