Formation and Behavior of the Solar Events Originated in Solar Bursts during the Solar Cycle Maximum Activity

The paper examines the formation and behavior of various solar events originated in solar bursts during the maximum activity of the solar cycle with special emphasis on their peak activity hours and the variation of their time differences. The analysis reveals that out of the fifteen recognized solar events for various time zones the probability of occurrences of each of the type is different. It has been noted that the XRA type is more probable than other types in the morning between 8.00 hr IST and 9 hr IST while at midday FLA and RBR events are more probable supporting that not all kinds of wavelengths are being emitted simultaneously during a solar burst.