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2016 | 37 | 1-11
Article title

Geo-effective Disturbances from the “Beta-Gamma-Delta” Magnetic Fields on Active Region AR 2403

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EN
Abstracts
EN
This moving solar radio burst type IV, which lies in between 980 – 1260 MHZ was observed using Compound Astronomical Low-Cost Low- Frequency Instrument for Spectroscopy and Transportable Observatory (CALLISTO) spectrometer and will discussed in detail. CALLISTO system was used and the data were recorded. From BLEN5M’s Radio Flux Density data, it shown that a brief description of the formation of a dynamic formation of solar radio burst type IV due to an active region, AR 2403. This event proved that solar radio burst type IV has a broadband continuum features and has strong pulsations in some range of time. In this event it was took about 8 minutes and it can be high in possibility solar flare and CMEs event followed due to this event. AR 2403 remained active and produced an X- class solar flares and it showed “Beta- Gamma-Delta” magnetic field that gives solar flares which can make geo-effective disturbance to our earth satellite and we have to investigate how plasma – magnetic field in the solar corona which can produce suprathermal electron pulsation about 8 minutes. In this event, it has solar wind speed in 364.8 km/sec and solar wind density in 11.0 protons/cm3.
Year
Volume
37
Pages
1-11
Physical description
Contributors
  • School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
author
  • School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia, zetysh@salam.uitm.edu.my
  • Academy of Contemporary Islamic Studies (ACIS), MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
author
  • Institute of Astronomy, Wolfgang-Pauli-Strasse 27, Building HIT, Floor J, CH-8093 Zurich, Switzerland
author
  • School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
author
  • School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
  • School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia
References
  • [1] Hamidi, Z., C. Monstein, and N. Shariff, Radio Observation of Coronal Mass Ejections (CMEs) Due to Flare Related Phenomenon on 7 th March 2012.
  • [2] Hamidi, Z., et al., The Beginning Impulsive of Solar Burst Type IV Radio Emission Detection Associated with M Type Solar Flare. International Journal of Fundamental Physical Sciences, 2012. 2(2).
  • [3] Z. S. Hamidi, M.B.I., N. N. M. Shariff, C. Monstein, An Analysis of Solar Burst Type II, III, and IV and Determination of a Drift Rate of a Single Type III Solar Burst. International Letters of Chemistry, Physics and Astronomy, 2014: p. 160-170.
  • [4] White, S.M., Solar Radio Bursts and Space Weather. Asian Journal of Physics, 2007. 16: p. 189-207.
  • [5] Hamidi, Z. and N. Shariff, Enormous Eruption of 2.2 X-class Solar Flares on 10 th June 2014. 2014.
  • [6] Hamidi, Z., et al. Dynamical structure of solar radio burst type III as evidence of energy of solar flares. in Persidangan Fizik Kebangsaan (PERFIK) 2012. 2012: Universiti Kebangsaan Malaysia.
  • [7] Fokker, A.D., Type IV Solar Radio Emission. Space Science Reviews, 1963. 2(1): p. 70--90.
  • [8] S. N. U. Sabri, Z.S.H, N. N. M. Shariff, C. Monstein, The Development of Long Series of Quasi-Periodic Pulsation in Active Region AR 2297. 2015.
  • [9] Hamidi, Z. and N. Shariff. Evaluation of signal to noise ratio (SNR) of log periodic dipole antenna (LPDA). in Business Engineering and Industrial Applications Colloquium (BEIAC), 2013 IEEE. 2013: IEEE.
  • [10] Z.S.Hamidi, N.N.M.Shariff, and R.Umar, Influence Factors of Radio Frequency Interference (RFI) for Solar Radio Astronomy Purpose at National Space Centre, Malaysia Thailand Journal of Physics, 2012. 3(2): p. 6.
  • [11] Hamidi, Z., et al., Application of Log Periodic Dipole Antenna (LPDA) in Monitoring Solar Burst at Low Region Frequencies Region. International Journal of Fundamental Physical Sciences, 2012. 2(4).
  • [12] Hamidi, Z., et al., Designing and Constructing Log Periodic Dipole Antenna to Monitor Solar Radio Burst: e-Callisto Space Weather Project. International Journal of Applied Physics and Mathematics, 2012. 2(3): p. 140-142.
  • [13] Z.S. Hamidi, et al., Coverage of Solar Radio Spectrum in Malaysia and Spectral Overview of Radio Frequency Interference (RFI) by Using CALLISTO Spectrometer from 1 MHz to 900 MHz. Middle-East Journal of Scientific Research, 2012. 12(6): p. 6.
Document Type
article
Publication order reference
Identifiers
YADDA identifier
bwmeta1.element.psjd-1930082c-f1a2-4c83-b0d8-d1c46c9af2e6
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