American Journal of Modern Physics

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Effective Temperature of the Sun Based on Log Periodic Dipole Antenna Performance In The Range From 45 MHz to 870 MHz

Received: 21 February 2013    Accepted:     Published: 10 March 2013
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Abstract

The Log Periodic Dipole Antenna (LPDA) performance of solar burst monitoring in the range of (45 -870) MHz is presented. This project is under the International Space Weather Initiative (ISWI) program in order to observe the solar activities within 12 hours per day. At the first stage, we make an effort by constructing LPDA that suitable with the criteria, specification and practical enough with 5.45 meter boom length size of the antenna. The rods then were perforated with nineteen (19) elements that were made of aluminum rods. Two (2) rod aluminums type with nineteenth (19) elements that signify different frequencies. The gain of this antenna is 6.67 which is required preamplifier to amplify the signal of the Sun. From the results, we found that the effective temperature of the antenna is 1.3 dB and the temperature of the Sun during that observation is 1578 K. Some suggestions on improving this design are also presented.

DOI 10.11648/j.ajmp.20130202.14
Published in American Journal of Modern Physics (Volume 2, Issue 2, March 2013)
Page(s) 58-60
Creative Commons

This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.

Copyright

Copyright © The Author(s), 2024. Published by Science Publishing Group

Keywords

Log Periodic Dipole Antenna (LPDA), Sun, Solar Burst, Effective Temperature

References
[1] G.H. Zhai, W. Hong, K. Wu, Z.Q. Kuai, Wideband substrate integrated printed log-periodic dipole array antenna, IET Microw. Antennas Propag. 4 (2010) 899-905.
[2] R. Carrel, The design of log-periodic dipole antennas, IRE International Convention Record, 1961, pp. 61- 75.
[3] Z.Z.e.a. Abidin, Investigation of Radio astronomical windows between 1 MHz-2060 MHz in University of Malaya, New Astron. 14 (2009) 579-583.
[4] Arnold O. Benz, C. Monstein, a.H. Meyer, CALLISTO, A New Concept for Solar Radio Spectrometers, Kluwer Aca-demic Publishers, 2004.
[5] D.J. McLean, a.N.R. Labrum, Solar Radiophysics, Cambridge University Press, Cambridge, 1985.
[6] N. Gopalswamy Geophysical Monograph Series 165 (2006).
[7] Z. Hamidi, Z. Abidin, Z. Ibrahim, N. Shariff, U.F.S.U. Ibrahim, R. Umar, Preliminary analysis of investigation Radio Frequency Interference (RFI) profile analysis at Universiti Teknologi MARA, IEEE, 2011, pp. 311-313.
[8] J. Carr, Some variations in log-periodic antenna structures, IRE Trans. Antennas Propag., 1961, pp. 229- 230.
[9] Z. Hamidi, Z. Ibrahim, Z. Abidin, M. Maulud, N. Radzin, N. Hamzan, N. Anim, N. Shariff, Designing and Constructing Log Periodic Dipole Antenna to Monitor Solar Radio Burst: e-Callisto Space Weather, (2012).
[10] Z. Hamidi, Z. Abidin, Z. Ibrahim, C. Monstein, N. Shariff, Signal Detection Performed by Log Periodic Dipole Antenna (LPDA) in Solar Monitoring, (2012).
[11] M.S.M. Aras, M.K.A. Rahim, Z.Rasin, M.Z.A.A. Aziz, An Array of Dielectric Resonator Antenna for wireless application, IEEE International RF and Microwave, 2008, pp. 459.463.
Author Information
  • Faculty of Applied Sciences, MARA University of Technology, UiTM S.Alam Selangor

  • Faculty of Applied Sciences, MARA University of Technology, UiTM P.Pinang

  • Faculty of Applied Sciences, MARA University of Technology, UiTM S.Alam Selangor

  • Faculty of Science, University Malaya, Kuala Lumpur, Malaysia

  • Faculty of Science, University Malaya, Kuala Lumpur, Malaysia

  • aculty of Electrical Engineering, MARA University of Technology, UiTM P.Pinang

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  • APA Style

    Z. S. Hamidi, S. H. Chumiran, Z. S. Hamidi, N. N. M. Shariff, Z. A. Ibrahim, et al. (2013). Effective Temperature of the Sun Based on Log Periodic Dipole Antenna Performance In The Range From 45 MHz to 870 MHz. American Journal of Modern Physics, 2(2), 58-60. https://doi.org/10.11648/j.ajmp.20130202.14

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    ACS Style

    Z. S. Hamidi; S. H. Chumiran; Z. S. Hamidi; N. N. M. Shariff; Z. A. Ibrahim, et al. Effective Temperature of the Sun Based on Log Periodic Dipole Antenna Performance In The Range From 45 MHz to 870 MHz. Am. J. Mod. Phys. 2013, 2(2), 58-60. doi: 10.11648/j.ajmp.20130202.14

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    AMA Style

    Z. S. Hamidi, S. H. Chumiran, Z. S. Hamidi, N. N. M. Shariff, Z. A. Ibrahim, et al. Effective Temperature of the Sun Based on Log Periodic Dipole Antenna Performance In The Range From 45 MHz to 870 MHz. Am J Mod Phys. 2013;2(2):58-60. doi: 10.11648/j.ajmp.20130202.14

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  • @article{10.11648/j.ajmp.20130202.14,
      author = {Z. S. Hamidi and S. H. Chumiran and Z. S. Hamidi and N. N. M. Shariff and Z. A. Ibrahim and A. Mohamad},
      title = {Effective Temperature of the Sun Based on Log Periodic Dipole Antenna Performance In The Range From 45 MHz to 870 MHz},
      journal = {American Journal of Modern Physics},
      volume = {2},
      number = {2},
      pages = {58-60},
      doi = {10.11648/j.ajmp.20130202.14},
      url = {https://doi.org/10.11648/j.ajmp.20130202.14},
      eprint = {https://download.sciencepg.com/pdf/10.11648.j.ajmp.20130202.14},
      abstract = {The Log Periodic Dipole Antenna (LPDA) performance of solar burst monitoring in the range of (45 -870) MHz is presented. This project is under the International Space Weather Initiative (ISWI) program in order to observe the solar activities within 12 hours per day. At the first stage, we make an effort by constructing LPDA that suitable with the criteria, specification and practical enough with 5.45 meter boom length size of the antenna. The rods then were perforated with nineteen (19) elements that were made of aluminum rods. Two (2) rod aluminums type with nineteenth (19) elements that signify different frequencies. The gain of this antenna is 6.67 which is required preamplifier to amplify the signal of the Sun.  From the results, we found that the effective temperature of the antenna is 1.3 dB and the temperature of the Sun during that observation is 1578 K. Some suggestions on improving this design are also presented.},
     year = {2013}
    }
    

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  • TY  - JOUR
    T1  - Effective Temperature of the Sun Based on Log Periodic Dipole Antenna Performance In The Range From 45 MHz to 870 MHz
    AU  - Z. S. Hamidi
    AU  - S. H. Chumiran
    AU  - Z. S. Hamidi
    AU  - N. N. M. Shariff
    AU  - Z. A. Ibrahim
    AU  - A. Mohamad
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    T2  - American Journal of Modern Physics
    JF  - American Journal of Modern Physics
    JO  - American Journal of Modern Physics
    SP  - 58
    EP  - 60
    PB  - Science Publishing Group
    SN  - 2326-8891
    UR  - https://doi.org/10.11648/j.ajmp.20130202.14
    AB  - The Log Periodic Dipole Antenna (LPDA) performance of solar burst monitoring in the range of (45 -870) MHz is presented. This project is under the International Space Weather Initiative (ISWI) program in order to observe the solar activities within 12 hours per day. At the first stage, we make an effort by constructing LPDA that suitable with the criteria, specification and practical enough with 5.45 meter boom length size of the antenna. The rods then were perforated with nineteen (19) elements that were made of aluminum rods. Two (2) rod aluminums type with nineteenth (19) elements that signify different frequencies. The gain of this antenna is 6.67 which is required preamplifier to amplify the signal of the Sun.  From the results, we found that the effective temperature of the antenna is 1.3 dB and the temperature of the Sun during that observation is 1578 K. Some suggestions on improving this design are also presented.
    VL  - 2
    IS  - 2
    ER  - 

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