scholarly journals Solar oscillations

2008 ◽  
Vol 4 (S257) ◽  
pp. 83-93
Author(s):  
H. M. Antia

AbstractStudy of solar oscillations has provided us detailed information about solar structure and dynamics. These in turn provide a test of theories of stellar structure and evolution as well as theories of angular momentum transfer and dynamo. Some of these results about the solar structure and its implication on the recent revision of heavy element abundances are described. Apart from these the solar cycle variations in the rotation rate and its gradients are also discussed.

2020 ◽  
Vol 19 ◽  
pp. 66
Author(s):  
G. I. Karathanou ◽  
V. Tsikoudi ◽  
T. S. Kosmas

In the present work we carry out an extensive study of the solar structure and solar evolution through the use of the TYCHO 6.92 code, which includes a variety of programs and subroutines. In this code we incorporate the most updated microphysical parameters such as screening, recent experimental measurements of the astrophysical factors-S (LUNA), several updated, recently measured, heavy element abundances, etc., and created new models describing crucial phenomena of the solar structure and solar evolution. We used this code to calculate and update nuclear reaction rates, solar neutrino fluxes, solar quantities which characterize the internal solar structure such as temperature, pressure, density, luminosity, heavy element abundances (4He, 12C, 14N, 16O, etc.) as well as sound speed profile and depth of the convection zone.


1988 ◽  
Vol 132 ◽  
pp. 501-506
Author(s):  
C. Sneden ◽  
C. A. Pilachowski ◽  
K. K. Gilroy ◽  
J. J. Cowan

Current observational results for the abundances of the very heavy elements (Z>30) in Population II halo stars are reviewed. New high resolution, low noise spectra of many of these extremely metal-poor stars reveal general consistency in their overall abundance patterns. Below Galactic metallicities of [Fe/H] Ã −2, all of the very heavy elements were manufactured almost exclusively in r-process synthesis events. However, there is considerable star-to-star scatter in the overall level of very heavy element abundances, indicating the influence of local supernovas on element production in the very early, unmixed Galactic halo. The s-process appears to contribute substantially to stellar abundances only in stars more metal-rich than [Fe/H] Ã −2.


1999 ◽  
Vol 511 (2) ◽  
pp. 639-659 ◽  
Author(s):  
Yuri I. Izotov ◽  
Trinh X. Thuan

2021 ◽  
Vol 103 (2) ◽  
Author(s):  
Mara Strungaru ◽  
Matthew O. A. Ellis ◽  
Sergiu Ruta ◽  
Oksana Chubykalo-Fesenko ◽  
Richard F. L. Evans ◽  
...  

2017 ◽  
Vol 8 (1) ◽  
Author(s):  
David H. Brooks ◽  
Deborah Baker ◽  
Lidia van Driel-Gesztelyi ◽  
Harry P. Warren

1981 ◽  
Vol 371 (3) ◽  
pp. 510-532 ◽  
Author(s):  
L.G. Sobotka ◽  
C.C. Hsu ◽  
G.J. Wozniak ◽  
D.J. Morrissey ◽  
L.G. Moretto

Sign in / Sign up

Export Citation Format

Share Document