The corona and the solar wind as a manifestation of the solar high speed mass emanation

Autor:	K. I. Nikolskaya, T. E. Valchuk
Rok vydání:	1999
Předmět:	Physics Astrophysics::High Energy Astrophysical Phenomena Coronal hole Astronomy and Astrophysics Coronal loop Solar irradiance Atmospheric sciences Corona Nanoflares Solar cycle Solar wind Physics::Space Physics Coronal mass ejection Astrophysics::Solar and Stellar Astrophysics Astrophysics::Earth and Planetary Astrophysics Instrumentation
Zdroj:	Astronomical & Astrophysical Transactions. 18:279-286
ISSN:	1476-3540 1055-6796
DOI:	10.1080/10556799908203067
Popis:	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 found out to be able to provide the energy and mass transfer from the Sun into the corona and the solar wind. Number density and velocity of the primary plasma outflows are estimated on the basis of the solar wind data and the corona energy balance requirement.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::082156f363445da5784f58a24f963203 https://doi.org/10.1080/10556799908203067 Zobrazit plný text záznamu Plný text ve formátu PDF Plný text ve formátu HTML
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