Heart-shape Active Region 2529 Producing Strong M6.7 class Solar Flare and Gradual Coronal Mass Ejections
ABSTRACT The Centre of the Sun is very important to be study because this layer is where the nuclear ...
ABSTRACT The Centre of the Sun is very important to be study because this layer is where the nuclear ...
ABSTRACT Proceeding from close association between solar eruptions, flare and CMEs, we analyze between burst at 980 MHz to 1270 ...
ABSTRACT The relativistic energy electron emission is found to occur only during proton events. Solar prominences usually occur in loop ...
ABSTRACT Statistical properties of solar radio burst radio type II and III of this work will be highlighted. One of ...
ABSTRACT The solar flares are generated from electromagnetic radiation which is sudden oscillation of the stored energy in the magnetic ...
References Hamidi, Z.S., et al., Magnetic Reconnection of Solar Flare Detected by Solar Radio Burst Type III. Journal of Physics: ...
ABSTRACT This moving solar radio burst type IV, which lies in between 980 – 1260 MHZ was observed using Compound ...
ABSTRACT The study of comparison between cosmic rays, sunspot and solar flare has been carried out and done with the ...
ABSTRACT A vigorous solar flare event marked on the spectrometer of the CALLISTO data, being one of the highest solar ...
ABSTRACT During 13th of May 2015, the solar wind is very high velocity, which is 733 kms-1as compared to 367.5 ...
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