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2015 | 9 | 59-69
Article title

The Development of Long Series of Quasi-Periodic Pulsation in Active Region AR 2297

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EN
Abstracts
EN
This phenomena allow us to explore about suprathermal electron population that produced by plasma-magnetic field interactions in the solar corona about tens of minutes.The characteristics of the structures of the emission is influenced by wave-particle interaction and wave-wave interaction. The Callisto spectrometer recorded broadband of solar radio burst Type IV from 250-900 MHz. Using data from BLEN7M observatory, we aim to provide inclusive description about the formation and dynamics of solar radio burst type IV due to active region AR2297. About five minutes, the events revealed strong pulsations and “broad patterns” with details of solar radio burst type III with presence of CMEs. AR2297 is the most active region which produced X2-Class solar flares. The speeds of solar wind exceeds 376.0 km/second with 4.0 g/cm3 density of proton in the solar corona. The radio flux shows 121 SFU. Furthermore, there are two active regions, AR2298 and AR2299 also presents in the X2-class solar flares. Active region AR2297 have unstabe ‘Beta-Gamma-Delta’ magnetic fields thet habor energy for M class to X2- class eruptions. As a conclusion, we conclude that Sun activities are more active to achieve maximum cycle at the end 2015. Solar flares on 11th of March 2015 showed long series of quasi-periodic pulsation that deeply modulate a continuum and its drifting toward lower frequency. The corona extends from the top of a narrow transition region to Earth and has a temperature millions of degrees that still mysterious properties.
Year
Volume
9
Pages
59-69
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
  • 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] Z. Hamidi, Z. Abidin, Z. Ibrahim, C. Monstein, N. Shariff, M. Sabaghi, The Beginning Impulsive of Solar Burst Type IV Radio Emission Detection Associated with M Type Solar Flare, International Journal of Fundamental Physical Sciences 2 (2012).
  • [2] Z. Hamidi, N. Shariff, C. Monstein, Disturbances of Solar Eruption From Active Region AR1613, (2014).
  • [3] Z. Hamidi, N. Shariff, Detailed Investigation of a Moving Solar Burst Type IV Radio Emission in on Broadband Frequency, International Letters of Chemistry, Physics and Astronomy 7 (2014) 30-36.
  • [4] G.P. Chernov, A Manifestation of Quasilinear Diffusion in Whistlers in the Fine Structure of Type IV, Solar Radio Bursts Astronomy Reports 40 (1996) 5.
  • [5] Z.S. Hamidi, 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, Scientific Publishing, 2014, pp. 85.
  • [6] H. Aurass, Coronal Physics from Radio and Space Observations, in: I.G. Trottet (Ed.), Lecture Notes in Physics, Springer, Berlin, 1997.
  • [7] A.D. Fokker, Type IV Solar Radio Emission, Space Science Reviews 2 (1963) 70-90.
  • [8] C.W. Young, C.L. Spencer, G.E. Moreton, J.A. and Roberts, Astrophys. J. 133 (1961).
  • [9] Ellis, Australian J.Phys. 22 (1969) 167.
  • [10] D.J. McLean, a.N.R. Labrum, Solar Radiophysics, Cambridge University Press, Cambridge, 1985.
  • [11] Z. Hamidi, N. Shariff, Enormous Eruption of 2.2 X-class Solar Flares on 10 th June 2014, (2014).
  • [12] Z. Hamidi, N. Shariff, C. Monstein, Understanding Climate Changes in Malaysia Through Space Weather Study, International Letters of Natural Sciences (2014).
  • [13] Z. Hamidi, N. Shariff, The Mechanism of Signal Processing of Solar Radio Burst Data in E-CALLISTO Network (Malaysia), International Letters of Chemistry, Physics and Astronomy (2014).
  • [14] Z. Hamidi, N. Shariff, Z. Abidin, Z. Ibrahim, C. Monstein, E-Callisto Collaboration: Some Progress Solar Burst Studies Associated with Solar Flare Research Status in Malaysia, Malaysian Journal of Science and Technology Studies 9 (2013) 15-22.
  • [15] Z.S. Hamidi, N. Shariff, Z. Abidin, Z. Ibrahim, C. Monstein, Coverage of Solar Radio Spectrum in Malaysia and Spectral Overview of Radio Frequency Interference (RFI) by Using CALLISTO Spectrometer from 1MHz to 900 MHz, 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, International Journal of Applied Physics and Mathematics 2 (2011) 3.
  • [17] Z. Hamidi, N. Shariff, C. Monstein, Evaluation of Spectral Overview and Radio Frequency Interference (RFI) Sources at Four Different Sites in CALLISTO Network at the Narrow Band Solar Monitoring Region, (2014).
  • [18] Z.S. Hamidi, N.N.M. Shariff, C. Monstein, Z.A. Ibrahim, Space Weather: The Significance of e-CALLISTO (Malaysia) As One of Contributor of Solar Radio Burst Due To Solar Activity, International Letters of Chemistry, Physics and Astronomy 7 (2014) 37-44.
  • [19] Z.S. Hamidi, N.N.M. Shariff, Z.A. Ibrahim, Z.Z. Abidin, SOLAR STUDIES IN RADIO EMISSION AND OPTICAL PHOTOMETRY, University of Malaya Publisher, 2013.
  • [20] Z.S.Hamidi, Z. Abidin, Z. Ibrahim, N. Shariff, Indication of radio frequency interference (RFI) sources for solar burst monitoring in Malaysia, ICPAP 2011, AIP Publisher, Indonesia, 2012, pp. 6.
  • [21] Z.S. Hamidi, N.N.M. Shariff, C. Monstein, High Time Resolution Observation of Solar Radio of A Group Type III And U Burst Associated of Solar Flares Event, The International Journal of Engineering 1 (2012) 3.
  • [22] Z. Hamidi, N. Shariff, C. Monstein, W.W. Zulkifli, M. Ibrahim, N. Arifin, N. Amran, Observation of the Radio Frequency Interference (RFI) at the National Space Centre, Malaysia, International Letters of Natural Sciences (2014).
  • [23] Z.S. Hamidi, Z.Z. Abidin, Z.A. Ibrahim, N.N.M. 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.
  • [24] R. Umar, Z. Abidin, Z. Ibrahim, N. Gasiprong, K. Asanok, S. Nammahachak, S. Aukkaravittayapun, P. Somboopon, A. Prasit, N. Prasert, The Study of Radio Frequency Interference (RFI) in Altitude Effect on Radio Astronomy In Malaysia And Thailand, Middle East Journal of Scientific Research 14 (2013).
  • [25] Z.S.Hamidi, N.N.M.Shariff, R.Umar, Influence Factors of Radio Frequency Interference (RFI) for Solar Radio Astronomy Purpose at National Space Centre, Malaysia Thailand Journal of Physics 3 (2012) 6.
  • [26] R. Umar, Z.Z. Abidin, Z.A. Ibrahim, M.S.R. Hassan, Z. Rosli, Z.S. Hamidi, Population density effect on radio frequencies interference (RFI) in radio astronomy, AIP Conference Proceedings 1454 (2012) 39.
  • [27] N. Anim, Z. Hamidi, Z. Abidin, C. Monstein, N. Rohizat, Radio frequency interference affecting type III solar burst observations, 2012 NATIONAL PHYSICS CONFERENCE: (PERFIK 2012), American Institute of Physics, 2013, pp. 82-86.
  • [28] Z. Hamidi, N. Shariff, 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 10 (2014) 38-45.
Document Type
article
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YADDA identifier
bwmeta1.element.psjd-ce823a8b-f9a8-4c4e-9d5a-09b71eaf2add
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