16-18 September 2009, Ponte de Lima, Portugal
The workshop will be centred on the seismic study of convective regions, mixing, ionization zones, rotation, etc., with particular emphasis on how seismic tools for the Sun and for other stars can be combined or adapted in order to improve our capacity to probe the physics of the Sun and stars.
Three Working sessions will be organized. The topics will be: 1) data analysis; 2) seismic probing of stellar rotation; 3) inference on solar / stellar cores and envelopes.
Tuesday, 15th September |
18:30 - 20:30 | | Welcome cocktail (in Porto) |
21:00 | | Bus to Ponte de Lima |
Wednesday, 16th September |
9:00 - 9:10 | | Opening |
9:10 - 9:50 | RV | Open issues in stellar modelling J. Christensen-Dalsgaard |
9:50 - 10:30 | RV | Future challenges for seismic inference on the Sun: views from a naive observer W. Chaplin |
10:30 - 11:00 | | Coffee break |
11:00 - 11:30 | IT | Classical methods for extraction of mode parameters of solar-like pulsators T. Appourchaux |
11:30 - 12:00 | IT | Recent techniques for extraction of mode parameters of solar-like pulsators T. Bedding |
12:00 - 12:30 | IT | Observations and extraction of mode parameters in classical pulsators: lessons from CoRoT E. Michel |
12:30 - 14:30 | | Lunch |
14:30 - 14:45 | OC | On detecting the large separation in the autocorrelation of stellar oscillation times series B. Mosser |
14:45 - 15:00 | OC | Automated Parallel Tempering MCMC: Bayesian Inference Applied to Solar-Type Oscillators T. Campante |
15:00 - 16:30 | | Working session on data analysis Chairs: T. Bedding and B. Chaplin |
16:30 - 17:00 | | Coffee break |
17:00 - 18:00 | | Working session on rotation Chairs: W. Dziembowski and M. Thompson |
Thursday, 17th September |
9:00 - 9:30 | IT | Inference of stellar properties: model grids versus MCMC approach M. Bazot |
9:30 - 10:00 | IT | Seismic signature of Helium ionization in the sun and stars G. Houdek |
10:00 - 10:30 | IT | Signatures of overshooting and rotational mixing in B-type pulsators A. Miglio |
10:30 - 11:00 | | Coffee break |
11:00 - 11:30 | IT | Inference on stellar cores I. Roxburgh |
11:30 - 12:00 | IT | Seismic signatures of stellar magnetic activity W. Dziembowski |
12:00 - 12:15 | OC | New insights on the solar core R. A. Garcia |
12:15 - 12:30 | OC | The relation between delta_nu and nu_max for solar-like oscillations D. Stello |
12:15 - 14:30 | | Lunch |
14:30 - 16:30 | | Working session on cores/envelopes Chairs: M. Cunha and D. Gough |
16:30 - 17:00 | | Coffee break |
17:00 - 17:30 | | Report(s) from working session(s) |
Friday, 18th September |
9:00 - 9:30 | IT | Seismic inferences on stellar rotation (what is required?) M.-J. Goupil |
9:30 - 10:00 | IT | Seismic signatures of rapid rotationD. Reese |
10:00 - 10:30 | IT | Effect of meridional circulation on global solar oscillations M. Roth |
10:30 - 11:00 | | Coffee break |
11:00 - 11:15 | OC | Joint effects of meridional circulation and differential rotation on solar p modes S. Vorontsov |
11:15 - 11:30 | OC | g modes in rapid rotating stars J. Ballot |
11:30 - 12:10 | RV | Final outlook: What bridges may be set between helioseismic and asteroseismic inference? D. O. Gough |
| | Bus to Porto * |
Caption
RV - review contribution
IT - invited contribution
OC - oral contribution
* the exact time will be defined later. When planning your trip back, if you plan to use the conference bus, you should consider the arrival to Porto Airport no earlier than 16h00.