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Abstracts |
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The discovery of new pulsators from the CoRoT exoplanet database and their potential for massive star asteroseismology |
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Conny Aerts, Jonas Debosscher and Pieter Degroote |
The quest for solar g modes |
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Thierry Appourchaux |
Solar like oscillations after 1 year 1/2 observations with CoRoT |
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Mariejo GOUPIL, Thierry Appourchaux, Annie Baglin, Eric Michel, Reza Samadi, and the Corot team |
PLATO: PLAnetary Transits and Oscillations of stars |
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Torben Arentoft |
Solar-like oscillations in Procyon A |
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Torben Arentoft On behalf of the team |
Instabilities in the magnetic tachocline |
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Rainer Arlt |
The solar butterfly diagram in the 18th century |
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Rainer Arlt |
Time-Distance envelope widths - what can they tell us? |
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J. D. Armstrong |
Solar cycle related changes at the base of the convection zone |
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Charles Baldner and Sarbani Basu |
The evolution of the sub-surface structure of long-lived active regions |
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Charles Baldner, Rick Bogart, Sarbani Basu and H. M. Antia |
Changing magnetic fields in the solar convection zone |
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Charles Baldner, H.M. Antia, Sarbani Basu and T.P. Larson |
SIAMOIS: an asteroseismic network with 1 single site in Antactica |
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Benoit Mosser and Caroline Barban |
The solar metallicity problem: Do we have the solution? |
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Sarbani Basu |
What is new with zonal flows? |
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H. M. Antia, Sarbani Basu and S. M. Chitre |
Travel Time Errors Due to Data Gaps |
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John Beck, Tom Duvall and Junwei Zhao |
Simulations of Wave Propagation: Simple Models for the Frequency Dependence of Helioseismic Travel-Time Shifts |
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Aaron Birch, Doug Braun, Shravan Hanasoge and Robert Cameron |
Local Helioseismology Data Products From the HMI Analysis Pipeline |
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Richard Bogart, Arthur Amezcua, Philip Scherrer, Karen Tian and Junwei Zhao |
Turbulence simulations showing mean-field dynamos |
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Axel Brandenburg |
Prospects for the Detection of the Deep Solar Meridional Circulation |
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Doug Braun and Aaron Birch |
AN INVESTIGATION OF SOLAR MAGNETIC INDICES FOR SPACE WEATHER FORECASTING |
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Alan Brockman |
The inhomogeneous response across the solar disc of unresolved Doppler velocity observations |
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Anne-Marie Broomhall, William J. Chaplin, Yvonne Elsworth and Roger New |
Are p-mode frequencies predictable from one solar cycle to the next? |
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Anne-Marie Broomhall, William J Chaplin, Yvonne Elsworth, Brek A. Miller, Roger New and Graham Verner |
Dynamo Action and Wreathes of Magnetism in a Younger Sun |
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Benjamin Brown |
German Data Center for the Solar Dynamics Observatory |
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Raymond Burston, Laurent Gizon, Yacine Saidi and Sami Solanki |
Effect of surface activity on amplitudes of high-degree solar p-modes |
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Olga Burtseva, Sushant Tripathy, Frank Hill and Shukur Kholikov |
Influence of magnetic activity on lifetime of high-l solar p-modes |
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Olga Burtseva, Frank Hill and Shukur Kholikov |
Seismology and the Dynamo: History and Prospects |
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Paul Cally |
Time-Distance Modeling In A Simulated Sunspot Atmosphere |
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Hamed Moradi and Paul Cally |
Modeling the seismic signature of sunspots
Robert Cameron Max Planck Institute for Solar System Research
Laurent Gizon Max Planck Institute for Solar System Research
Hannah Schunker Max Planck Institute for Solar System Research
We have used the SLiM code to model the seismic signature of sunspots. In this talk we shall discuss the comparison between the simulations and the cross-covariance of the wavefield obtained from MDI/SOHO observations of an isolated sunspot in 2002. Various f- and p-mode wavepackets are used to infer some properties of the observed sunspot. |