First Light Detection of a Single Solar Radio Burst Type III due to Solar Flare Event

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

doi:10.18052/www.scipress.com/ILCPA.30.51

ILCPA > ILCPA Volume 30 > First Light Detection of a Single Solar Radio...

< Back to Volume

First Light Detection of a Single Solar Radio Burst Type III due to Solar Flare Event

Full Text PDF

Abstract:

The eruption mechanism of solar flares and type III are currently an extremely active area of research, especially during the solar cycle is towards maximum. In this case, the total energy of solar burst type III is of the order of solar flare with the explosion of the energy can up to 10¹⁵ ergs. The solar flare event is one of the most spectacular explosions that still be on-going study in the solar physics world. This event occurred at 2:000 UT on 15^th April 2012 is due to the explosion of the magnetic energy in from the chromosphere and converted into the heating, mass motion and particle acceleration which can be detected by solar radio burst type III. In this work, we will highlight our first light detection of very tiny solar radio burst type III, which has been observed at the National Space Centre, Banting, Selangor detected by the Compound Low Cost Low Frequency Transportable Observatories (CALLISTO) system at 5:53:23. The region of the data is from 150 − 400 MHz in radio region. This burst is drifted from 150 MHz till 260 MHz. It represents a total energy of 6.2035 × 10^-7 eV − 1.0753 × 10^-6 eV. This fast drift burst is a continuity of the acceleration of the particles which is intermittent, and can be observed since the explosion of the solar flare. Although the burst is very tiny, it is still significant because this burst is the first detection of a single type III burst from our site. Still, the acceleration of the particles can be detected from Earth in the radio region within 3 hours period of observation at the post stage of solar flare.

Info:

Periodical:

International Letters of Chemistry, Physics and Astronomy (Volume 30)

Pages:

51-58

DOI:

https://doi.org/10.18052/www.scipress.com/ILCPA.30.51

Citation:

Z. S. Hamidi et al., "First Light Detection of a Single Solar Radio Burst Type III due to Solar Flare Event", International Letters of Chemistry, Physics and Astronomy, Vol. 30, pp. 51-58, 2014

Online since:

March 2014

Authors:

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

Keywords:

CALLISTO, Low Frequency, Radio Wavelength, Solar Burst, Solar Flare, Type III

Export:

RIS, BibTeX, Text

Distribution:

Open Access

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

References:

D. Herdiwijaya, S. Imelda, Jurnal Matematika dan Sains 11 (2006) 7.

A. O. Benz, Plasma Astrophysics, Springer, Dordrecht, (2002).

M. J. Aschwanden, Güdel M., ApJ 401 (1992) 736-753.

G. D. Fleishman, Gary D. E., Nita G. M., ApJ 593 (2003).

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

M. V. Goldman, D. F. Smith, Physics of the Sun, Dordrecht: Reidel, (1986).

M. Karlický, Kosugi T. , A & A 419 (2004).

D. B. Melrose, Australian J. Phys. 23 (1970) 885-903.

P. A. Sturrock, Phys. Rev. Lett. 16 (1966).

A. O. Benz, C. Monstein, A. H. Meyer, Solar Phys. 226 (2005) 143-151.

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. 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, International Letters of Chemistry, Physics and Astronomy 4 (2014) 29-36.

Z. S. Hamidi, N. N. M. Shariff, Thermal Energy and Power Engineering 3 (2014) 181-184.

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, N. N. M. Shariff, Z. A. Ibrahim, Z. Z. Abidin, Solar Studies in Radio Emission and Optical Photometry, Dimensi Penyelidikan Astronomi Islam, University of Malaya Publisher, University of Malaya, 2013, pp.33-40.

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, 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. S. Hamidi, et al., International Journal of Fundamental Physical Sciences 2 (2012) 4.

A. O. Benz, C. Monstein, H. Meyers, CALLISTO, A New Concept for Solar Radio Spectrometer, Kluwer Academic Publishers, The Netherland, (2004).

Z. S. Hamidi, N. Anim, N. N. M. Shariff, Z. Z. Abidin, Z. A. Ibrahim, C. Monstein, Dynamical structure of solar radio burst type III as evidence of energy of solar flares, in: R. Shukor (Ed. ), PERFIK 2012, American Institute of Physics, Malaysia, 2013, pp.11-15.

Z. S. Hamidi, N. Shariff, Z. Abidin, Z. Ibrahim, C. Monstein, Middle-East Journal of Scientific Research 12 (2012) 6. ( Received 01 March 2014; accepted 06 March 2014 ).

Show More Hide

Cited By:

[1] M. Batubara, T. Manik, R. Suryana, M. Lathif, P. Sitompul, M. Zamzam, F. Mumtahana, "Solar Radio Burst Data Processing of CALLISTO and Frequency Drift Rate Determination of Solar Radio Burst Detected by CALLISTO Network in Indonesia", IOP Conference Series: Materials Science and Engineering, Vol. 180, p. 012049, 2017

DOI: https://doi.org/10.1088/1757-899X/180/1/012049

[2] Z. Hamidi, M. Ali, N. Shariff, C. Monstein, "Electron Density and Drift Rate of Solar Burst Type II during 1^st June 2015", International Letters of Chemistry, Physics and Astronomy, Vol. 63, p. 49, 2016

DOI: https://doi.org/10.18052/www.scipress.com/ILCPA.63.49