Solar Burst Type IV Signature Associated with Solar Prominences on 20th January 2016
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Proceeding from close association between solar eruptions, flare and CMEs, we analyze between burst at 980 MHz to 1270 MHz, recorded at the Blein, Switzerland on 20th January 2016. This burst indicates the emission radiation from the Sun from numerous high energy electrons in active region AR2484 and AR2487 forming a large prominence in that particular area. Solar prominences usually occur in loop shape and can last for weeks or months. This event allows us to investigate the electron density and drift rate of solar burst type IV During that time the Sun has the moderate number of sunspots with 55.The radio sources responsibly for IV appear to expand spherically through the solar corona after eject on y solar flare. This event shows a strong radiation in radio region, but not in X-ray region. This burst intense radio phenomena that follow with solar flares. It has a wide band and fine structure. It can be considered as an intermediate fast drift burst (IMDs). This fiber burst has a negative drift rate where the drift is interpreted by the group velocity of the whistler-mode waves. This burst appears is single SRBT III for approximately within 7 minutes with starting time is 8.23 UT. This burst duration is longer compared to the other events. It can be considered as a IV because it begins at the same time as the explosive phase of solar flare. The solar optical, radio and X-ray emission associated with these various energetic particle emissions as well as the propagation characteristics of each particle species are examined in order to study the particle acceleration and emission mechanisms in a solar flare. At the same time, the number of particles traveled a given path in reconnecting area falls exponentially with the increase of this path because of losses owing to a leaving of particles the acceleration volume due to drift.
- School of Physics and Material Sciences, Faculty of Sciences, Universiti Teknologi MARA, 40450, Shah Alam, Selangor, Malaysia, email@example.com
- School of Physics and Material Sciences, Faculty of Sciences, Universiti Teknologi MARA, 0450, Shah Alam, Selangor, Malaysia
- Academy of Contemporary Islamic Studies (ACIS), Universiti Teknologi MARA, 40450, Shah Alam, Selangor, Malaysia
- Institute of Astronomy, Wolfgang-Pauli-Strasse 27, Building HIT, Floor J, CH-8093 Zurich, Switzerland
-  Z. Hamidi, N. Shariff, Z. Ibrahim, C. Monstein, W.W. Zulkifli, M. Ibrahim, N. Arifin, N. Amran, Magnetic Reconnection of Solar Flare Detected by Solar Radio Burst Type III, Journal of Physics: Conference Series, IOP Publishing, 2014, pp. 012006.
-  V.V. Grechnev, An Impulsive Solar Flare Accompanied by a Cusplike Structure in Soft X-Rays, ApJ 566 (2002).
-  D.B. Melrose, A Solar Flare Model Based on Magnetic Reconnection between Current-carrying Loops, ApJ 486 (1994).
-  Z.Z. Abidin, N.M. Anim, Z.S. Hamidi, C. Monstein, Z.A. Ibrahim, R. Umar, N.N.M. Shariff, N. Ramli, N.A.I. Aziz, I. Sukma, Radio frequency interference in solar monitoring using CALLISTO, New Astronomy Reviews 67 (2015) 18-33.
-  X. Sun, J.T. Hoeksema, Y. Liu, T. Wiegelmann, K. Hayashi, Q. Chen, J. Thalmann, Evolution of magnetic field and energy in a major eruptive active region based on SDO/HMI observation, The Astrophysical Journal 748 (2012) 77.
-  N. Ramli, Z. Hamidi, Z. Abidin, S. Shahar, The relation between solar radio burst types II, III and IV due to solar activities, Space Science and Communication (IconSpace), 2015 International Conference on, IEEE, 2015, pp. 123-127.
-  Z. Hamidi, N. Zainol, M. Ali, S. Sabri, N. Shariff, M. Faid, N. Husien, C. Monstein, Signal Detection of the Solar Radio Burst Type III Based on the CALLISTO System Project Management, Industrial Engineering, Management Science and Application (ICIMSA), 2016 International Conference on, IEEE, 2016, pp. 1-4.
-  Z.S. Hamid, N. Shariff, Z. Ibrahim, N. Ramli, Investigation of the statistical properties of solar radio burst type II and III, Space Science and Communication (IconSpace), 2015 International Conference on, IEEE, 2015, pp. 335-338.
-  A. Belov, H. Garcia, V. Kurt, and E. Mavromichalaki Proton events and X-ray flares in the last three solar cycles, Cosmic Res 43 (2005).
-  T.A. Chubb, Creplin, H. Friedman, Observations of Hard X-Ray ESnission from Solar Flares, J. Geophys. Res. 97 (1966).
-  S.M. White, S. Krucker, R.P. Lin, Solar Flare Hard X-ray Emission from the High Corona, Ap. J. Lett 40 (2007).
-  Z. Hamidi, Z. Abidin, Z. Ibrahim, N. Shariff, C. Monstein, N. Ibrahim, R. Abd-Shukor, I.A. Rahman, Z. Ibarahim, C. Yap, Observations of coronal mass ejections (CMEs) at low frequency radio region on 15th April 2012, AIP Conference Proceedings, AIP, 2013, pp. 55-60.
-  M. Zhang, Flyer, N. and Low, B.C., Magnetic Field Confinement in the Corona: The Role of Magnetic Helicity Accumulation, Astrophys. J. 644 (2006) 575-586.
-  I.H. Cairns, P.A. Robinson, N.I. Smith, J. Geophys. Res. 103 (1998).
-  N. Gopalswamy, A. Lara, M.L. Kaiser, J.L. Bougeret, Near-Sun and near-Earth manifestations of solar eruptions, J. Geophys. Res. 106 (2001a) 25261-25278.
-  A.D. Fokker, Type IV Solar Radio Emission, Space Science Reviews 2 (1963) 70-90.
-  Vrsnak B, H. Aurass, J. Magdalenic, N. Gopalswamy, Band-splitting of coronal and interplanetary type II bursts. I. Basic properties Astron. Astrophys. 377 (2001) 321-329.
-  E. Aguilar-Rodriguez, N. Gopalswamy, R.J. MacDowall, S. Yashiro, M.L. Kaiser, A Study of the Drift Rate of Type II Radio Bursts at Different Wavelengths, Solar Wind 11/SOHO, 2005, pp. 393-396.
-  N. Gopalswamy, S. Akiyama, S. Yashiro, Major solar ﬂares without coronal mass ejections, in: N. Gopalswamy, D.F. Webb (Eds.), Universal Heliophysical Processes, 2009a, pp. 283-286.
-  N. Gopalswamy, Energetic Particle and Other Space Weather Events of Solar Cycle 24, (2012).
-  S. Suzuki, G.A. Dulk, Bursts of type III and type V, in: D.J. McLean, N.R. Labrum (Eds.), Solar Radiophysics: Studies of Emission from the Sun at Metre Wavelengths, Cambridge Univ. Press, New York, 1985.
-  T.B. Veronese, R.R. Rosa, M.J.A. Bolzan, F.C. Rocha Fernandes, H.S. Sawant, M. Karlicky, Fluctuation analysis of solar radio bursts associated with geoeffective X-class ﬂares, Journal of Atmospheric and Solar-Terrestrial Physics (2010).
-  S.N.U. Sabri, Z.S. Hamidi, N.N.M. Shariff, C. Monstein, The Significance of e-CALLISTO System and Construction of Log Periodic Dipole Antenna (LPDA) and CALLISTO System for Solar Radio Burst Study, Information Science and Applications (ICISA) 2016, Springer Singapore, 2016, pp. 181-188.
-  Z.S. Hamidi, N.N.M. Shariff, C. Monstein, A. Ibrahim, M. Yusof, The International Cooperation of Solar Radio Burst Project Using e-Callisto System Network, Information Science and Applications (ICISA) 2016, Springer, 2016, pp. 309-317.
-  S. Sabri, N. Zainol, M. Ali, N. Shariff, N. Hussien, M. Faid, Z. Hamidi, C. Monstein, The Dependence of Log Periodic Dipole Antenna (LPDA) and e-CALLISTO Software to Determine the Type of Solar Radio Burst (I-V), Industrial Engineering, Management Science and Application (ICIMSA), 2016 International Conference on, IEEE, 2016, pp. 1-5.
-  N. Zainol, S. Sabri, Z. Hamidi, M. Ali, N. Shariff, N. Husien, C. Monstein, M. Faid, Effective Data Collection and Analysis of Solar Radio Burst Type II Event Using Automated CALLISTO Network System, Industrial Engineering, Management Science and Application (ICIMSA), 2016 International Conference on, IEEE, 2016, pp. 1-5.
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