Paper Titles in Periodical
International Letters of Chemistry, Physics and Astronomy
ILCPA Volume 63

Subscribe to our Newsletter and get informed about new publication regulary and special discounts for subscribers!

ILCPA > ILCPA Volume 63 > Electron Density and Drift Rate of Solar Burst...
< Back to Volume

Electron Density and Drift Rate of Solar Burst Type II during 1st June 2015

Full Text PDF


This event allows us to investigate the electron density and drift rate of solar burst type II During 1st June 2015. It is believed that the plasma–magnetic field interactions in the solar corona can produce suprathermal electron populations over periods from tens of minutes to several hours, and the interactions of wave-particle and wave-wave lead to characteristic fine structures of the emission. An intense and broad solar radio burst type II was recorded by CALLISTO spectrometer from 25-80 MHz. Using data from a the Blein observatory, the complex structure of solar burst type III can also be found in the early stage of the formation of type II solar burst type event due to active region AR2358. The drift rate of solar burst type II exceeds 0.03 MHz/s with a density of electron in the solar corona. There are 18 CMEs occurring that day and the distributions of CME speed are between 200 ms-1 to 1100 ms-1 so that the average velocity of the CMEs that occur that day is 1025 m/s. This is one of the largest number of sunspots that have recorded in this year. However, all of these sunspots are quiet and stable and the solar activity remains low. Therefore, it can be observed that only B class of flare from the X-Ray Flux Data.


International Letters of Chemistry, Physics and Astronomy (Volume 63)
Z. S. Hamidi et al., "Electron Density and Drift Rate of Solar Burst Type II during 1st June 2015", International Letters of Chemistry, Physics and Astronomy, Vol. 63, pp. 49-56, 2016
Online since:
January 2016

[1] M. Stix, The sun : an introduction, (2004).

[2] Z. Hamidi, N. Shariff, C. Monstein, Understanding Climate Changes in Malaysia Through Space Weather Study, International Letters of Natural Sciences (2014).

[3] J.P. Wild , Smerd S.F., and Weiss, A.A. , Ann. Rev. Astron. Astrophysicsv 10 (1972).

[4] Z. Hamidi, N. Shariff, C. Monstein, First Light Detection of A Single Solar Radio Burst Type III Due To Solar Flare Event, (2014).

[5] J.G. Andrews, A. D. R, J. Inst. Maths. Applic. 15 (1976).

[6] G.D. Fleishman, Gary, D. E., & Nita, G. M. , ApJ 593 (2003).

[7] A.O. Benz, Sol. Phys. 96 (1985).

[8] H.T. Classen, & Aurass, H., A&A 384 (2002).

[9] A. Shanmugaraju, Y. -J. Moon, K. -S. Cho, M. Dryer, & Umapathy,S. , Sol. Phys. 233 (2006).

[10] H.S. Hudson, & Warmuth, A. , ApJ 614 (2004).

[11] K.S. Cho, Y.J. Moon, M. Dryer, et al. , JGR 110 (2005).

[12] K.S. Cho, J. Lee, Y.J. Moon, et al., A&A 461 (2007).

[13] S. Pohjolainen, & Lehtinen, N.J. , A&A 449 (2006).

[14] M.J. Reiner, Krucker, S., Gary, D.E., et al., ApJ 657 (2007).

[15] B. Vrˇsnak, Warmuth, A., Temmer, M., et al. , A&A 448 (2006).

[16] C. Dauphin, N. Vilmer, S. & Krucker, A&A 455 (2006).

[17] Y. Liu, Luhmann, B. J.G., S.D., R.P. & Lin, ApJ 691 (2009).

[18] D.M. Rust, D.F. and Webb, Soft X-ray observations of large-scale coronal active region brightenings, Solar Phys. 54 (1977) 403–417.

[19] N. Gopalswamy Coronal Mass Ejections and Type II Radio Bursts, in Solar Eruptions and Energetic Particles, Geophysical Monograph Series 165 (2006).

[20] 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.

[21] Vrˇsnak. 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.

[22] 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.

[23] 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.

[24] 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, p.85.

[25] Z. Hamidi, N. Shariff, C. Monstein, The Different Between the Temperature of the Solar Burst at the Feed Point of the Log Periodic Dipole Antenna (LPDA) and the CALLISTO Spectrometer, (2014).

[26] 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).

[27] 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).

[28] Z.S. Hamidi, Z. Abidin, Z. Ibrahim, N. Shariff, C. Monstein, Modification and Performance of Log Periodic Dipole Antenna, International Journal of Engineering Research and Development 3 (2012) 36-39.

Show More Hide
Cited By:
This article has no citations.