Magnetic reconnection of solar flare detected by solar radio burst type III

Magnetic reconnection of solar flare detected by solar radio burst type III

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The Sun is an ideal object of a blackbody with a large and complex magnetic field. In solar activity specifically solar flare phenomenon, the magnetic reconnection is one of the most significant factors of the Sun that can simplify a better understanding of our nearest star. This factor is due to th...

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Bibliographic Details
Main Authors: Amran, N.A (Author), Arifin, N.S (Author), Cari (Author), Deta U.A (Author), Hamidi, Z.S (Author), Ibrahim, M.B (Author), Ibrahim, Z.A (Author), Monstein, C. (Author), Shariff, N.N.M (Author), Wan Zulkifli, W.N.A (Author)
Format: Article
Language:English
Published: Institute of Physics Publishing 2014
Subjects:
Kinetic energy
Kinetics
Magnetic fields
Magnetic potential energies
Magnetic reconnections
Magnetism
Magnetoplasma
Potential energy
Radio astronomy
Short time intervals
Solar activity
Solar corona
Solar energy
Solar flare
Solar radiation
Solar radio bursts
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