A Caltech Library Service

The O VI emission from the sun

Kozlovsky, Ben-Zion and Zirin, Harold (1968) The O VI emission from the sun. Solar Physics, 5 (1). pp. 50-54. ISSN 0038-0938. doi:10.1007/bf00147119.

[img] PDF (ADS) - Published Version
See Usage Policy.


Use this Persistent URL to link to this item:


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.

Item Type:Article
Related URLs:
URLURL TypeDescription
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).
Funding AgencyGrant Number
Office of Naval Research (ONR)UNSPECIFIED
Subject Keywords:Oxygen; Recombination; Transition Region; Considerable Fraction; Ionization Equilibrium
Issue or Number:1
Record Number:CaltechAUTHORS:20200702-125854922
Persistent URL:
Official Citation:Kozlovsky, B., Zirin, H. The O VI emission from the sun. Sol Phys 5, 50–54 (1968).
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:104210
Deposited By: Tony Diaz
Deposited On:02 Jul 2020 20:22
Last Modified:16 Nov 2021 18:29

Repository Staff Only: item control page