An Analysis of Eruption of the Sun Detected by Solar Radio Burst Type I

• Autorzy: Hamidi Z. S. , Shariff N. N. M. , Arifin S. , Monstein C.

Identyfikatory

DOI

10.18052/www.scipress.com/ILCPA.47.139

• Języki publikacji: EN

Abstrakty

EN

Type I solar burst were identified based on data recorded by CALLISTO BLEIN, Switzerland in the period of 17th of January, 2011. Solar Radio Burst Type I is one of the main type of solar burst which is believed to provide a diagnostic of electron acceleration in the corona. This noise storm burst is associated with emerging and growing active regions and last from hours to days. It can be observed that solar radio burst type I is formed within four minutes, although the number of sunspots is just 15. The results of the recent time indicate that Sunspot group 1147 has been mostly quiet since it rounded the eastern limb, but previous week's far side activity shows it is capable of significant eruptions. In 2011, only one day has been detected with spotless day, which means that it is about 7% of overall cases. Probabilities for significant disturbances in Earth's magnetic field are given for three activity levels: active, minor storm, severe storm. From the current conditions in the space weather website on 16th January 2011 that is the first event was shown that the solar wind occurred with a speed of 433.2 km/second while its density about 3.2 protons/cm3. Besides the solar wind, X-ray solar flare with 6 hours maximum: B1 at 1846 UT and 24 hours: B2 at 1544 UT were detected. While type I seem to be an indicator of pre-solar flare and CMEs, on the observational analysis, we could not directly confirmed that this is the only possibility, and we need to consider other processes to explain in detailed the injection, energy loss and the mechanism of the acceleration of the particles. We could conclude one active region will not produce a huge explosion of solar phenomena.

Słowa kluczowe

EN

sun; low frequency; solar radio; burst; type 1; e-CALLISTO

• Wydawca: Przedsiębiorstwo Wydawnictw Naukowych "DARWIN"
• Czasopismo: International Letters of Chemistry, Physics and Astronomy
• Rocznik: 2015
• Tom: Vol. 47
• Strony: 139--146
• Opis fizyczny: Bibliogr. 22 poz., rys., wykr., wz.

Twórcy

autor

Hamidi Z. S.

• School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia

autor

Shariff N. N. M.

• Academy of Contemporary Islamic Studies (ACIS), MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia

autor

Arifin S.

• School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia

autor

Monstein C.

• Institute of Astronomy, Wolfgang-Pauli-Strasse 27, Building HIT, Floor J, CH-8093 Zurich, Switzerland

Bibliografia

• [1] K. Kai, Melrose, D., Suzuki, S., Storms (1985) 415.
• [2] J.M. Maville, Astron. J. 135 (1962).
• [3] S. Krucker, R.P. Lin, Two classes of solar proton events derived from onset time analysis, Astrophys. J. 542 (2000) 61-64.
• [4] D.B. Melrose, Plasma emission due to isotropic fast electrons, and types I, II, and V solar radio bursts, Sol. Phys. 43 (1975) 211–236.
• [5] G. Mann, Coronal Magnetic Energy Releases, Springer, Berlin, 1995.
• [6] M. Karlický, Bárta, J.i.k. M., K., H. Mészárosová, H.S. Sawant, F.C.R. Fernandes, J.R. Cecatto, A&A 375 (2001).
• [7] A. Kruger, Introduction to Solar Radio Astronomy and Radio Physics, D. Reidel, Publ. Co., Dordrecht, Holland, 1979.
• [8] B. Kliem, M. Karlick´y, A.O. Benz, Solar flare radio pulsations as a signature of dynamic magnetic reconnection, Astron. Astrophys. 360 (2000) 715-728.
• [9] N. Gopalswamy, Radio-rich Solar Eruptive Events, Geophys. Res. Lett 27 (2000).
• [10] Z.S.Hamidi, U.F.S.U. Ibrahim, Z.Z. Abidin, Z.A. Ibrahim, N.N.M.Shariff, Theoretical Review of Solar Radio Burst III (SRBT III) Associated With of Solar Flare Phenomena, International Journal of Fundamental Physical Sciences 3 (2013) 20-23.
• [11] Z. Hamidi, N. Shariff, C. Monstein, First Light Detection of A Single Solar Radio Burst Type III Due To Solar Flare Event, (2014).
• [12] 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.
• [13] Z.S. 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, Scientific Publishing, 2014, pp. 85.
• [14] 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) 3.
• [15] Roslan Umar, Zamri Zainal Abidin, Zainol Abidin Ibrahim, Mohd Saiful Rizal Hassan, Zulfazli Rosli, Z.S.Hamidi, Population density effect on radio frequencies interference (RFI) in radio astronomy, ICPAP 2012, AIP Conference Proceedings, Bandung Indonesia, 2012, pp. 4.
• [16] 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) 4.
• [17] 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.
• [18] 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.
• [19] 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) 4.
• [20] 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.
• [21] 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, pp. 6.
• [22] 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.