FLOW SOURCES AND FORMATION LAWS OF SOLAR WIND STREAMS
作者： N.A. Lotova , V.N. Obridko , K.V. Vladimirskii , M.K. Bird , P. Janardhan
关键词: Corona 、 Meteorology 、 Interplanetary magnetic field 、 Sunspot 、 Solar observatory 、 Physics 、 Atmospheric sciences 、 Coronal mass ejection 、 Solar cycle 、 Magnetopause 、 Solar irradiance
摘要: The large-scale stream structure of the solar wind flow is studied in main acceleration zone from 10 to 40 radii Sun. Three independent sets experimental data were used: radio astronomical observations wave scattering using large telescopes Lebedev Physical Institute; dual-frequency Doppler speed measurements Ulysses Solar Corona Experiment during spacecraft's two conjunctions summer 1991 and winter 1995; magnetic field strength configuration computed Wilcox Observatory data. Both on position transonic region estimates used as parameters reflecting intensity process. Correlation studies these with corona revealed several types differing their velocities location primary region.
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