
doi: 10.1007/bf00151949
Spectral scans of the wavelength regions around 3039 A and 3269 A were used as a basis for the determination of the solar abundance of germanium. A solar model similar to the one given by Elste (1968) was used in the analysis of the data. The germanium abundance values obtained are presented in a table. Taking into account an abundance compilation for the solar system conducted by Cameron (1973), it is concluded that the 'solar system' and solar atmospheric abundances of germanium are in accord.
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 7 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Top 10% | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
