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International Letters of Chemistry, Physics and Astronomy
Volume 47

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Determining a Complex Solar Radio Burst Type II on 2<sup>nd</sup> November 2014 Driven by a Hydra Solar Flare as a Blast Waves
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Determining a Complex Solar Radio Burst Type II on 2nd November 2014 Driven by a Hydra Solar Flare as a Blast Waves

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Abstract:

Recent data of a complex solar radio burst type II is analyzed and reviewed. The monitoring of solar radio burst was done by using the Compact Astronomical Low cost, Low frequency Instrument for Spectroscopy and Transportable Observatory (CALLISTO) from BLEIN 7 meter dish telescope at ETH, Zurich in frequency range of 25 until 1000 MHz. During the inspection of the X-ray spectrum, we observed that the C3-category flare was caused by a filament of magnetism, which rose up and erupted between 0400 and 0600 UT. This occurred three hours before the signature of solar radio burst type II. There are some of the material in the filament fell back to the sun, causing a flash of X-rays where it hit the Sun surface. This is a Hydra Flare which occurred without sunspots. On the basis of these results, we suggest that a single shock in the leading edge of the CME could be the source of the multiple type II bursts and support the notion that the CME nose and the CME-streamer interaction are the two main mechanisms able to generate the bursts.

Info:

Periodical:
International Letters of Chemistry, Physics and Astronomy (Volume 47)
Pages:
87-93
DOI:
https://doi.org/10.18052/www.scipress.com/ILCPA.47.87
Citation:
Z. S. Hamidi et al., "Determining a Complex Solar Radio Burst Type II on 2nd November 2014 Driven by a Hydra Solar Flare as a Blast Waves", International Letters of Chemistry, Physics and Astronomy, Vol. 47, pp. 87-93, 2015
Online since:
February 2015
Authors:
Zety Sharizat Hamidi, M.B. Ibrahim, N.N.M. Shariff, C. Monstein
Keywords:
Active Region, Hydra Solar Flare, Radio Region, Solar Burst, Sun, Type II, X-Ray Region
Export:
RIS, BibTeX, Text
Distribution:
Open Access

Creative Commons License
This work is licensed under a
Creative Commons Attribution 4.0 International License

References:

R. Payne-Scott, D.E. Yabsley, J.G. Bolton, Relative Times of Arrival of Bursts of Solar Noise on Different Radio Frequencies, Nature 160 (1947) 256-257.

V.L. Ginzburg, V.V. Zheleznyakov, On the possible mechanisms of sporadic solar radio emission (radiation in an isotropic plasma), Sov. Astron. 2 (1958).

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.

E.W. Cliver, McNamara, L. F., & Gentle, L. C. , AFGL 85 (1985).

Z. 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, International Letters of Chemistry, Physics and Astronomy 16 (2014) 85.

N. Gopalswamy, N. Nitta, P.K. Manoharan, A. Raoult, M. Pick, X-ray and radio manifestations of a solar eruptive event, Astronomy and Astrophysics 347 (1999) 684695.

N. Gopalswamy, H. Xie, S. Yashiro, I.G. and Usoskin, Coronal mass ejections and ground level enhancements, in: B. e. a. Sripathi Acharya (Ed. ), 29th International Cosmic Ray Conference, Pune, India, 2005, pp.169-172.

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) 1522.

Z.S. Hamidi, N.N.M. Shariff, Evaluation of Signal to Noise Ratio (SNR) of Log Periodic Dipole Antenna (LPDA) Business Engineering and Industrial Applications Colloquium 2013, IEEE, Langkawi, Malaysia, 2013, pp.434-438.

Z. Hamidi, N. Shariff, Determination of Flux Density of the Solar Radio Burst Event by Using Log Periodic Dipole Antenna (LPDA), International Letters of Chemistry, Physics and Astronomy 7 (2014) 21-29.

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).

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).

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).

Z.S. Hamidi, S. Chumiran, A. Mohamad, N. Shariff, Z. Ibrahim, N. Radzin, N. Hamzan, N. Anim, A. Alias, Effective temperature of the sun based on log periodic dipole antenna performance in the range from 45 Mhz to 870 Mhz, American Journal of Modern Physics 2 (2013).

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.

Z.S. Hamidi, Z. Abidin, Z. Ibrahim, C. Monstein, N. Shariff, Signal Detection Performed by Log Periodic Dipole Antenna (LPDA) in Solar Monitoring, International Journal of Fundamental Physical Sciences 2 (2012) 32-34.

Z.S. Hamidi, N.M. Anim, N. N.S. Hakimi, N. Hamzan, A. Mokhtar, N. Syukri, S. Rohizat, I. Sukma, Z.A. Ibrahim, Z.Z. Abidin, N.N.M. Shariff, C. Monstein, Application of Log Periodic Dipole Antenna (LPDA) in Monitoring Solar Burst at Low Region Frequencies Region International Journal of Fundamental Physical Sciences 2 (2012).

Z.S. Hamidi, N.N.M. Shariff, Determination of Isotropic Source Spectral Power of the Log Periodic Dipole Antenna (LPDA), International Journal of Science and Mathematics 2 (2014) 3.

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, p.6.

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.

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.

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.

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.

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).

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.

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