Abstract
The ionization conditions in coronal loops are investigated in the temperature range 2 × 105–2 × 106K, assuming velocity, density and temperature distributions computed for a siphon model of a pure hydrogen plasma. Use is made of the set of the carbon ions as an example of the general behaviour of the ions characteristic of that temperature range. It is found that the deviation from equilibrium ionization is large for subsonic-supersonic flow if the density is less than 5 × 109cm−-3, with the exception of the lower part of the first leg of very cool loops (T ≈ 2 × 10 K). With this exception cooler loops, given their larger density drop along the axis, show deviations from ionization equilibrium more easily than hotter ones, in spite of their lower flow velocity. We conclude that the possibility of a non-equilibrium state must be taken into account when deducing from measurements of line intensities the temperature of loops in which a flow may occur.
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Now at Institute for Plasma Research, Stanford University, as an E.S.A. Fellow.
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Borrini, G., Noci, G. Non-equilibrium ionization in coronal loops. Sol Phys 77, 153–166 (1982). https://doi.org/10.1007/BF00156101
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DOI: https://doi.org/10.1007/BF00156101