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Space Weather: The Significance of e-CALLISTO (Malaysia) As One of Contributor of Solar Radio Burst Due To Solar Activity

Treść / Zawartość
Identyfikatory
Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
The impact of solar activities indirectly affected the conditions of earth's climate and space weather in general. In this work, we will highlight a low cost project, however, potentially gives a high impact through a dedicated long-term and one of the most successful space weather project. This research is a part of an initiative of the United Nations together with NASA in order to support developing countries participating in „Western Science‟ research. At the beginning of 2007, the objective to monitor the solar activities (solar flares and Coronal Mass Ejections) within 24 hours all over the world has positively turned to reality. Realize how important for us to keep doing a research about the solar bursts, by using the new radio spectrometer, CALLISTO. This research is not only hoping to give a knowledge to the people about how the solar bursts are produced, the characteristics of every type of solar burst at the wide range (45 MHz to 870 MHz) but also the effect of the solar burst toward the Earth. By using the same CALLISTO spectrometer within the 45-870 MHz, designing and leading by Christian Monstein from ETH Zurich, Switzerland, this research project is the one of successful project under ISWI program. Malaysia becomes the 19th countries that involve this research. One of the advantages to start the solar monitoring in Malaysia is because our strategic location as equator country that makes possible to observing a Sun for 12 hours daily throughout a year. We strongly believe that Malaysia as one of contributor of solar activity data through E-CALLISTO network. This is a very good start for developing a radio astronomy in Malaysia.
Rocznik
Tom
Strony
37--44
Opis fizyczny
Bibliogr. 27 poz., rys.
Twórcy
autor
  • MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
  • Department of Science and Technology Studies, University of Malaya, 50603, Kuala Lumpur, Malaysia
autor
  • Institute of Astrophysics, ETH, Zurich, Switzerland
  • Department of Physics, University of Malaya, 50603, Kuala Lumpur, Malaysia
Bibliografia
  • [1] S. M. White, Asian Journal of Physics 16 (2007) 189-207.
  • [2] J. S. Hey, S. J. Parsons, J. W. Phillips, Monthly Notices of the Royal Astronomical Society 108 (1948) 354-371.
  • [3] R. Tousey, The solar corona, in: M.J. Rycroft, S.K. Runcorn (Eds.), Space Research XIII, Proceedings, Akademie-Verlag, Berlin, Madrid, Spain, 10-24 May, 1972, pp. 713-730.
  • [4] N. Gopalswamy, A Global Picture of CMEs in the Inner Heliosphere, in: G. Poletto, Suess, S.T. (Ed.), Astrophysics and Space Science 2004, pp. 201-251.
  • [5] R. A. Howard, Sheeley Jr. N. R., Michels D. J., Koomen M. J., J. Geophys. Res. 90 (1985) 8173-8191.
  • [6] O. C. St Cyr, et al., J. Geophys. Res. 18 (2000) 169-186.
  • [7] R. M. E. A. H. Illing, A. J., J. Geophys. Res. 90 (1985) 275-282.
  • [8] A. O. Benz, C. Monstein, H. Meyer, P. K. Manoharan, R. Ramesh, A. Altyntsev, A. Lara, J. Paez, K.-S. Cho, Earth Moon and Planets 104 (2009) 277-285.
  • [9] A. O. Benz, C. Monstein, H. Meyers, CALLISTO, A New Concept for Solar Radio Spectrometer, Kluwer Academic Publishers, The Netherland, 2004.
  • [10] F.-Y. Xu, Z.-C. Xu, G.-I.Y. Huang, M. Q.-J., X., H.-A. Wu, Solar Phys. 216 (2003).
  • [11] T. Kondo, T. Isobe, S. Igi, S. Watari, M. Okumaru, J. Communications Res. Lab. 42 (1995).
  • [12] K. Jiricka, M. Karlicky, O. Kepka, A. Tlamicha, Solar Phys. 147 (1993).
  • [13] H. S. Sawant, e. al., Sol. Phys. 200 (2001).
  • [14] G. Mann, A. Klassen, Astron. Astrophys. 441 (2005) 319-326.
  • [15] Z. S. Hamidi, N. Shariff, Z. Abidin, Z. Ibrahim, C. Monstein, Middle-East Journal of Scientific Research 12 (2012) 6.
  • [16] Z. S. 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).
  • [17] Z. S. Hamidi, Z. Abidin, Z. Ibrahim, N. Shariff, C. Monstein, International Journal of Engineering Research and Development 3 (2012) 3.
  • [18] Z. S. Hamidi, et al., International Journal of Fundamental Physical Sciences 2 (2012) 4.
  • [19] Z. S.Hamidi, N. N. M.Shariff, Evaluation of Signal to Noise Ratio (SNR) of LogPeriodic Dipole Antenna (LPDA) BEIAC 2013, IEEE, Langkawi, Malaysia, 2013, pp. 6.
  • [20] Z. S. Hamidi, Z. Abidin, Z. Ibrahim, N. Shariff, Indication of radio frequency interference (RFI) sources for solar burst monitoring in Malaysia, AIP Conference Proceedings 1454 (2012) 43.
  • [21] Z. S.Hamidi, N. N. M.Shariff, R. Umar, Malaysia Thailand Journal of Physics 3 (2012) 6.
  • [22] Z. Z. Abidin, Radio Astronomy Research in Malaysia: Past, Present and Future., Proc. of Space Science and Communication, 2009, pp. 179-181.
  • [23] Z. S. Hamidi, N. N. M. Shariff, C. Monstein, The International Journal of Engineering 1 (2012) 3.
  • [24] Z. S. Hamidi, Z. Abidin, Z. Ibrahim, C. Monstein, N. M. Shariff, Signal Detection Performed by Log Periodic Dipole Antenna (LPDA) in Solar Monitoring, (2012).
  • [25] Z. S. Hamidi, N. N. M. Shariff, International Letters of Chemistry, Physics and Astronomy 4 (2014) 29-36.
  • [26] Z. S. Hamidi, N. N. M. Shariff, International Letters of Chemistry, Physics and Astronomy 5 (2014) 32-42.
  • [27] Z. S. Hamidi, N. N. M. Shariff, International Letters of Chemistry, Physics and Astronomy 5 (2014) 43-49.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-02083f18-631b-41ac-bb34-e1f62b5fa0aa
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