The research program in helioseismology carried out at the Institute for Theoretical Physics (ITP) at the University of California, Santa Barbara during the six-month interval from January to June 1990 involved 61 scientists of diverse disciplines: theorists, observers and instrumentalists in physics, astrophysics and geophysics. The main topics of research and joint discussion included mode excitation and decay, the internal structure of the sun and its sensitivity to the physics of the equation of state and opacity, seismological inverse procedures, and solar rotation and convection-zone dynamics.
CY - Berlin, Heidelberg DO - 10.1007/3-540-54420-8_46 N2 -The research program in helioseismology carried out at the Institute for Theoretical Physics (ITP) at the University of California, Santa Barbara during the six-month interval from January to June 1990 involved 61 scientists of diverse disciplines: theorists, observers and instrumentalists in physics, astrophysics and geophysics. The main topics of research and joint discussion included mode excitation and decay, the internal structure of the sun and its sensitivity to the physics of the equation of state and opacity, seismological inverse procedures, and solar rotation and convection-zone dynamics.
PB - Springer Berlin Heidelberg PP - Berlin, Heidelberg PY - 1991 SN - 978-3-540-38355-0 SP - 1 EP - 9 TI - Program at ITP: Helioseismology —- Probing the interior of a star ER -