Model of Solar Sunspotless Flare
A. V. Borovik, D. Yu. Myachin, A. M. Uralov
We presented the model of sunspotless solar flare on the basis of flare on March 16, 1981. The model allows to explain the main stages of development of flare and observed phenomenon – extended bright chromospheric «streamer» over the polarity reversal line section of a longitudinal magnetic field. We used observational data of the solar chromosphere in the Hα lines from the Baikal Astrophysical Observatory (BAO) and magnetic field data from Kitt Peak Observatory (USA).
solar-terrestrial physics, solar activity, solar flares