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First Light Detection of A Single Solar Radio Burst Type III Due To Solar Flare Event

Treść / Zawartość
Identyfikatory
Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
The eruption mechanism of solar flares and type III are currently an extremely active area of research, especially during the solar cycle is towards maximum. In this case, the total energy of solar burst type III is of the order of solar flare with the explosion of the energy can up to 1015 ergs. The solar flare event is one of the most spectacular explosions that still be on-going study in the solar physics world. This event occurred at 2:000 UT on 15th April 2012 is due to the explosion of the magnetic energy in from the chromosphere and converted into the heating, mass motion and particle acceleration which can be detected by solar radio burst type III. In this work, we will highlight our first light detection of very tiny solar radio burst type III, which has been observed at the National Space Centre, Banting, Selangor detected by the Compound Low Cost Low Frequency Transportable Observatories (CALLISTO) system at 5:53:23. The region of the data is from 150 − 400 MHz in radio region. This burst is drifted from 150 MHz till 260 MHz. It represents a total energy of 6.2035 × 10-7 eV − 1.0753 × 10-6 eV. This fast drift burst is a continuity of the acceleration of the particles which is intermittent, and can be observed since the explosion of the solar flare. Although the burst is very tiny, it is still significant because this burst is the first detection of a single type III burst from our site. Still, the acceleration of the particles can be detected from Earth in the radio region within 3 hours period of observation at the post stage of solar flare.
Rocznik
Strony
51--58
Opis fizyczny
Bibliogr. 22 poz., rys., tab., wykr.
Twórcy
autor
  • School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia, zetysh@salam.uitm.edu.my
  • Academy of Contemporary Islamic Studies (ACIS), MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
autor
  • Institute of Astronomy, Wolfgang-Pauli-Strasse 27, Building HIT, Floor J, CH-8093 Zurich, Switzerland
Bibliografia
  • [1] D. Herdiwijaya, S. Imelda, Jurnal Matematika dan Sains 11 (2006) 7.
  • [2] A. O. Benz, Plasma Astrophysics, Springer, Dordrecht, 2002.
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  • [4] G. D. Fleishman, Gary D. E., Nita G. M., ApJ 593 (2003).
  • [5] Z. S.Hamidi, U. F. S. U. Ibrahim, Z. Z. Abidin, Z. A. Ibrahim, N. N. M. Shariff, International Journal of Fundamental Physical Sciences 3 (2013) 20-23.
  • [6] M. V. Goldman, D. F. Smith, Physics of the Sun, Dordrecht: Reidel, 1986.
  • [7] M. Karlický, Kosugi T. , A & A 419 (2004).
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  • [10] A. O. Benz, C. Monstein, A. H. Meyer, Solar Phys. 226 (2005) 143-151.
  • [11] Z. S. Hamidi, Z. Abidin, Z. Ibrahim, C. Monstein, N. Shariff, International Journal of Fundamental Physical Sciences 2 (2012) 32-34.
  • [12] Z. S. Hamidi, N. N. M. Shariff, C. Monstein, Z.A. Ibrahim, International Letters of Chemistry, Physics and Astronomy 7 (2014) 37-44.
  • [13] Z. S. Hamidi, N. N. M. Shariff, International Letters of Chemistry, Physics and Astronomy 4 (2014) 29-36.
  • [14] Z. S. Hamidi, N. N. M. Shariff, Thermal Energy and Power Engineering 3 (2014) 181-184.
  • [15] Z. S. Hamidi, S. Chumiran, A. Mohamad, N. Shariff, Z. Ibrahim, N. Radzin, N. Hamzan, N. Anim, A. Alias, American Journal of Modern Physics 2 (2013) 4.
  • [16] Z. S. Hamidi, N. N. M. Shariff, Z. A. Ibrahim, Z. Z. Abidin, Solar Studies in Radio Emission and Optical Photometry, Dimensi Penyelidikan Astronomi Islam, University of Malaya Publisher, University of Malaya, 2013, pp. 33-40.
  • [17] Z. S. Hamidi, Z. Ibrahim, Z. Abidin, M. Maulud, N. Radzin, N. Hamzan, N. Anim, N. Shariff, International Journal of Applied Physics and Mathematics 2 (2011) 3.
  • [18] Z. S.Hamidi, N. N. M. Shariff, Evaluation of Signal to Noise Ratio (SNR) of Log Periodic Dipole Antenna (LPDA) Business Engineering and Industrial Applications Colloquium 2013, IEEE, Langkawi, Malaysia, 2013, pp. 434-438.
  • [19] Z. S. Hamidi, et al., International Journal of Fundamental Physical Sciences 2 (2012) 4.
  • [20] A. O. Benz, C. Monstein, H. Meyers, CALLISTO, A New Concept for Solar Radio Spectrometer, Kluwer Academic Publishers, The Netherland, 2004.
  • [21] Z. S. Hamidi, N. Anim, N. N. M. Shariff, Z. Z. Abidin, Z. A. Ibrahim, C. Monstein, Dynamical structure of solar radio burst type III as evidence of energy of solar flares, in: R.Shukor (Ed.), PERFIK 2012, American Institute of Physics, Malaysia, 2013, pp. 11-15.
  • [22] Z. S. Hamidi, N. Shariff, Z. Abidin, Z. Ibrahim, C. Monstein, Middle-East Journal of Scientific Research 12 (2012) 6.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-8022a3ce-a17b-4293-9c1c-490eb0b79b69
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