Results 71 to 80 of about 42,046 (150)
Cycle 23 Variation in Solar Flare Productivity
The NOAA listings of solar flares in cycles 21-24, including the GOES soft X-ray magnitudes, enable a simple determination of the number of flares each flaring active region produces over its lifetime.
Fletcher, Lyndsay+2 more
core +1 more source
Operational prediction of solar flares using a transformer-based framework. [PDF]
Abduallah Y, Wang JTL, Wang H, Xu Y.
europepmc +1 more source
Characteristics of flight delays during solar flares. [PDF]
Xu XH+17 more
europepmc +1 more source
The probability of SWF occurrence in relation to solar activity [PDF]
Solar terrestrial researches have revealed substantial meaning of nonsteady events on the Sun, mainly solar flares, for the processes taking place in ionosphere.
Morozova, L. P.
core +1 more source
Scaling laws of solar and stellar flares
In this study we compile for the first time comprehensive data sets of solar and stellar flare parameters, including flare peak temperatures T_p, flare peak volume emission measures EM_p, and flare durations t_f from both solar and stellar data, as well ...
Doyle J. G.+9 more
core +1 more source
Driving Influences of the Doppler Flash Observed by SuperDARN HF Radars in Response to Solar Flares. [PDF]
Chakraborty S+5 more
europepmc +1 more source
Abstract : A model is proposed for solar flares, involving a slow build-up of the pre-flare configuration in which gases circulate in the chromosphere and corona. At some stage this configuration becomes unstable and the flash phase of the flare occurs.
Peter A. Sturrock, B. Coppi
openaire +4 more sources
Interplanetary shock waves associated with solar flares [PDF]
The interaction of the earth's magnetic field with the solar wind is discussed with emphasis on the influence of solar flares. The geomagnetic storms are considerered to be the result of the arrival of shock wave generated by solar flares in ...
Chao, J. K., Sakurai, K.
core +1 more source
The correlation between soft and hard X-rays component in flares: from the Sun to the stars
In this work we study the correlation between the soft (1.6--12.4 keV, mostly thermal) and the hard (20--40 and 60--80 keV, mostly non-thermal) X-ray emission in solar flares up to the most energetic events, spanning about 4 orders of magnitude in peak ...
Favata, F.+3 more
core +1 more source
Four New Horsemen of an Apocalypse? Solar Flares, Super-volcanoes, Pandemics, and Artificial Intelligence. [PDF]
Noy I, Uher T.
europepmc +1 more source