Type II Solar Radio Burst with a Split and Herring − Bones during a Minimum Solar Activity

Hamidi, Zety Sharizat; Shariff, N.N.M.; Monstein, C.

doi:10.18052/www.scipress.com/ILCPA.32.104

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Type II Solar Radio Burst with a Split and Herring − Bones during a Minimum Solar Activity

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Abstract:

A preliminary correlation study of the herring − bone type II with a type III solar burst of has been made. On the basis of this study and in combination with the observation in radio emission, an interpretation of the mechanism of the occurrence of this event has been proposed. The type II solar radio burst with a split and herring bone is occurring at the same time from 36 MHz till 50 MHz. We have noted that an individual type III burst also can be observed at 13:23 UT from 45-50 MHz. During that day, a stream of solar wind from a coronal hole on the Sun has disturbing Earth's magnetosphere creating a minor geomagnetic storm, G1 on the NOAA scale of G1-G5. In this case, the solar flare is not very high, but CME is responsible to form a solar radio burst type II. Overall, based on seven days observation beginning from 25th March 2013, the solar activity is considered as very low. The highest solar flare can be observed within 7 days is only a class of B8 flare. There was no CMEs event that directed to the Earth is detected. The geomagnetic field activities are also at minimum level. Although the solar flare event is at a lower stage, it is still possible to form the solar radio burst type II which is associated with CME event. From the selected event, although theoretically solar radio burst type II is associated with CMEs, there is no compelling solar radio burst type II without a flare. The only difference is the dynamic structure and the intensity and speed of both phenomena (solar flares and CMEs) which depend on the active region. Nevertheless, understanding how energy is released in solar ﬂares is one of the central questions in astrophysics. This solar radio burst type II formation is the first event that successfully detected by e-CALLISTO network in 2013.

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Periodical:

International Letters of Chemistry, Physics and Astronomy (Volume 32)

Pages:

104-111

DOI:

https://doi.org/10.18052/www.scipress.com/ILCPA.32.104

Citation:

Z. S. Hamidi et al., "Type II Solar Radio Burst with a Split and Herring − Bones during a Minimum Solar Activity", International Letters of Chemistry, Physics and Astronomy, Vol. 32, pp. 104-111, 2014

Online since:

April 2014

Authors:

Zety Sharizat Hamidi, N.N.M. Shariff, C. Monstein

Keywords:

Burst, e-CALLISTO, Low Frequency, Solar Radio, Sun, Type II

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Creative Commons Attribution 4.0 International License

References:

M.R. Kundu, Solar Radio Astronomy, John Wiley, (1965).

Z. Hamidi, Z. Abidin, Z. Ibrahim, C. Monstein, N. Shariff, M. Sabaghi, International Journal of Fundamental Physical Sciences 2(2) (2012) 29-31.

Z. Hamidi, N. Shariff, C. Monstein, International Letters of Chemistry, Physics and Astronomy 10 (2014) 81-90.

Z. Hamidi, Z. Abidin, Z. Ibrahim, C. Monstein, N. Shariff, International Journal of Fundamental Physical Sciences 2(2) (2012) 21-23.

Z. Hamidi, Z. Abidin, Z. Ibrahim, C. Monstein, N. Shariff, International Journal Physical Fundamental Sciences 2(3) (2012) 32-34.

Z. Hamidia, Z. Abidina, Z. Ibrahima, N. Shariffa, C. Monsteinc, Observations of Coronal Mass Ejections (CMEs) at Low Frequency Radio Region on 15th April 2012, AIP Conf. Proc 1528 (2013) 55-60.

N. Gopalswamy, P. Makela, H. Xie, S. A. Y. Akiyama, S. Yashiro, Journal Geophysical Research: Speace Physics 114(A3) (2009) A00-A22.

N. Gopalswamy, N. Nitta, P.K. Manoharan, A. Raoult, M. Pick, Astronomy and Astrophysics 347 (1999) 684-695.

R. Payne-Scott, D.E. Yabsley, J.G. Bolton, Nature 160 (1947) 256-257.

Boischot A., C. R. Acad. Sci. 244 (1957) 1326.

Z. Hamidi, U.F.S.U. Ibrahim, Z. Abidin, Z. Ibrahim, N. Shariff, International Journal Physical Fundamental Sciences 3 (2013) 20-23.

Z. Hamidi, N. Shariff, F.Z. Ulum, Z. Abidin, Z. Ibrahim, International Journal of Astronomy 1 (2012) 101-104.

Z. Hamidi, N. Shariff, C. Monstein, International Letters of Chemistry, Physics and Astronomy 12 (2014) 84-102.

J. P. Wild, Smerd S. F., Weiss A. A., Solar Burst, Ann. Rev. Astron. Astrophysics 1 (1963) 291-366.

G.A. Dulk, Type III solar radio bursts at long wavelengths, in: R. Stone, E. Weiler, M. Goldstein (Eds. ), Geophys. Monogr., (2000).

T. Takakura, Pub. Astron. Soc. Japan 12 (1960).

A.F. Kuckes, Sudan R. N, Sol. Phys. 17 (1971).

K. Kai, Sol. Phys. 11 (1970).

G. B. L. Gelfreikh, Soviet Astron. 23 (1979).

P. Lantos, Sol. Phys. 22 (1972).

A. Vourlidas, Bastian T. S., Nitta N., Aschwanden M. J., Sol. Phys. 163 (1996).

E. Y. Zlotnik, Soviet Astron. 12 (1968).

V. V. Zheleznyakov, Radio Emission of the Sun and Planets (1970).

Z.S. Hamidi, Z. Ibrahim, Z. Abidin, M. Maulud, N. Radzin, N. Hamzan, N. Anim, N. Shariff, International Journal of Applied Physics and Mathematics 2 (2011) 3.

Z.S. Hamidi, S. Chumiran, A. Mohamad, N. Shariff, Z. Ibrahim, N. Radzin, N. Hamzan, N. Anim, A. Alias, American Journal of Modern Physics 2 (2013) 4.

Z.S. Hamidi, Z. Abidin, Z. Ibrahim, N. Shariff, C. Monstein, International Journal of Engineering Research and Development 3 (2012) 36-39.

Z.S. Hamidi, Z. Abidin, Z. Ibrahim, C. Monstein, N. Shariff, 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, International Journal of Fundamental Physical Sciences 2 (2012) 4.

Z.S. Hamidi, N.N.M. Shariff, 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, The International Journal of Engineering 1 (2012) 3.

Z.S. Hamidi, N. Shariff, Z. Abidin, Z. Ibrahim, C. Monstein, Middle-East Journal of Scientific Research 12 (2012) 6.

Z. S. Hamidi, N. N. M. Shariff, C. Monstein, International Letters of Chemistry, Physics and Astronomy 13(1) (2014) 77-87.

Z. S. Hamidi, N. N. M. Shariff, International Letters of Chemistry, Physics and Astronomy 4 (2014) 29-36.

Z. S. Hamidi, N. N. M. Shariff, International Letters of Chemistry, Physics and Astronomy 5 (2014) 32-42.

Z. S. Hamidi, N. N. M. Shariff, International Letters of Chemistry, Physics and Astronomy 5 (2014) 43-49.

Z. S. Hamidi, N. N. M. Shariff, International Letters of Chemistry, Physics and Astronomy 7 (2014) 21-29.

Z. S. Hamidi, N. N. M. Shariff, International Letters of Chemistry, Physics and Astronomy 7 (2014) 30-36.

Z. S. Hamidi, N. N. M. Shariff, C. Monstein, Z. A. Ibrahim, International Letters of Chemistry, Physics and Astronomy 7 (2014) 37-44.

Z. S. Hamidi, N. N. M. Shariff, C. Monstein, W. N. A. Wan Zulkifli, M. B. Ibrahim, N. S. Arifin, N. A. Amran, International Letters of Chemistry, Physics and Astronomy 8 (2014) 13-19.

Z. S. Hamidi, N. N. M. Shariff, C. Monstein, W. N. A. Wan Zulkifli, M. B. Ibrahim, N. S. Arifin, N. A. Amran, International Letters of Chemistry, Physics and Astronomy 9 (2014) 8-15.

Z. S. Hamidi, N. N. M. Shariff, M. F. Ali, C. Monstein, W. N. A. Wan Zulkifli, M. B. Ibrahim, N. S. Arifin, N. A. Amran, International Letters of Chemistry, Physics and Astronomy 9 (2014) 84-92.

Z. S. Hamidi, N. N. M. Shariff, C. Monstein, International Letters of Chemistry, Physics and Astronomy 11(1) (2014) 51-58.

Z. S. Hamidi, N. N. M. Shariff, C. Monstein, International Letters of Chemistry, Physics and Astronomy 11(2) (2014) 135-145.

Z. S. Hamidi, N. N. M. Shariff, C. Monstein, International Letters of Chemistry, Physics and Astronomy 11(2) (2014) 167-176.

Z. S. Hamidi, C. Monstein, N. N. M. Shariff, International Letters of Chemistry, Physics and Astronomy 11(3) (2014) 243-256. ( Received 05 April 2014; accepted 13 April 2014 ).

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