Published August 1976
| Version v1
Journal article
The solar hafnium abundance
Creators
- 1. Aarhus Univ. (Denmark). Inst. of Physics
- 2. Institute of Theoretical Astrophysics, Oslo (Norway)
Description
The solar Hf abundance is determined using nine Hf II lines in the photospheric spectrum. The transition probabilities were obtained from lifetime measurements performed by the beam-foil technique. The abundance derived from synthetic spectrum calculations is A(Hf)=0.88 +- 0.08 in the logarithmic A(H)=12.00 scale. (Auth.)
Additional details
Identifiers
- DOI
- 10.1007/bf00162445;
Publishing Information
- Journal Title
- Solar Physics
- Journal Volume
- 49
- Journal Issue
- 2
- Series
- Sol. Phys.
- Journal Page Range
- 211-215
- ISSN
- 0038-0938
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 8314153
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ELEMENT ABUNDANCE; EMISSION SPECTRA; ENERGY-LEVEL TRANSITIONS; HAFNIUM; HAFNIUM IONS; LIFETIME; PHOTOSPHERE; PROBABILITY; SUN; ULTRAVIOLET RADIATION
- Descriptors DEC
- ATOMIC IONS; CHARGED PARTICLES; ELECTROMAGNETIC RADIATION; ELEMENTS; IONS; METALS; QUANTITY RATIO; RADIATIONS; SPECTRA; STARS; TRANSITION ELEMENTS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent