The new solar abundances - Part II: the crisis and possible solutions

Details The new solar abundances - Part II: the crisis and possible solutions The new solar abundances - Part II: the crisis and possible solutions

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006coast.147...80m&link_type=abstract

Communications in Asteroseismology, vol. 147, p. 80-84

Computer Science

Sound

13

Scientific paper

Recent 3D, NLTE analysis of the solar spectrum (Asplund et al. 2006, Part I; Asplund et al. 2005) have led to a significant reduction of the CNO and Ne abundances leading to a (Z/X) 30% smaller than the previously recommended value. The corresponding decrease in opacity increases dramatically the discrepancies between the sound-speed derived from helioseismology and our new standard solar models (SSM). We present in this paper some numerical experiments trying to reduce this discrepancy.

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