Results 231 to 240 of about 1,712,646 (286)
Origin and Evolution of the Galilean Satellites Within the Jovian System. [PDF]
Space Sci RevNimmo F +10 more
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Light hydrogen isotopes in terrestrial core. [PDF]
Sci AdvZhang Y, Wang W, Deng Z, Wu Z, Chen B.
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Physics Reports, 1993
Abstract This report confronts the different aspects of the solar interior from the experimental and theoretical points of view, discussing photospheric abundances, neutrinos and acoustic mode measurements. The theoretical approach mainly concerns the classical framework of stellar evolution, nevertheless, particle interpretation of the data and ...
D Vignaud +2 more
exaly +2 more sources
Abstract This report confronts the different aspects of the solar interior from the experimental and theoretical points of view, discussing photospheric abundances, neutrinos and acoustic mode measurements. The theoretical approach mainly concerns the classical framework of stellar evolution, nevertheless, particle interpretation of the data and ...
D Vignaud +2 more
exaly +2 more sources
AIP Conference Proceedings, 2007
The equations of stellar structure and evolution need to be solved to model the interior of the Sun. Modelling the Sun is, however, slightly more complicated than modelling other stars since we have more observational constraints for the Sun than for other stars. In this article we discuss the basics of modelling the interior structure of the Sun.
Sarbani Basu
exaly +2 more sources
The equations of stellar structure and evolution need to be solved to model the interior of the Sun. Modelling the Sun is, however, slightly more complicated than modelling other stars since we have more observational constraints for the Sun than for other stars. In this article we discuss the basics of modelling the interior structure of the Sun.
Sarbani Basu
exaly +2 more sources
Thermonuclear Reactions in the Solar Interior
1986The probable role of thermonuclear reactions in the solar interior had already begun to be recognized as early as the 1920s by astrophysicists such as Eddington (1926). This recognition was based not on any direct observation of these reactions but instead was arrived at more on the basis of default.
exaly +2 more sources
2001
The quest to learn the internal structure and dynamics of the Sun is motivated by several issues. For most people the most obvious is the desire to understand the source of energy for the Earth, which is essential for the maintenance of life. Astronomers are interested in the Sun because it is an example of a typical main-sequence star that can be ...
Douglas O. Gough, Philip H. Scherrer
openaire +1 more source
The quest to learn the internal structure and dynamics of the Sun is motivated by several issues. For most people the most obvious is the desire to understand the source of energy for the Earth, which is essential for the maintenance of life. Astronomers are interested in the Sun because it is an example of a typical main-sequence star that can be ...
Douglas O. Gough, Philip H. Scherrer
openaire +1 more source
Solar neutrinos and nuclear reactions in the solar interior
2018We discuss the results of Homestake and Kamioka experiments, showing that - if the results of these experiments are taken at their face values - one way to save "conventional neutrinos" is to look for a nuclear solution decreasing both 7Be and 8B neutrino fluxes with respect to the predictions of the standard solar models.
Castellani V +2 more
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Rapid Rotation of the Solar Interior
Science, 1967A model proposed for the sun apparently can account for the maintenance of photospheric rotation against deceleration by the solar wind. The rotational period is about half a day near the top of the radiative mass, and 1.6 times shorter at the center.
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Present problems of the solar interior
Solar Physics, 1985The standard model of solar evolution is reviewed and a number of problems highlighted. A fundamental question is whether there is any mixing of matter in the central regions, since such mixing could radically alter the model of the present Sun and modify our understanding of the evolution of other stars.
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