Published December 11, 1980
| Version v1
Journal article
Is the Sun helium-deficient
- 1. Liege Univ. (Belgium). Inst. d'Astrophysique
- 2. Cambridge Univ. (UK). Dept. of Applied Mathematics and Theoretical Physics
- 3. Cambridge Univ. (UK). Inst. of Astronomy
Description
The recent observations of solar 5-min oscillations of low degree agree approximately with the predictions of a standard solar model with normal abundances of helium and heavy elements. Much of the apparent discrepancy noticed when the observations were first announced was a result of having neglected the influence of the Sun's atmosphere in the normal mode analysis of the theoretical models. The standard solar models discussed here are not in perfect agreement with observation, but it seems that major modifications will not be necessary to remove the remaining small discrepancies. (author)
Additional details
Publishing Information
- Journal Title
- Nature (London)
- Journal Volume
- 288
- Journal Issue
- 5791
- Series
- Nature (London).
- Journal Page Range
- 544-547
- ISSN
- 0028-0836
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 12590354
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- EIGENFREQUENCY; ELEMENT ABUNDANCE; FREQUENCY ANALYSIS; HELIUM; MILLI HZ RANGE; OSCILLATION MODES; OSCILLATIONS; SOLAR ATMOSPHERE; STAR MODELS; SUN; THEORETICAL DATA
- Descriptors DEC
- ATMOSPHERES; DATA; ELEMENTS; FREQUENCY RANGE; HZ RANGE; INFORMATION; MAIN SEQUENCE STARS; MATHEMATICAL MODELS; NONMETALS; NUMERICAL DATA; QUANTITY RATIO; RARE GASES; STARS