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Exact(31)
There is an 11.7-year periodicity to the overall activity cycle of B. Both stars exhibit stellar flare activity, but the chromosphere of component B is 25% more active than for component A. As a result of differential rotation, the period of rotation varies by latitude from 32 to 47 days, with an average period of 38 days.
Although, the flary active regions show magnetic flux imbalance, it is hard to predict flare activity based on this parameter alone.
This encounter is also likely to enhance Sgr A*'s flare activity across the electromagnetic spectrum.
The flare activity of the southern hemisphere was observed to be more dominant in determining the characteristics of the flare activity in the solar cycle 23.
Solar flare activity stopped cold and weeks and months went by without any sunspots, or areas of intense magnetism.
The rate and depth beneath the surface of the sun at which this process occurs is critical for predicting the sun's magnetic and flare activity, but has remained largely unknown until now.
Similar(29)
These results suggest that the sign-reversal of the helicity injection rate is a key signature of flare activities.
The power grids that serve people around the globe also depend on solar flare activities reported from space.
Our results suggest that the coronae of stars from low to intermediate activity may be explained as the effect of structures similar to those present on the Sun, changing the relative weight of the different kinds of non-flaring coronal regions; the coronae of very active stars may be explained if a continuous flaring activity characterizes these stars.
A flare associated with magnetic cancellation and small pre-flare activity is analyzed.
This allowed us to carefully characterize the X-ray flaring activity of the region immediately around the hole.
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