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The 3B/X3 solar flare of 27 February 1992The 3B/X3 solar flare of 27 February 1992
(Instituto de Geofísica, 2012)
Fast Mid-IR Flashes Detected During Small Solar X-Ray Bursts
(SpringerDordrechtHolanda, 2010)
Predicting Extreme Solar Flare Events Using Lu and Hamilton Avalanche Model
(Springer, 2020-11)
Solar flares are the most powerful events in the solar atmosphere, releasing a huge amount of energy in a few minutes. Any progress in predicting when a flare of a big magnitude will occur is extremely important to evaluate ...
Effects of high-energy astrophysical events on habitable planets
(CAMBRIDGE UNIV PRESSNEW YORK, 2012)
With the possible exception of meteor impacts, high-energy astrophysical events such as supernovae, gamma-ray bursts (GRB) and flares are usually not taken into account for biological and evolutionary studies due to their ...
Equatorial ionospheric electrodynamics during solar flares
(American Geophysical Union, 2017-05-09)
Previous investigations on ionospheric responses to solar flares focused mainly on the photoionization caused by the increased X‐rays and extreme ultraviolet irradiance. However, little attention was paid to the related ...
Observed flux density enhancement at submillimeter wavelengths during an X-class flare
(Elsevier Sci LtdOxfordInglaterra, 2007)
X-type interactions of the loops in the flare of 25 September 1997 - Part II
(EDP Sciences, 2001-06)
The interaction of magnetic structures and the conversion of magnetic free energy into heating of the plasma and acceleration of particles are commonly accepted as the origin of solar flares. The 3-dimensional (3D) structure ...