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A study of activity in interacting sunspot groups
Why does the radio activity accompanying the flares in the two large active regions
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A.Ls Academy of Sciences active regions Astron Astronomical Institute Astrophys atomic Bloch wall boundary Bumba chromosphere CMEs component configuration corona Coronagraph coronal loops Crimean Astrophysical Observatory current sheet cycle Czechosl Czechoslovakia density disk distribution electron energy release equation eruption evolution Figure filament flare activity flare loops flux tube footpoints Forbes Gouttebroze H-alpha hard X-ray burst heating height Heinzel HXIS hydrogen impulsive phase intensity Jakimiec km/s large flares limb longitudinal magnetic energy magnetic field magnetic field lines magnetic flux magnetic reconnection maximum Mergentaler motions NLTE modeling Observatory observed Ondfejov parasitic polarity particles photospheric plasma Poland Priest profiles quiescent prominences radio Rompolt rotational velocity separatrix sheared Simnett slab soft X-ray solar activity solar flares Solar Phys solar prominences spectral spectrograph structure sunspot sunspot group surge Svestka sympathetic flares temperature turbulent umbra Wroclaw University X-point X-ray burst X-ray emission X-ray images