On spicules and the stability analysis of the minimum flux corona theory |
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| Authors: | W Van Tend |
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| Institution: | (1) The Astronomical Institute at Utrecht, Sterrewacht, Zonnenburg 2, Utrecht, The Netherlands |
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| Abstract: | It is shown that the stability analysis of coronae envisaged by Hearn (1975, 1979) does not lead to a unique stable configuration. The chromosphere-corona transition region is inevitably non-steady. Spicules are a manifestation of this. It is suggested that a point to point analysis of energy losses and gains, rather than a stability analysis, can determine the coronal parameters. |
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