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Home 2016

The Formation of Fundamental Structure of Solar Radio Burst Type II Due X6.9 Class Solar Flare

Author: N. H. Zainol, Z. S. Hamidi , N. N. M. Shariff , Marhana Omar Ali , Nurulhazwani Husien , S. N. U. Sabri , C. Monstein 35 (2016) 30-43

2024-01-05
Reading Time: 3 mins read
0

ABSTRACT
A vigorous solar flare event marked on the spectrometer of the CALLISTO data, being one of
the highest solar flare event that successfully detected. The formation of solar burst type II in meter
region and their associated with X6. 9-class solar flares have been reported. The burst has been
observed at the Blein Obsevatory, Switzerland, which detected by the Compound Astronomical Lowcost Low-frequency Instrument for Spectroscopy and Transportable Observatory (CALLISTO) system
in the range of 170-870 MHz in the two polarizations of left and right circular polarization. It occurred
between 08:01 UT to 08:08 UT within 7 minutes. The Compound Astronomical Low-cost Lowfrequency Instrument for Spectroscopy and Transportable Observatory CALLISTO spectrometer is a
solar dedicated spectrometer system that has been installed all over the world to monitor the Sun
activity in 24 hours. The growth of this burst is often accompanied by abundance enhancement of
particles which may take the form of multiple independent drifting bands or other forms of fine
structure. Due to the results, the drift rate of this burst is 85.71 MHz s-1
, which is considered as a fast
drift rate. The burst detected using CALLISTO also being compared to results detected by X-ray
GOES data. Both different electromagnetic spectrum shows the exact time. The observations of the
burst being discussed in details.

References
[1] Goldman, M.V. and D.F. Smith, Physics of the Sun. Vol. 2. 1986: Dordrecht: Reidel.
[2] 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.
[3] Z.S. Hamidi, N.N.M.S., Z.A. Ibrahim, C. Monstein, W.N.A. Wan Zulkifli, M.B.
Ibrahim, N.S. Arifin, N. A. Amran, Magnetic Reconnection of Solar Flare Detected by
Solar Radio Burst Type III. Journal of Physics : Conference Series 539 (2014) 012006.
[4] White, S.M., Solar Radio Bursts and Space Weather. Asian Journal of Physics, 2007. 16: p. 189-207.
[5] N. Gopalswamy1, H.X., P. Mäkelä2, S. Akiyama2, S. Yashiro3, M. L. Kaiser1, and
R.A.H.a.J.-L. Bougeret5, Interplanetary shocks lacking type II radio bursts. 2007.
[6] N. Gopalswamy, M.R.K., P. K. Manoharan, A. Raoult, and P.Z. N. Nitta, X-Ray And
Radio Studies Of A Coronal Eruption: Shock Wave, Plasmoid, and Coronal Mass
Ejection. The Astrophysical Journal, 1997
[7] E-Aguilar-Rodriguez, N.G., R. MacDowall, S. Yashiro and M.L Kaiser, A Study of Drift
Rate Type II Radio Burst At Different Wavelengths. 2005.
[8] Z. S. Hamidi, Z.Z.A., Z. A. Ibrahim, N. N. M. Shariff and C. Monstein, Observations of
Coronal Mass Ejections (CMEs) at Low Frequency Radio Region on 15th April 2012.
2013.
[9] Z. S. Hamidi1, N. N. M. Shariff2, C. Monstein3, Type II Solar Radio Burst with a Split
and Herring − Bones During a Minimum Solar Activity. International Letters of
Chemistry, Physics and Astronomy, 2014.
[10] Gopalswamy, N., et al., Type II radio bursts and energetic solar eruptions. Journal of
Geophysical Research, 2005. 110( A12).
[11] Hamidi, Z., N. Shariff, and C. Monstein, Type II Solar Radio Burst with a Split and
Herring− Bones During a Minimum Solar Activity. International Letters of Chemistry,
Physics and Astronomy, 2014. 13(2): p. 104-111.
[12] Gopalswamy, N., et al., Relation between type II bursts and CMEs inferred from
STEREO observations. Sol. Phys., 2009b. 259: p. 227-254.
[13] Hamidi, Z., et al., Theoretical Review of Solar Radio Burst III (SRBT III) Associated
With of Solar Flare Phenomena. International Journal Physical Fundamental Sciences,
2013. 3(2): p. 20-23.
[14] Hamidi, Z., N. Shariff, and C. Monstein, Fundamental and Second Harmonic Bands of
Solar Radio Burst Type II Caused by X1. 8-Class Solar Flares. 2014.
[15] Aguilar-Rodriguez, E., et al., A Study of the Drift Rate of Type II Radio Bursts at
Different Wavelengths, in Solar Wind 11/SOHO. 2005. p. 393-396.
[16] Hamidi, Z., N. Shariff, and C. Monstein, The Tendencies and Timeline of the Solar
Burst Type II Fragmented. 2014


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Tags: Coronal Mass Ejections (CMEs)radio regionsolar burstsolar flareSuntype IIX-ray region
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