Abstract
Following previous order of magnitude estimates (Poletto, 1980), the possibility that hot downflowing motions in the solar transition region could be ascribed to spicular matter returning to the chromosphere after being heated by compression, is more thoroughly investigated. The equations describing the one-dimensional non stationary motion of the spicular plasma during the heating process are analytically solved, and the temporal profiles of temperature, density and velocity are given for a set of representative situations. The results are finally compared with available data.
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Poletto, G. Mass motions in the transition region. Sol Phys 73, 233–256 (1981). https://doi.org/10.1007/BF00151680
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DOI: https://doi.org/10.1007/BF00151680