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2016 | 35 | 30-43
Article title

The Formation of Fundamental Structure of Solar Radio Burst Type II Due X6.9 Class Solar Flare

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EN
Abstracts
EN
A vigorous solar flare event marked on the spectrometer of the CALLISTO data, being one of the highest solar flare event that successfully detected. The formation of solar burst type II in meter region and their associated with X6. 9-class solar flares have been reported. The burst has been observed at the Blein Obsevatory, Switzerland, which detected by the Compound Astronomical Low-cost Low-frequency Instrument for Spectroscopy and Transportable Observatory (CALLISTO) system in the range of 170-870 MHz in the two polarizations of left and right circular polarization. It occurred between 08:01 UT to 08:08 UT within 7 minutes. The Compound Astronomical Low-cost Low-frequency Instrument for Spectroscopy and Transportable Observatory CALLISTO spectrometer is a solar dedicated spectrometer system that has been installed all over the world to monitor the Sun activity in 24 hours. The growth of this burst is often accompanied by abundance enhancement of particles which may take the form of multiple independent drifting bands or other forms of fine structure. Due to the results, the drift rate of this burst is 85.71 MHz s-1, which is considered as a fast drift rate. The burst detected using CALLISTO also being compared to results detected by X-ray GOES data. Both different electromagnetic spectrum shows the exact time. The observations of the burst being discussed in details.
Year
Volume
35
Pages
30-43
Physical description
Contributors
author
  • School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia, hidayahnur153@yahoo.com
author
  • School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
  • Academy of Contemporary Islamic Studies (ACIS), MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
  • School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
  • School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
  • School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
author
  • Institute of Astronomy, Wolfgang-Pauli-Strasse 27, Building HIT, Floor J, CH-8093 Zurich, Switzerland
References
  • [1] Goldman, M.V. and D.F. Smith, Physics of the Sun. Vol. 2. 1986: Dordrecht: Reidel.
  • [2] Hamidi, Z.S., Probability of Solar Flares Turn Out to Form a Coronal Mass Ejections Events Due to the Characterization of Solar Radio Burst Type II and III. International Letters of Chemistry, Physics and Astronomy, 2014. 16.
  • [3] Z.S. Hamidi, N.N.M.S., Z.A. Ibrahim, C. Monstein, W.N.A. Wan Zulkifli, M.B. Ibrahim, N.S. Arifin, N. A. Amran, Magnetic Reconnection of Solar Flare Detected by Solar Radio Burst Type III. Journal of Physics : Conference Series 539 (2014) 012006.
  • [4] White, S.M., Solar Radio Bursts and Space Weather. Asian Journal of Physics, 2007. 16: p. 189-207.
  • [5] N. Gopalswamy1, H.X., P. Mäkelä2, S. Akiyama2, S. Yashiro3, M. L. Kaiser1, and R.A.H.a.J.-L. Bougeret5, Interplanetary shocks lacking type II radio bursts. 2007.
  • [6] N. Gopalswamy, M.R.K., P. K. Manoharan, A. Raoult, and P.Z. N. Nitta, X-Ray And Radio Studies Of A Coronal Eruption: Shock Wave, Plasmoid, and Coronal Mass Ejection. The Astrophysical Journal, 1997
  • [7] E-Aguilar-Rodriguez, N.G., R. MacDowall, S. Yashiro and M.L Kaiser, A Study of Drift Rate Type II Radio Burst At Different Wavelengths. 2005.
  • [8] Z. S. Hamidi, Z.Z.A., Z. A. Ibrahim, N. N. M. Shariff and C. Monstein, Observations of Coronal Mass Ejections (CMEs) at Low Frequency Radio Region on 15th April 2012. 2013.
  • [9] Z. S. Hamidi, N. N. M. Shariff, C. Monstein, Type II Solar Radio Burst with a Split and Herring − Bones During a Minimum Solar Activity. International Letters of Chemistry, Physics and Astronomy, 2014.
  • [10] Gopalswamy, N., et al., Type II radio bursts and energetic solar eruptions. Journal of Geophysical Research, 2005. 110( A12).
  • [11] Hamidi, Z., N. Shariff, and C. Monstein, Type II Solar Radio Burst with a Split and Herring− Bones During a Minimum Solar Activity. International Letters of Chemistry, Physics and Astronomy, 2014. 13(2): p. 104-111.
  • [12] Gopalswamy, N., et al., Relation between type II bursts and CMEs inferred from STEREO observations. Sol. Phys., 2009b. 259: p. 227-254.
  • [13] Hamidi, Z., et al., Theoretical Review of Solar Radio Burst III (SRBT III) Associated With of Solar Flare Phenomena. International Journal Physical Fundamental Sciences, 2013. 3(2): p. 20-23.
  • [14] Hamidi, Z., N. Shariff, and C. Monstein, Fundamental and Second Harmonic Bands of Solar Radio Burst Type II Caused by X1. 8-Class Solar Flares. 2014.
  • [15] Aguilar-Rodriguez, E., et al., A Study of the Drift Rate of Type II Radio Bursts at Different Wavelengths, in Solar Wind 11/SOHO. 2005. p. 393-396.
  • [16] Hamidi, Z., N. Shariff, and C. Monstein, The Tendencies and Timeline of the Solar Burst Type II Fragmented. 2014.
Document Type
article
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bwmeta1.element.psjd-11a3f3b2-9a36-4765-be51-659e05079f44
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