Abstract
Ultraviolet spectrograms and spectroheliograms of the solar chromosphere are
used to test the suggestion (Dere et al. 1986, Rutten & Uitenbroek 1991a) that
bright points observed at h = 1600 Å, chromospheric jets observed in CI lines
near h = 1560 Å, and Ca II K2V bright points are associated with each
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