Abstract
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.
| Original language | English |
|---|---|
| Pages (from-to) | 400-403 |
| Number of pages | 4 |
| Journal | European Space Agency, (Special Publication) ESA SP |
| Issue number | 559 |
| 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 |
Keywords
- Chemical abundance
- Equation of state
- Helioseismology