✦ LIBER ✦

The ‘solar model problem’ solved by the abundance of neon in nearby stars

✍ Scribed by Drake, Jeremy J.; Testa, Paola

Book ID: 109894411
Publisher: Nature Publishing Group
Year: 2005
Tongue: English
Weight: 186 KB
Volume: 436
Category: Article
ISSN: 0028-0836
DOI: 10.1038/nature03803

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Is the problem of solar iron abundance s

Is the problem of solar iron abundance solved?

✍ R.I. Kostik; N.G. Shchukina 📂 Article 📅 1995 🏛 Elsevier Science 🌐 English ⚖ 358 KB

Can asteroseismology solve the solar abu

Can asteroseismology solve the solar abundance problem? The test case of HD 43587

✍ A. Mazumdar; L. Singhal; S. Prabhu 📂 Article 📅 2010 🏛 John Wiley and Sons 🌐 English ⚖ 171 KB

The role of abundances in the solar inte

The role of abundances in the solar interior models

✍ S. Turck-Chièze 📂 Article 📅 1995 🏛 Elsevier Science 🌐 English ⚖ 780 KB

Mathematical modelling in the context of

Mathematical modelling in the context of problem solving

✍ Richard D. Noble 📂 Article 📅 1982 🏛 Elsevier Science ⚖ 288 KB

The abundance of3He in the solar wind -

The abundance of3He in the solar wind - A constraint for models of solar evolution

✍ P. Bochsler; J. Geiss; A. Maeder 📂 Article 📅 1990 🏛 Springer 🌐 English ⚖ 724 KB

3He is an intermediate product in the proton-proton chain, and standard models of the Sun predict a large bulge of enhanced 3He abundance near Mr/M o = 0.6 in the contemporary Sun. The relatively low abundance of 3He at the solar surface, which is derived from solar wind observations, poses severe c

Standard solar model uncertainties and t

Standard solar model uncertainties and their correlations in the analysis of the solar neutrino problem

✍ G.L. Fogli; E. Lisi 📂 Article 📅 1995 🏛 Elsevier Science 🌐 English ⚖ 827 KB