| |
Abstracts |
|
The discovery of new pulsators from the CoRoT exoplanet database and their potential for massive star asteroseismology |
|
Conny Aerts, Jonas Debosscher and Pieter Degroote |
The quest for solar g modes |
|
Thierry Appourchaux |
Solar like oscillations after 1 year 1/2 observations with CoRoT |
|
Mariejo GOUPIL, Thierry Appourchaux, Annie Baglin, Eric Michel, Reza Samadi, and the Corot team |
PLATO: PLAnetary Transits and Oscillations of stars |
|
Torben Arentoft |
Solar-like oscillations in Procyon A |
|
Torben Arentoft On behalf of the team |
Instabilities in the magnetic tachocline |
|
Rainer Arlt |
The solar butterfly diagram in the 18th century |
|
Rainer Arlt |
Time-Distance envelope widths - what can they tell us? |
|
J. D. Armstrong |
Solar cycle related changes at the base of the convection zone |
|
Charles Baldner and Sarbani Basu |
The evolution of the sub-surface structure of long-lived active regions |
|
Charles Baldner, Rick Bogart, Sarbani Basu and H. M. Antia |
Changing magnetic fields in the solar convection zone |
|
Charles Baldner, H.M. Antia, Sarbani Basu and T.P. Larson |
SIAMOIS: an asteroseismic network with 1 single site in Antactica |
|
Benoit Mosser and Caroline Barban |
The solar metallicity problem: Do we have the solution? |
|
Sarbani Basu |
What is new with zonal flows? |
|
H. M. Antia, Sarbani Basu and S. M. Chitre |
Travel Time Errors Due to Data Gaps |
|
John Beck, Tom Duvall and Junwei Zhao |
Simulations of Wave Propagation: Simple Models for the Frequency Dependence of Helioseismic Travel-Time Shifts |
|
Aaron Birch, Doug Braun, Shravan Hanasoge and Robert Cameron |
Local Helioseismology Data Products From the HMI Analysis Pipeline |
|
Richard Bogart, Arthur Amezcua, Philip Scherrer, Karen Tian and Junwei Zhao |
Turbulence simulations showing mean-field dynamos |
|
Axel Brandenburg |
Prospects for the Detection of the Deep Solar Meridional Circulation |
|
Doug Braun and Aaron Birch |
AN INVESTIGATION OF SOLAR MAGNETIC INDICES FOR SPACE WEATHER FORECASTING |
|
Alan Brockman |
The inhomogeneous response across the solar disc of unresolved Doppler velocity observations |
|
Anne-Marie Broomhall, William J. Chaplin, Yvonne Elsworth and Roger New |
Are p-mode frequencies predictable from one solar cycle to the next? |
|
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 |
|
Benjamin Brown |
German Data Center for the Solar Dynamics Observatory |
|
Raymond Burston, Laurent Gizon, Yacine Saidi and Sami Solanki |
Effect of surface activity on amplitudes of high-degree solar p-modes |
|
Olga Burtseva, Sushant Tripathy, Frank Hill and Shukur Kholikov |
Influence of magnetic activity on lifetime of high-l solar p-modes |
|
Olga Burtseva, Frank Hill and Shukur Kholikov |
Seismology and the Dynamo: History and Prospects |
|
Paul Cally |
Time-Distance Modeling In A Simulated Sunspot Atmosphere |
|
Hamed Moradi and Paul Cally |
Modeling the seismic signature of sunspots |
|
Robert Cameron and Hannah Schunker |
A new method to probe the interaction between solar acoustic waves and magnetic regions |
|
Dean-Yi Chou |
SONG |
|
Jørgen Christensen-Dalsgaard |
Asteroseismic mass and radius of Kepler stars |
|
Orlagh L. Creevey |
Testing the potential and limitations of seismic stellar systems |
|
Orlagh L. Creevey |
Sensitivity of p-modes for determining the microscopic diffusion coefficient at the base of the convection zone |
|
Orlagh L. Creevey, Savita Mathur and Rafael A. Garcia |
The interaction of solar oscillations with magnetic fields |
|
Ashley Crouch |
Axisymmetric instabilities in solar/stellar tachocline |
|
Mausumi Dikpati, Paul Cally, Peter Gilman and Mark Miesch |
Measuring merdional circulation in the Sun |
|
Thomas Duvall and Shravan Hanasoge |
BiSON update |
|
John Allison, Ian Barnes, Anne-Marie Broomhall, William J. Chaplin, Guy Davies, Yvonne Elsworth, Stephen T. Fletcher, Steven Hale, Barry Jackson, Brek A. Miller and Roger New |
Modeling the subsurface evolution of emerging active region flux tubes |
|
Yuhong Fan |
The generation of more realistic BiSON-like artificial helioseismic data |
|
Stephen Fletcher, Anne-Marie Broomhall, William Chaplin, Yvonne Elsworth and Roger New |
Efficient pseudo-global peak-bagging for helioseismic data |
|
Stephen Fletcher, William Chaplin, Yvonne Elsworth and Roger New |
Spatial Cross Spectrum: reducing the incoherent convective background of resolved helioseismic instruments |
|
Rafael A. Garcia, Savita Mathur, Irene Gonzalez Hernandez, Antonio Jimenez |
On the solar origin of the 220.7 signal |
|
Antonio Jimenez and Rafael Garcia |
GOLF: Analysis of the low frequency spectrum and comparison with a calculated solar g-mode spectrum |
|
Gerard Grec, Janine Provost and Catherine Renaud |
Turbulent magnetic pumping in Babcock-Leighton dynamos |
|
Gustavo Guerrero and Elisabete de Gouveia Dal Pino |
Exploring uncertainties in solar model physics and predictions arising from the new abundances |
|
Joyce Guzik, Alexander Friedland, L.S. Watson, Andrew Reindel and David Kilcrease |
Flows Derived from New Multi-Ridge Ring Analyses |
|
Deborah Haber and Bradley Hindman |
A new tool for forecasting the solar UV/EUV irradiance |
|
Margit Haberreiter, Juan Fontenla, Irene Gonzalez-Hernandez, Charles Lindsey and Eric Quemérais |
Signatures of emerging subsurface structures in acoustic power maps |
|
Thomas Hartlep and Alexander Kosovichev |
The advection of supergranules by large-scale flows |
|
David Hathaway, Peter Williams and Manfred Cuntz |
Improving the prediction capability of the helioseismic far-side maps |
|
Irene Gonzalez Hernandez, Philip Scherrer, Charles Lindsey, Doug Braun, Frank Hill |
Meridional circulation in the declining phase of solar cycle 23 |
|
Irene Gonzalez Hernandez, Shukur Kholikov, Frank Hill, Rachel Howe, Rudolph Komm |
A different approach to calculate the far-side seismic migration Green's functions |
|
Fernando Perez Hernandez and Irene Gonzalez Hernandez |
Connection among data from GONG, SOHO/MDI and HMI |
|
Frank Hill |
Solar Subsurface Flows |
|
Bradley Hindman |
Ring diagram analysis of 96x96x20 Mm artificial data set |
|
Rachel Howe, Irene Gonzalez Hernandez, Rudi Komm and Frank Hill |
The torsional oscillation and the solar cycle: is it minimum yet?
Rachel Howe, National Solar Observatory
Frank Hill, National Solar Observatory
Rudi Komm, National Solar Observatory
Timothy P. Larson, Stanford University
Jesper Schou, Stanford University
Michael J. Thompson, University of Sheffield
Roger Ulrich, UCLA
The torsional oscillation pattern of migrating zonal flows is related to the solar activity cycle. In the approach to solar minimum, we compare the current flow profile with that seen at the previous minimum, using GONG and MDI data as well as Mount Wilson Doppler observations that reach further back in time. Will the flow patter at the upcoming minimum match that for the previous one? |