By Jean-Claude Pecker (auth.), Gabrielle Berthomieu, Michel Cribier (eds.)
'Good print, wealthy illustrations, and lots of 'hot' subject matters are priorities of this ebook, that are steered to all astrophysicists, desiring a superb evaluate during this topic sector. it's very appropriate for the younger scientist who desire an exhaustive advent to present difficulties in sun physics. 'Space technological know-how Reviews58:386 1991
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Extra info for Inside the Sun: Proceedings of the 121st Colloquium of the International Astronomical Union, Held at Versailles, France, May 22–26, 1989
This article is based, with permission of the publisher, on Chapters 1 and 4 of Neutrino Astrophysics by J. N. Bahcall, Cambridge University Press (1989). 1. Introduction The Sun is an astronomical laboratory. Because of its proximity to the Earth, we are able to obtain information about the Sun that is not accessible for other stars. We can determine precise values for the solar mass, radius, geometric shape, photon spectrum, total luminosity, surface chemical composition, and age. In addition, astronomers have measured accurate frequencies for thousands of acoustic oscillation modes that are observed at the solar surface.
P. B. van der Raay, and T. A. B. Kidman (1989) Ap. , 999, 999 R. Davis (1989) These proceedings. -L. R. G. N. (1989) These proceedings. O. M. Bonnet and P. 3. , E. A. Pomerantz (1980) Nature, 288, 541 Grevesse, N. (1984) Physica Scripta, T8, 49. Harari, H. (1989) These proceedings. Hayashi, C. (1961) Pub. Astro. Soc. Japan, 13, 450 Hayashi, C. (1966) Ann. Rev. Astron. , 4, 171 Hirata, K. , et al. (1989) KEK preprint 89-63. F. A. E. M. K. A. (1989) These proceedings. Kirsten, T. (1989) These proceedings.
All three quantities are equal to within the errors of their determinations, which are at least a few percent. 5. Solar neutrinos Is there really a solar neutrino problem? The answer is yes if the difference between the predicted and the measured capture rates exceeds the range of the uncertainties. The answer is no if the uncertainties exceed the discrepancy between theory and observation. The solar neutrino fluxes as well as the uncertainties, calculated from the standard solar model are shown in first row of Table 4.
Inside the Sun: Proceedings of the 121st Colloquium of the International Astronomical Union, Held at Versailles, France, May 22–26, 1989 by Jean-Claude Pecker (auth.), Gabrielle Berthomieu, Michel Cribier (eds.)