PL EN


Preferences help
enabled [disable] Abstract
Number of results
2016 | 40 | 188-198
Article title

The Development of the X2-Class of flares with Presence of Type IV burst and Single Type III burst in Low Frequency (20-85 MHz) on 5th May 2015

Content
Title variants
Languages of publication
EN
Abstracts
EN
The plasma-magnetic field interaction in the solar corona is caused exploration of suprathermal electron population have been made to study about the phenomena solar radio burst. This burst only took about approximately 2 minutes to produce X2- class of solar flares which occurred at 22:10 UT till 22:11UT. The wave-wave interaction and wave-particle interaction influenced the characteristic structures of the emission. The CALLISTO spectrometer has been used to detect and record the Type IV and Type III occurred during 22:07UT till 22:11 UT and it only took about 3.30 minutes to occur. The range of frequency of this burst 20-85 MHz and data is from ROSWELL-NM observatory. With the presence of the data, we aim to determine the causes of the Solar Radio Burst Type IV produced Type III burst in several minutes and describe briefly about the formation and dynamics of solar radio burst type IV occurred on active region, AR2335 which also produced beta-gamma magnetic field. This event showed the strong pulsation and a broadband pattern with details about Type IV burst, then Type III burst present in fast drift. AR 2335 is the most active region and produced X2-class of solar flares which has solar wind speed about 361.6km/second and proton density about 4.3 protons/cm3 in the solar corona. AR 2335 harbor energy for X2-class from 6-H to 24-H observation on X-Ray solar flares have been recorded. The data showed that it has a strong energy electrons presence during the burst occurred in the active region and this class of solar flares are more powerful which has potential to cause radio blackout and long lasting space weather storms. As the conclusion, the sun activity showed on 5th May 2015 has quasi-periodic pulsation that has continuum and drift in lower frequency. The temperature that corona took to extend from the top of a narrow transition region still be as mysterious properties.
Year
Volume
40
Pages
188-198
Physical description
Contributors
  • School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
author
  • School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia, zetysh@salam.uitm.edu.my
author
  • Academy of Contemporary Islamic Studies (ACIS), MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
  • Academy of Contemporary Islamic Studies (ACIS), MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
  • Academy of Contemporary Islamic Studies (ACIS), MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
  • Academy of Contemporary Islamic Studies (ACIS), 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] Hamidi, Z.S., et al., Magnetic Reconnection of Solar Flare Detected by Solar Radio Burst Type III. Journal of Physics: Conference Series, 2014. 539: p. 012006.
  • [2] Ling, W.D.C., Magnetic Fine Structures in the Solar Corona and Their Heating by Kinetic Alfvén Waves. 2011. 25.
  • [3] Z. S. Hamidi, S.N.U.S., N. N. M. Shariff, C. Monstein, The Evolution of Unstable 'Beta-Gamma' Magnetic Fields of Active Region AR 2222. 2015. 48: p. 95-102.
  • [4] Ramli, N., et al. The relation between solar radio burst types II, III and IV due to solar activities. in Space Science and Communication (IconSpace), 2015 International Conference on. 2015. IEEE.
  • [5] Hamidi, Z.S., N.N.M. Shariff, and C. Monstein3, Disturbances of Solar Eruption From Active Region AR1613. 2014: p. 77-87.
  • [6] White, S.M., Solar Radio Bursts and Space Weather. Asian Journal of Physics, 2007. 16: p. 189-207.
  • [7] S. N. U. Sabri, Z.S.H. Hamidi, N. N. M. Shariff, C. Monstein, The Development of Long Series of Quasi-Periodic Pulsation in Active Region AR 2297. 2015: p. 70-80.
  • [8] Z. S. Hamidi, N. N. M. Shariff, Enormous Eruption of 2.2 X-class Solar Flares on10th June 2014. 2014: p. 249- 257.
  • [9] Z. S. Hamidi, N.N.M. Sharif, The Mechanism of Signal Processing of Solar Radio Burst Data in E-CALLISTO Network (Malaysia). (2014).
  • [10] Hamidi, Z., et al., Designing and Constructing Log Periodic Dipole Antenna to Monitor Solar Radio Burst: e-Callisto Space Weather Project. 2nd International Conference on Applied Physics and Mathematics, AICIT Press, 2011: p. 1-4.
  • [11] Z. S. Hamidi, N. N. M. Shariff, Detailed Investigation of a Moving Solar Burst Type IV Radio Emission in on Broadband Frequency. 2014: p. 30-36.
  • [12] Hamidi, Z.S., et al., Indication of radio frequency interference (RFI) sources for solar burst monitoring in Malaysia. 2012: p. 43-46.
  • [13] Hamidi, Z.S., et al., Observation of the Radio Frequency Interference (RFI) at the National Space Centre, Malaysia. 2014.
  • [14] Hamidi, Z.S., N.N.M. Shariff, and C. Monstein, High Time Resolution Observation of Solar Radio of A Group Type III And U Burst Associated of Solar Flares Event. 2012: p. 101-103.
  • [15] R. Umar, Z.Z.A., Z.A. Ibrahim, N. Gasiprong, K. Asanok, S. Nammahachak, P.S. S. Aukkaravittayapun, A. Prasit, N. Prasert, Z.S. Hamidi, and N.H.a.U.F.S.U. Ibrahim, The Study of Radio Frequency Interference (RFI) in Altitude Effect on Radio Astronomy in Malaysia and Thailand. 2013.
  • [16] Z.S.Hamidi, Abidin, Z.Z, Ibrahim, Z.A., N.N.M.Shariff , R.Umar, Influence Factors of Radio Frequency Interference (RFI) for Solar Radio Astronomy Purpose at National Space Centre, Malaysia. 2012.
  • [17] Umar, R., et al., Population density effect on radio frequencies interference (RFI) in radio astronomy, ICPAP 2012. AIP Conference Proceedings, Bandung Indonesia, 2012: p. 4.
  • [18] Anim, N., et al., Radio frequency interference affecting type III solar burst observations. 2012 National Physics Conference:(PERFIK 2012), American Institute of Physics, 2013: p. 82-86.
  • [19] Hamidi, Z., N. Shariff, and C. Monstein, Comparison of the Radio Frequency Interference (RFI) in the Region of Solar Burst Type III Data At Selected CALLISTO Network. International Letters of Chemistry, Physics and Astronomy, 2014. 10.
Document Type
article
Publication order reference
Identifiers
YADDA identifier
bwmeta1.element.psjd-365585e4-213a-49cf-9666-4f8c97112d23
JavaScript is turned off in your web browser. Turn it on to take full advantage of this site, then refresh the page.