Signal Detection Performed by Log Periodic Dipole Antenna (LPDA) in Solar Monitoring

Z.S. Hamidi; Z.Z Abidin; Z.A. Ibrahim; C. Monstein; N.N.M. Shariff

doi:10.14331/ijfps.2012.330029

Authors

Z.S. Hamidi Department of Physics, Faculty Science, University of Malaya, 50603 Kuala Lumpur, Malaysia Author
Z.Z Abidin Department of Physics, Faculty Science, University of Malaya, 50603 Kuala Lumpur, Malaysia Author
Z.A. Ibrahim Department of Physics, Faculty Science, University of Malaya, 50603 Kuala Lumpur, Malaysia Author
C. Monstein Institute of Astronomy, ETH, Zurich, Switzerland Author
N.N.M. Shariff Department of Physics, Faculty Science, University of Malaya, 50603 Kuala Lumpur, Malaysia Author

DOI:

https://doi.org/10.14331/ijfps.2012.330029

Keywords:

Log Periodic Dipole Antenna (LPDA), signal detection, CALLISTO

Abstract

This article describes signal detection by Log-Periodic Dipole-Antenna (LPDA) which designed for solar monitoring with very high-performance in 45 MHz till 870 MHz. The LPDA, consisting of 19-elements, achieves a gain higher than 10 dBi with low noise amplifier. It has successfully setup at National Space Centre, Banting on 15th February 2012. Our objective in this work is to detect any signal at National Space Centre, Sg. Lang, Selangor which connected with CALLISTO spectrometer. Detailed analysis also revealed the interference sources that caused interruption of solar signal. Specific range of frequency that considered a minimum Radio Frequency Interference (RFI) also has been done. We found that high level interference is received from FM-band (80 MHz – 108 MHz), from VHF-band and from UHF-band. In the UHF-band, we could recognize (beside a lot of analog-TV) two (2) DVB-T channels between 650 MHz and 700 MHz. The ‘comb’ of signals proves that the whole system is working correctly with good sensitivity. This feature can be used to check the system as part of periodic maintenance. Beside the established detection techniques, some improvization of LPDA is also highlighted. The noise floor at all frequencies below 3 dB is in fact not noise, but represents standing waves due to the fact that the LPD antenna is not matched to the 50Ω coaxial cable due to the small size of boom’s diameter. Total sensitivity can be improved by impedance matching of antenna and coaxial cable.

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Author Biography

Z.S. Hamidi, Department of Physics, Faculty Science, University of Malaya, 50603 Kuala Lumpur, Malaysia

Faculty of Applied Sciences, MARA University of Technology, UiTM 40450 Shah Alam Selangor, Malaysia

References

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