Spectroscopy at the Solar Limb: II. Are Spicules Heated to Coronal Temperatures?
Spicules of the so-called type II were suggested to be relevant for coronal heating because of their ubiquity on the solar surface and their eventual extension into the corona. We investigate whether solar spicules are heated to transition-region or coronal temperatures and reach coronal heights ({≫} 6 Mm) using multiwavelength observations of limb
Beck, C. et al.
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2016