The evolution of the solar composition and possible implications on the study of interplanetary particles

Details The evolution of the solar composition and possible implications on the study of interplanetary particles The evolution of the solar composition and possible implications on the study of interplanetary particles

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh52c02t&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH52C-02 INVITED

Other

7522 Helioseismology, 7599 General Or Miscellaneous

Scientific paper

The predicted evolution of the abundance of the most important elements in the Sun is calculated in precise models taking into account the constraints provided by helioseismology. These theoretical results are then examined in the context of existing abundance measurements in the solar wind mainly, but also in the Sun directly and in other bodies in the solar system. The ultimate goal of such comparisons would be to identify possible correlation between different measurements to help construct a more complete and accurate picture of the evolution of the composition in the Sun itself and in the solar wind. The feasibility of this approach will be discussed.

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