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Formation of resonance spectral line profiles in stellar wind: Theory and observations
Sapar, L.; Sapar, A.
The theory of the formation of resonance spectral line profiles in the stellar wind of hot stars has been elaborated taking into account the presence of microturbulent motions. In this case the local frequency redistribution in the line profile function is incomplete. This circumstance generates dominating backscattering of photons and drastic cha…
The corona and the solar wind as a manifestation of the solar high speed mass emanation.
Nikolskaya, K. I.; Valchuk, T. E.
A concept of the solar corona and the solar wind resulting from the interaction between the solar primary high speed mass emanation and over-photospheric magnetic fields is outlined and developed. The model arises from the recent view of the solar corona spatial structure and Ulysses solar wind measurement data. The initial solar fast outflow is f…