A Note On Heat Transfer In The Upper Chromosphere And Corona
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Dynamics of the solar atmosphere: Spicules and fibrils - UNH
by AC Sterling 1988 The flow of coronal heat down Into the upper chromosphere is Beckers (1972) notes that spicules near the solar poles seem to follow the polar (coronal)
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by RG Athay 1964 Cited by 7 corona. The great brilliance of the photosphere obscures the chromosphere Spicules in the upper and middle chromosphere, as observed in the Ha line of
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the upper chromosphere is much hotter, there must be a temperature minimum are assumed then losses due to radiation and heat conduction can be