Observations of Different Type of Bursts Associated with M 6.3 Solar Flares

• Autorzy: Hamidi Z. S. , Shariff N. N. M.
• Języki publikacji: EN

Abstrakty

EN

Variation of solar bursts due to solar flares such as type an isolated type III , a complex type III, U is being highlighted. These bursts occurred on 9th March 2012 at the National Space Centre, Sg. Lang, Selangor, Malaysia Here, we study a unique case with a combination of two types burst associated with solar flare and CMEs. Our observation is focused on the low frequency region starting from 150 MHz till 400 MHz. We found that a solar flare type solar flare type M 6.3 which occurred in active region AR 1429 starting from 3:32 UT and ending at 05:00 UT. The flare has been confirmed to be the largest flare since 2005. Some physical parameters will be measured. We then compared our results with X-ray data from NOAA Space Weather Prediction Centre (SWPC).

Słowa kluczowe

EN

sun; low frequency; solar radio; burst; type III; type U; e-CALLISTO

• Wydawca: Przedsiębiorstwo Wydawnictw Naukowych "DARWIN"
• Czasopismo: International Letters of Chemistry, Physics and Astronomy
• Rocznik: 2014
• Tom: Vol. 4
• Strony: 29--36
• Opis fizyczny: Bibliogr. 19 poz., ryc.

Twórcy

autor

Hamidi Z. S.

• MARA Universiti of Technology, 40450, Shah Alam, Selangor, Malaysia

autor

Shariff N. N. M.

• Department of Science and Technology Studies, University of Malaya, 50603, Kuala Lumpur, Malaysia

Bibliografia

• [1] S. M. White, Asian Journal of Physics 16 (2007) 189-207.
• [2] V. L. Ginzburg, V. V. Zheleznyakov, On the possible mechanisms of sporadic solar radio emission (radiation in an isotropic plasma), Sov. Astron. 2 (1958).
• [3] W. C. Erickson, J. Geophys. Res. 68 (1963).
• [4] T. A A. Langmuir, Oscillations in ionized gas, Physical Review 33 (1929).
• [5] M. R. Kundu, Solar Radio Astronomy, John Wiley, 1965.
• [6] J. P. Wild, J. Sci. Res 3 (1950a).
• [7] J. P. Wild , Smerd S. F., Weiss A. A., Australian J. Sci. Res 12 (1959) 369.
• [8] N. Gopalswamy, H. Xie, S. Yashiro, I. G., 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.
• [9] A. O. Benz, C. Monstein, A. H. Meyer, Solar Phys. 226 (2005) 143-151.
• [10] Z. 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, (2012).
• [11] M. J. Aschwanden, Güdel M., ApJ 401 (1992).
• [12] H. Aurass, Coronal Physics from Radio and Space Observations, in: I.G. Trottet (Ed.), Lecture Notes in Physics, Springer, Berlin, 1997.
• [13] B. Kliem, M. Karlick´y, A. O. Benz, Astron. Astrophys. 360 (2000) 715-728.
• [14] S. Suzuki, G. A. Dulk, Bursts of type III and type V, in: D. J. McLean, N. R. Labrum (Eds.), Solar Radiophysics: Studies of Emission from the Sun at Metre Wavelengths, Cambridge Univ. Press, New York, 1985.
• [15] Swarup G., et.al, Astrophys. J. 131 (1960) 725.
• [16] A. D. Fokker, Space Science Reviews 2 (1963) 70-90.
• [17] Z. Hamidi, N. Shariff, Z. Abidin, Z. Ibrahim, C. Monstein, Middle-East Journal of Scientific Research 12 (2012) 6.
• [18] Z. Hamidi, Z. Abidin, Z. Ibrahim, C. Monstein, N. Shariff, Signal Detection Performed by Log Periodic Dipole Antenna (LPDA) in Solar Monitoring, (2012).
• [19] Z. 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.