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Published September 1968 | Published
Journal Article Open

The O VI emission from the sun

Abstract

The ionization equilibrium of oxygen is calculated for various temperatures. A peculiarity in the dielectronic recombination leads to a considerable fraction of O VI in the corona. Thus, the O VI lines may be emitted from the corona rather than the transition region.

Additional Information

© 1968 Kluwer Academic Publishers. Provided by the NASA Astrophysics Data System. Received 17 March 1968; Published 01 September 1968; Issue Date September 1968. This work was supported by NASA and ONR (HZ) and by NSF and ONR (BZ).

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September 15, 2023
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