... microwave emission of active regions-a fundamental property of active solar corona ... 251-252. V.G.Ledenev. Electron beam propagation in the solar corona. ... V.G. Ledenev. The propagation of electron fluxes in the solar corona. ...
... triggered by emergence of deep-seated magnetic fields and evolve in the solar corona ... provide a powerful tool for studying the corona at the background of the solar disk ...
... upper chromosphere), in soft X-rays (space-borne Yohkoh telescope - upper corona), and in ultraviolet emission (SOHO/EIT - upper chromosphere - lower corona) shows that the observations in these ranges successfully supplement but not duplicate each other ...
... Propagation of electron beams in the solar corona, and generation of radio emission by them - V.G. Ledenev . ... Propagation of MHD shock wves in the inhomogeneous solar corona and in the interplanetary medium, and the accompanying ...
... the solar disk center, which is accounted for by the scattering of radio emission from a compact source in the lower corona ... size of a point source as it is expanding due to the scattering of emission from turbulent irregularities in the corona ...
... Smolkov, A.M. Uralov The manifestation of magnetic fluxes in microvawe emission of the solar corona. ... CESRA Workshop on Energy Conversion and Particle Acceleration in the Solar Corona. 2-6 July 2001. Programme. P. 10. ...
... density fluctuations in the lower solar corona Astronomy Reports, V. 50, p.249-254 ... Long-lived hot coronal structures observed with CORONAS-F/SPIRIT in the Mg XII line ...
... of coronal active regions from the CORONAS-F list of solar flares observed in Gamma ... during the XUV experiment SPIRIT/CORONAS-F. IAU Symposium 223 'Multi-wavelength ...
... of emission in the source region and during its propagation in the corona of the AR ... stationary release of energy in the corona of AR's. NLS brightness temperatures in ...