ABSTRACT
The complex solar radio burst type III is very related to generation of Coronal Mass Ejections
(CMEs). In a previous study, they deduced that the burst was produced by electron beams accelerated
in blast wave shocks and injected along open magnetic field lines, similar to the herringbone bursts at
metric wavelengths. Usually, if there is another solar flare recorded during complex solar radio burst
type III it should be type II burst. Different for this event, the single solar radio burst recorded occur 8
minutes 30 seconds before the complex solar radio burst type III. The Coronal Mass Ejections also
recorded occurred 7 hours before the single and complex solar radio burst type III. It is noted that
CMEs occurred several hours before this event recorded by the SOHO websites.It is proved that the
production of coronal mass ejection contributed to the production of complex solar radio burst type III.
References
[1] White, S.M., Solar radio bursts and space weather. Asian J. Phys, 2007. 16: p. 189-207.
[2] Reid, H.A.S. and H. Ratcliffe, A review of solar type III radio bursts. Research in
Astronomy and Astrophysics, 2014. 14(7): p. 773.
[3] Vidojevic, S., et al., Statistical Analysis of Langmuir Waves Associated with Type III
Radio Bursts. Publications of the Astronomical Society, 2012. 11: p. 343-349.
[4] Cane, H., et al., Radio evidence for shock acceleration of electrons in the solar corona.
Geophysical Research Letters, 1981. 8(12): p. 1285-1288.
[5] Kundu, M. and R. Stone, Observations of solar radio bursts from meter to kilometer
wavelengths. Advances in Space Research, 1984. 4(7): p. 261-270.
[6] Bougeret, J., et al., A shock associated (SA) radio event and related phenomena
observed from the base of the solar corona to 1 AU. Geophysical research letters, 1998.
25(14): p. 2513-2516.
[7] Reiner, M., et al., Bastille Day event: A radio perspective. Solar Physics, 2001. 204(1-
2): p. 121-137.
[8] Cane, H., W. Erickson, and N. Prestage, Solar flares, type III radio bursts, coronal mass
ejections, and energetic particles. Journal of Geophysical Research: Space Physics
(1978–2012), 2002. 107(A10): p. SSH 14-1-SSH 14-19.
[9] Gopalswamy, N., Type II solar radio bursts. Radio Astronomy at Long Wavelengths,
2000: p. 123-135.
[10] Klassen, A., et al., Solar energetic electron events and coronal shocks. Astronomy &
Astrophysics, 2002. 385(3): p. 1078-1088.
[11] MacDowall, R., et al., Long‐duration hectometric type III radio bursts and their
association with solar energetic particle (SEP) events. Geophysical research letters,
2003. 30(12).
[12] Gopalswamy, N., Interplanetary radio bursts, in Solar and Space Weather
Radiophysics. 2005, Springer. p. 305-333.
[13] Hamidi, Z., et al., An X-ray Observations of A Gradual Coronal Mass Ejections (CMEs)
on 15th April 2012. International Letters of Chemistry, Physics and Astronomy, 2014. 8.
[14] Karlický, M., Cyclic Magnetic Field Reconnection. The Astrophysical Journal Letters,
2009. 692(2): p. L72.
[15] Li, L. and J. Zhang, Observations of the magnetic reconnection signature of an M2 flare
on 2000 March 23. The Astrophysical Journal, 2009. 703(1): p. 877.
[16] Daly, E. Space weather: a brief review. in Solspa 2001, Proceedings of the Second
Solar Cycle and Space Weather Euroconference. 2002.
[17] Birn, J. and E.R. Priest, Reconnection of magnetic fields: magnetohydrodynamics and
collisionless theory and observations. 2007: Cambridge University Press.
[18] Hamidi, Z., et al. Magnetic Reconnection of Solar Flare Detected by Solar Radio Burst
Type III. in Journal of Physics: Conference Series. 2014: IOP Publishing.
[19] Avendaño Valencia, J.D., Scaling Laws for Asymmetric Magnetic Reconnection,
Universidad Nacional de Colombia-Sede Manizales.
[20] Boischot, A., R. Lee, and J. Warwick, Low-Frequency Solar Bursts and Noise Storms.
The Astrophysical Journal, 1960. 131: p. 61.
[21] Gopalswamy, N., Recent advances in the long-wavelength radio physics of the Sun.
Planetary and Space Science, 2004. 52(15): p. 1399-1413.
[22] Nelson, G. and D. Melrose, Type II bursts. Solar Radiophysics: Studies of Emission
from the Sun at Metre Wavelengths, 1985. 1: p. 333-359.
[23] Wild, J., Observations of the spectrum of high-intensity solar radiation at metre
wavelengths. II. Outbursts. Australian Journal of Scientific Research A Physical
Sciences, 1950. 3: p. 399.
[24] McLean, D.J. and N.R. Labrum, Solar radiophysics: Studies of emission from the sun at
metre wavelengths. 1985.
[25] Benz, A.O., C. Monstein, and H. Meyer, CALLISTO–a new concept for solar radio
spectrometers. Solar Physics, 2005. 226(1): p. 143-151.
[26] Zavvari, A., et al., Analysis of radio astronomy bands using CALLISTO spectrometer at
Malaysia-UKM station. Experimental Astronomy, 2015: p. 1-11.
[27] 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.
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