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