The quality of present helioseismic data provides the possibility to investigate the microscopic physics of the solar interior. An inversion procedure to reveal the equation of state and chemical composition in the Sun has been developed.
|Number of pages||4|
|Journal||European Space Agency, (Special Publication) ESA SP|
|State||Published - 2004|
|Event||SOHO 14/GONG 2004 Workshop - Helio- and Asteroseismology: Towards a Golden Future - New Haven, CT, United States|
Duration: 12 Jul 2004 → 16 Jul 2004
- Chemical abundance
- Equation of state