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Abstract list

Talks that were not selected for an oral presentation are de facto poster

Poster : format is 1.8 m tall by 1.2 m wide
Talk : you will have the choice of using the PC / Mac of the conference center using regular PowerPoint or pdf presentation, or using your own PC / Mac. If you use the PC / Mac of the conference center, you will be provided with a remote control of your presentation.

Please come see Stephane Caminade before the start of your session for checking the technical details. Try to see Stephane the day before, or during coffee breaks, or at opening of the congress center. Please also make sure to hand over to Stephane your presentation in electronic format for making it available later on the web site.

Allen Walter An Introduction to Wave Trapping in Supergranulation
Arlt Rainer An attempt to determine the differential rotation in the 18th century
Augustson Kyle Modeling the Near-Surface Shear Layer Trhough Coupled Simulations of Surface and Deep Convection
Ayukov Sergey Low-Z solar model: sound speed profile under the convection zone
Baldner Charles The thermal structure of sunspots from ring diagram analysis
Baldner Charles High frequency power in HMI ring diagrams
Basu Sarbani Are recent solar heavy element abundances consistent with helioseismology?
Basu Sarbani Characteristics of solar meridional flows
Basu Sarbani Zonal flows throughout cycle 23
Baturin Vladimir Adiabatic exponent in isentropic convective zone: a heavy elements abundance and seismic inversion
Belkacem Kevin Amplitudes of solar p modes: a refined modeling of the eddy-time correlation function
Berdyugina Svetlana Local Asteroseismology: A new approach to old puzzles
Birch Aaron Local Helioseismology
Bogart Richard HMI Ring-Diagram Analysis. I. First Results
Bogart Richard HMI Ring-Diagram Analysis. II. The Processing Pipeline and Data Products
Braun Douglas Properties of Near-surface Flows around Active Regions from Helioseismic Holography
Braun Douglas The Need for Physics-based Inversions of Sunspot Structure and Flows
Broomhall Anne-Marie Are short-term variations in solar oscillation frequencies the signature of a second dynamo?
Burrows Keiran Velocity flows inside NOA AR 10720 derived by ring diagram analysis from SOHO/MDI dopplergrams
Burtseva Olga Temporal variations of high-degree solar acoustic modes from GONG and MDI
Bush Rock The HMI Observing Program to Study the Evolution of the Sun's Shape
Cally Paul Seismic Probing of Sunspot Umbrae
Cally Paul How to turn Gravity Waves into Alfvén Waves and other such Tricks
Chakraborty Sudeepto A first look at solar meridional circulation with HMI
Chakraborty Sudeepto Is there a correlation between high-frequency global oscillations and solar flares?
Chatterjee Piyali What do global p-modes tell us about large scale solar flows?
Creevey Orlagh Probing the parameter space of HD49933
Demarque Pierre Evolutionary Scenarios and Chemical Inhomogeneities of Extended Horizontal Branch Stars
Doerr Hans-Peter The Meridional flow as derived from Fourier-Legendre decomposition of the first data from the Helioseismic and Magnetic Imager
Dombroski Daniel TESTING AND RECOMMENDATIONS FOR USING THE SPARC CODE FOR IMPROVED SOLAR SIMULATIONS
Donea Alina Stochastic Seismic Emission from Acoustic Glories in New Active Regions of cycle 24
duvall thomas Time-Distance Helioseismology with the HMI instrument
Felipe Tobías Magneto-acoustic waves in sunspots from observations and numerical simulations
Fleck Bernhard On the origin of high-frequency “acoustic” power in photospheric and chromospheric velocity power spectra
Garcia Rafael A. Detection of individual dipole g modes in the Sun
Garcia Rafael A. The acoustic low-degree eigenfrequencies of the Sun measured with 14 years of continuous GOLF velocity measurements
gaulme patrick Mode identification with Kepler Data
Giersch Owen Automated Region Detection and Sunspot Analysis using GONG Imagery
Gonzalez Hernandez Irene Meridional Flow Observations: Implications for the current Flux Transport Models
Gonzalez Hernandez Irene Towards a global solar magnetic index
Gonzalez-Morales Pedro A. Helioseismic tests with the FLASH simulation code
Gorshkov Alexey Diffusion segregation of heavy elements in the Sun
GREC GERARD Low frequency signal in the GOLF measurements
Grundahl Frank SONG - Stellar Observations Network Group
Haber Deborah The Influence of Tracking Rate on Helioseismic Flow Inferences
Hill Frank GONG Program Status
Hindman Bradley 3D Helioseismic Inversions of Ring-Analysis Flow Measurements
Hoeksema J. Todd Initial Magnetic Field Observations from HMI
Howe Rachel The torsional oscillation and the new solar cycle
Howe Rachel Low-degree helioseismology with AIA
Howe Rachel Comparison of HMI Dopplergrams with GONG and MDI Data
Howe Rachel Low-degree helioseismology with AIA
Howe Rachel Ring-diagram frequency comparisons for GONG, MDI and HMI
Howe Rachel Rotation-rate variations at the tachocline: an update
Howe Rachel Global Rotation Inversions of HMI Data
Ilonidis Stathis Searching Subsurface Signatures of Emerging Active Regions
Jain Rekha Axisymmetric Absorption of p Modes by Thin Magnetic Flux Tubes
Jain Kiran Testing the GONG ring-diagram pipeline with HMI Dopplergrams
Jain Kiran Towards Near Real Time High-resolution Dopplergrams from GONG
Jimenez Mancebo Antonio The acoustic cutoff frequency of the Sun and the solar cycle.
Kholikov Shukirjon Time-Distance Analysis of GONG Global Mode Time Series.
Khomenko Elena Numerical simulations of the conversion to Alfven waves in solar active regions
Kitiashvili Irina Subsurface structure of the Evershed flows in sunspots
Komm Rudi Subsurface Flows of Emerging and Decaying Active Regions
Komm Rudi A Search for Coherent Structures in Subsurface Flows
Komm Rudi Solar flares and temporal changes in subsurface vorticity measurements
Komm Rudi Solar cycle variation of zonal and meridional flow
Korzennik Sylvain The Solar Core as Never Seen Before
Korzennik Sylvain The Rotation Rate and its Evolution Derived from Improved Mode Fitting and Inversion Methodology
Korzennik Sylvain Accurate Mapping of the Torsional Oscillations: a Trade-Off Study between Time Resolution and Mode Characterization Precision
Kosovichev Alexander Local helioseismology of sunspot regions: comparison of ring-diagram and time-distance results.
Kuhn Jeff Solar Diameter, Irradiance, and Solar Activity
Kumar Brajesh Analysis of peculiar penumbral flows in the NOAA active region 10930 during a major solar flare
Larson Timothy HMI Global Helioseismology Data Analysis Pipeline
Larson Timothy Improving Leakage Matrix Calculation
Leibacher John Meridional flow measurements from 15 years of GONG spherical harmonic time series.
Liang Zhi-Chao Finite-wavelength scattering of high-degree modes by a sunspot
Mathis stephane Angular momentum transport by internal gravity waves in rotating magnetic solar-type stars
Mathur Savita Unveiling stellar magnetic activity using CoRoT seismic observations
Maurya Ram Ajor Kinetic and Magnetic Helicities of Flare Productive and Dormant Active Regions
McManus Sean GONG Data Management and Analysis Center Status and Future Directions
Moradi Hamed Helioseismology of Sunspots: An Extended Analysis of AR 9787
Mullan Dermott Radial profile of changes in wave speed between solar min and max
Nutto Christian Numerical simulations of magneto-acoustic wave propagation from the upper convection zone into the chromosphere
Parchevsky Konstantin Numerical simulation of interaction of MHD waves with magnetostatic models of sunspots
Pinter Balazs Torsional motion of sunspots
Rabello-Soares M. Cristina Frequency dependence of the solar-cycle frequency variation
Reiter Johann Temporal changes in the frequencies, widths, amplitudes, and asymmetries of the solar p-mode oscillations
Richardson Matthew Solar Flares: A Driving Mechanism of High-Frequency Solar Acoustic Waves
Roth Markus Moat Flow around AR9787
Roth Markus p-modes in Sunrise/IMAX data
Roxburgh Ian Rapidly rotating stars in shellular rotation
Roxburgh Ian Phase shift analysis of solar-like oscillators
Salabert David Mode visibility and m-amplitude ratio in velocity and intensity helioseismic measurements
Salabert David Global p-mode oscillations throughout the complete solar cycle 23
Salabert David Variation in the frequency separations with activity and impact on stellar parameter determination
Schad Ariane Observations of oscillation coupling ratios and the meridional flow
Schou Jesper From MDI to HMI
Schunker Hannah Semi-empirical sunspot models and helioseismology
Schunker Hannah Recently discovered properties of acoustic power
Staiger Joachim Groundbased Multiline Spectroscopy for the Investigation of Solar Atmospheric Waves
Svanda Michal Validation of linear inversions for 3D vector flows using numerical simulation
Tanner Joel Convection in the Superadiabatic Layer of Stars
Thompson Michael Asteroseismic results for the evolved solar-type star KIC 11026764 (Gemma)
Toomre Juri Assessing the deep interior dyamics and magnetism of A-type stars
Trampedach Regner A New Solar Convection Simulation - Does the Abundance Problem Persist?
Tripathy Sushanta Variation of High-Degree Mode Frequencies During the Declining Phase of Solar Cycle 23
Tripathy Sushanta Angular-degree dependence of p mode frequencies during the solar cycle 23
TURCK-CHIEZE Sylvaine News from opacity calculations in solar radiative zone and in stellar enveloppes
TURCK-CHIEZE Sylvaine Impact of activity and rotation on the sound speed and diameter of the Sun
TURCK-CHIEZE Sylvaine The dynamics of the solar-like stars radiative zone
vauclair Sylvie new stellar modelling including radiative acceleration on elements and thermohaline convection
Vorontsov Sergei Coupling of solar p-modes of high degree l by joint effects of differential rotation and meridional circulation
Williams Peter Comparisons of Supergranule Characteristics During the Solar Minima of Cycles 22/23 and 23/24
Zhao Junwei HMI Time-Distance Pipeline: First Results
Zhao Junwei HMI Time-Distance Pipeline: An Overview and Data Products

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