Detailed Investigation of a Moving Solar Burst Type IV Radio Emission in on Broadband Frequency

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

doi:10.18052/www.scipress.com/ILCPA.26.30

ILCPA > Volume 26 > Detailed Investigation of a Moving Solar Burst...

< Back to Volume

Detailed Investigation of a Moving Solar Burst Type IV Radio Emission in on Broadband Frequency

Full Text PDF

Abstract:

The moving type IV burst component of the solar radio region from 260-380 MHz observed using the CALLISTO spectrometer is discussed in detail. We used the Compound Astronomical Low Cost Low Frequency Spectrometer Transportable Observatory (CALLISTO) system connected to the Log Periodic Dipole Antenna (LPDA) at the National Space Centre, Selangor located (3.0833333°N 101.5333333°E) on 22nd February 2012. It is found that a strong burst that caused by extraordinary solar flares are due to magnetic reconnection effect potentially induced in the near-Earth magneto tail. From our observation the indication of signal potentially drives Coronal Mass Ejections (CMEs). We also compare our results with the Geostationary Operational Environmental Satellites (GOES) data. From our analysis, one possible reason behind the formation of this very complex long duration of this loop is the magnetic reconnection and disruption of the loops which is observed during flare maximum. The Active Region, AR 1429 active region was a site of several intense in several days. From the results, it showed that the burst is formed from the explosion of M-class solar flare which can be observed at 412UT. As a conclusion, a good agreement was reached and we believe that Sun’s activities are more active to pursuit the solar maximum cycle.

Info:

Periodical:

International Letters of Chemistry, Physics and Astronomy (Volume 26)

Pages:

30-36

DOI:

https://doi.org/10.18052/www.scipress.com/ILCPA.26.30

Citation:

Z. S. Hamidi and N.N.M. Shariff, "Detailed Investigation of a Moving Solar Burst Type IV Radio Emission in on Broadband Frequency", International Letters of Chemistry, Physics and Astronomy, Vol. 26, pp. 30-36, 2014

Online since:

January 2014

Authors:

Zety Sharizat Hamidi, N.N.M. Shariff

Keywords:

Active Region 1429, e-CALLISTO, Solar Burst Type IV, Solar Flare, Solar Radio Emission

Export:

RIS, BibTeX, Text

Distribution:

Open Access

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

References:

[1] S. M. White, Asian Journal of Physics 16 (2007).

[2] T. S. Bastian, Benz A. O., Gary D. E., Annu. Rev. Astron. Astrophys. 36 (1998).

[3] M. Aschwanden, Physics of the Solar Corona, Praxis Publication, Chichester, UK, (2004).

[4] M.R. Kundu, Haddock F. T., Trans. I. R. E., PGAP, AP 82 (1961).

[5] A. Kruger, Introduction to Solar Radio Astronomy and Radio Physics, Reidel, Dordrecht, (1979).

[6] C. Slottje, Atlas of fine structure of dynamic spectra of solar type IV-dm and some type II radio bursts, (1981).

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

[8] 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 (2012) 3.

DOI: https://doi.org/10.7763/ijapm.2012.v2.70

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

[10] Z. S. Hamidi, N. N. M. Shariff, R. Umar, Malaysia Thailand Journal of Physics 3 (2012) 6.

[11] Z. S. Hamidi, Z. Abidin, Z. Ibrahim, C. Monstein, N. Shariff, International Journal of Fundamental Physical Sciences 2 (2012) 32-34.

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

[13] Z. S. Hamidi, N. N. M. Shariff, Evaluation of Signal to Noise Ratio (SNR) of Log Periodic Dipole Antenna (LPDA) BEIAC 2013, IEEE, Langkawi, Malaysia, 2013, p.6.

DOI: https://doi.org/10.1109/beiac.2013.6560164

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

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

[16] Z. S. Hamidi, N. N. M. Shariff, International Letters of Chemistry, Physics and Astronomy 5 (2014) 43-49. ( Received 13 January 2014; accepted 18 January 2014 ).

Show More Hide

Cited By:

[1] N. Ansor, Z. Hamidi, N. Shariff, "Characterization of type III and IV solar radio bursts from e-CALLISTO", Journal of Physics: Conference Series, Vol. 1349, p. 012063, 2019

DOI: https://doi.org/10.1088/1742-6596/1349/1/012063