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The solar interior.

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Title: The solar interior.
Authors: Antia, H. M.1 antia@tifr.res.in
Source: Current Science (00113891). 9/25/2009, Vol. 97 Issue 6, p911-922. 12p. 6 Graphs.
Subjects: Solar interior, Helioseismology, Neutrino astrophysics, Seismic waves, Thermodynamic equilibrium, Solar research
Abstract: The Sun being the nearest star, provides us a unique opportunity to study stellar processes in sufficient detail to test theories of stellar structure and evolution. Although the solar interior is not directly accessible to observations, development of helioseismology during the last three decades has enabled us to study the structure and dynamics of solar interior with unprecedented accuracy. Some of these developments are described in this article. [ABSTRACT FROM AUTHOR]
Copyright of Current Science (00113891) is the property of Indian Academy of Sciences and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
Database: Engineering Source
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DbLabel: Engineering Source
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  Data: <searchLink fieldCode="JN" term="%22Current+Science+%2800113891%29%22">Current Science (00113891)</searchLink>. 9/25/2009, Vol. 97 Issue 6, p911-922. 12p. 6 Graphs.
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  Data: <searchLink fieldCode="DE" term="%22Solar+interior%22">Solar interior</searchLink><br /><searchLink fieldCode="DE" term="%22Helioseismology%22">Helioseismology</searchLink><br /><searchLink fieldCode="DE" term="%22Neutrino+astrophysics%22">Neutrino astrophysics</searchLink><br /><searchLink fieldCode="DE" term="%22Seismic+waves%22">Seismic waves</searchLink><br /><searchLink fieldCode="DE" term="%22Thermodynamic+equilibrium%22">Thermodynamic equilibrium</searchLink><br /><searchLink fieldCode="DE" term="%22Solar+research%22">Solar research</searchLink>
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  Data: The Sun being the nearest star, provides us a unique opportunity to study stellar processes in sufficient detail to test theories of stellar structure and evolution. Although the solar interior is not directly accessible to observations, development of helioseismology during the last three decades has enabled us to study the structure and dynamics of solar interior with unprecedented accuracy. Some of these developments are described in this article. [ABSTRACT FROM AUTHOR]
– Name: AbstractSuppliedCopyright
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  Data: <i>Copyright of Current Science (00113891) is the property of Indian Academy of Sciences and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Text: English
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      – SubjectFull: Solar interior
        Type: general
      – SubjectFull: Helioseismology
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      – SubjectFull: Neutrino astrophysics
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      – SubjectFull: Seismic waves
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              Text: 9/25/2009
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