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 On 16th March 2016 the solar radio burst type II is recorded to appear on spectrograph after the type ...
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 The LPDA antenna because it is very suitable and economic amount the types of antennas. It consists of an ...
ABSTRACT Statistical properties of solar radio burst radio type II and III of this work will be highlighted. One of ...
References Hamidi, Z.S., et al., Magnetic Reconnection of Solar Flare Detected by Solar Radio Burst Type III. Journal of Physics: ...
ABSTRACT During solar activity the energy particles of the sun released due to solar flare, Coronal Mass Ejections (CMEs), coronal ...
ABSTRACT This moving solar radio burst type IV, which lies in between 980 – 1260 MHZ was observed using Compound ...
ABSTRACT The complex solar radio burst type III is very related to generation of Coronal Mass Ejections (CMEs). In a ...
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