Constraints on the solar coronal tempera
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Egil Leer; Thomas E. Holzer
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Article
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1979
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Springer
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English
β 698 KB
It is shown that the simultaneous consideration of observed values of the solar wind proton flux density at 1 AU and of the electron pressure at the base of the solar corona leads to relatively strong constraints on the coronal temperature in the region of subsonic solar wind flow. The extreme upper