Development of 408MHz V-shape Dipole-based Antenna for Solar Observation

 
 
 
  • Abstract
  • Keywords
  • References
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  • Abstract


    Solar is one of the most observed object in a radio astronomy, as it is highly affects the space weather. In this paper, a new 408 MHz dipole-based antenna for solar radio telescope system is presented. High gain up to 11.30 dBi with beamwidth size of about 58° has been achieved by optimizing the structure of parasitic elements on the antenna. Measurement result shows a good agreement with simulation, with error rate on frequency peak down to 0.98%. The proposed antenna has been utilized in several solar observation and the results are also presented in this paper.

     


  • Keywords


    V-Shape, Dipole-based Antenna, Solar Observation.

  • References


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Article ID: 26360
 
DOI: 10.14419/ijet.v8i1.9.26360




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