科研之友
微信
新浪微博
Facebook
分享链接
摘要
We use recently released solar wind compositional data to determine the metallicity of the Sun-the fraction per unit mass that is composed of elements heavier than He. We focus on a present-day solar sample available to us, which is the least fractionated solar wind from coronal holes near the poles of the Sun. Using these data, we derive a metallicity of Z = 0.0196 +/- 0.0014, which is significantly larger than recent published values based on photospheric spectroscopy, but consistent with results from helioseismology.
- 出版日期2016-1-1
