CaltechAUTHORS
  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. https://resolver.caltech.edu/CaltechAUTHORS:20200702-125854922

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

182kB

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20200702-125854922

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.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/bf00147119DOIArticle
https://ui.adsabs.harvard.edu/abs/1968SoPh....5...50K/abstractADSArticle
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).
Funders:
Funding AgencyGrant Number
NASAUNSPECIFIED
Office of Naval Research (ONR)UNSPECIFIED
NSFUNSPECIFIED
Subject Keywords:Oxygen; Recombination; Transition Region; Considerable Fraction; Ionization Equilibrium
Issue or Number:1
Record Number:CaltechAUTHORS:20200702-125854922
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200702-125854922
Official Citation:Kozlovsky, B., Zirin, H. The O VI emission from the sun. Sol Phys 5, 50–54 (1968). https://doi.org/10.1007/BF00147119
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:104210
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:02 Jul 2020 20:22
Last Modified:02 Jul 2020 20:22

Repository Staff Only: item control page