Poster presentations for this Symposium have been grouped according the
relevant conference sessions. The Abstract Codes are the
original 4-digit abstract submission number and the IAU Abstract Booklet Number
(prefixed by S239-).
| | Author | Title | Abstract Codes |
|---|
| Session A: Modelling Convection and Radiative Transfer |
| PT A1 | O. Kochukhov et al. | 3-D Hydrodynamic Simulation of Convection in A Stars | 0245 | 41 |
| PT A2 | L. Sbordone et al. | ATLAS 9 and 12 under GNU-Linux | 1482 | 42 |
| PT A3 | F. Kupka & F.J. Robinson | Coherent structures in granulation convection and their importance for higher order closure models | 1773 | 43 |
| PT A4 | F. Kupka & I.W. Roxburgh | Reynolds stress models of convection in stellar structure calculations for convective cores. | 1774 | 44 |
| PT A5 | F. Kupka & H.J. Muthsam | Probing Reynolds stress models of convection with numerical simulations: I. Overall properties: fluxes, mean profiles. | 1836 | 45 |
| PT A6 | F. Kupka & H.J. Muthsam | Probing Reynolds stress models of convection with numerical simulations: II. Non-locality and third order moments. | 1837 | 46 |
| PT A7 | F. Kupka & H.J. Muthsam | Probing Reynolds stress models of convection with numerical simulations: III. Compressibility, pressure fluctuations, and dissipation. | 1838 | 47 |
| PT A8 | H.J. Muthsam et al. | Modelling of Solar Granulation: Effects of Numerics, Resolution and Treatment of Opacity | 1843 | 48 |
| PT A9 | F. Kupka | Some open questions concerning the modelling of non-locality in Reynolds stress type models of stellar convection. | 1849 | 49 |
| PT A10 | P. Ventura & V. Penza | The impact of non grey atmospheric treatment and convective modelling on the solar structure. | | |
| Session B: Observational Probes of Convection |
| PT B1 | B. Smalley | Stellar Fluxes as Probes of Convection in Stellar Atmospheres | 0423 | 50 |
| PT B2 | R.V. Yudin et al. | Magnetic fields in Herbig Ae/Be stars | 0568 | 51 |
| PT B3 | P. Gondoin | On the relation between rotation, convection and magnetic activity in intermediate-mass giants | 0984 | 52 |
| PT B4 | J. Southworth | Testing Convection In Stellar Models Using Eclipsing Binaries | 1180 | 53 |
| PT B5 | L. da Silva et al. | The Li depletion in Southern Young Stellar Associations | 1867 | 54 |
| PT B6 | M. Gebran & R. Monier | Microturbulent Velocities and Abundances for A and F dwarfs in Open clusters | 2008 | 55 |
| PT B7 | K. Janssen & G. Cauzzi | Reversed Granulation In Mid-Photosphere Of The Sun | 2048 | 56 |
| PT B8 | J. Montalban et al. | The Effect of the microturbulence parameter on the Color-Magnitude Diagram | 2131 | 57 |
| PT B9 | U. Heiter et al. | Eclipsing binaries as a test for synthetic photometry | 2242 | 58 |
| PT B10 | S.G. Els & K. Vogiatzis | Revealing the onset of convection in terrestial planet atmospheres. | 2276 | 59 |
| Session C: Convection in planets and brown dwarfs |
| PT C1 | M. Evonuk & G.A. Glatzmaier | Vorticity generation and heat transport in 3D anelastic simulations of the internal dynamics of giant planets without cores | 0459 | 60 |
| PT C2 | Ch. Helling | The chemical composition of dust clouds in a turbulent brown dwarf atmosphere | 1201 | 61 |
| PT C3 | M. Dehn et al. | The influence of convective energy transport on dust formation in brown dwarf atmospheres | 1275 | 62 |
| PT C4 | K.L. Chan | A Finite-Difference Convective Model for Jupiter's Equatorial Jet | 1505 | 63 |
| Session D: Stellar evolution, nucleosynthesis, and convective mixing |
| PT D1 | C.A. Meakin & W.D. Arnett | Simulations of Type II Supernova Progenitors: Oxygen and Silicon Shell Burning Hydrodynamics | 0171 | 64 |
| PT D2 | R. Smiljanic et al. | The Extra Mixing After the RGB-Bump from C12/C13 Ratios | 0379 | 65 |
| PT D3 | G. Tautvaisiene et al. | Abundances of C, N and O as Probes of Mixing in Low-Mass Helium-Core Burning Stars | 0599 | 66 |
| PT D4 | N.A. Drake & C.B. Pereira | CNO and Li Abundances in Barium-Enriched Stars | 0661 | 67 |
| PT D5 | T. Tsuji | Isotopic Abundances of Carbon and Oxygen in Oxygen-Rich Giants as Probes of Mixing in RGB and AGB Stars | 1277 | 68 |
| PT D6 | N.R.L. Landin et al. | Rotational Properties of the Orion Nebular Cluster Revised | 1469 | 69 |
| PT D7 | M. Flaskamp & A. Weiss | Inclusion of a time-dependent, non-local convection theory in a stellar evolution code | 1637 | 70 |
| PT D8 | G.P. Bascoul | Numerical Simulations of Semiconvection | 1693 | 71 |
| PT D9 | J. Montalban & F. D'Antona | Pre-MS sequence models with convection description given by 2D-RHD numerical simulations | 2124 | 72 |
| PT D10 | N.J. Hammer et al. | Convective Processes And Hydromagnetic Instabilities In Core Collapse Supernova Simulations | 2189 | 73 |
| PT D11 | M. Liebendoerfer et al. | Toward Three-Dimensional Simulations of Stellar Core Collapse with Magnetic Fields | 2428 | 74 |
| Session E: Oscillations, mass loss, and convection |
| PT E1 | J.Y. Yang & Y. Li | Testing turbulent hydrodynamic models in solar interior | 0074 | 75 |
| PT E2 | K. Belkacem et al. | A Closure Model for Turbulent Convection. Application to the Stochastic Excitation of Stellar p modes | 0286 | 76 |
| PT E3 | L. Deng & D.R. Xiong | Non-adiabatic oscillations of red giants | 0294 | 77 |
| PT E4 | E. Pakstiene | Monitoring of the Cool ZZ Ceti Star PG 2303+243. | 0613 | 78 |
| PT E5 | J. Montalban & M.-A. Dupret | Effect of convection modelling on non-adiabatic seismic observables of delta Scuti stars | 2117 | 79 |
| PT E6 | C.W. Straka et al. | Probing Turbulence with Seismic Observations of α Centauri | 2251 | 80 |
| Session F: Convection and rotation |
| PT F1 | A.S. Petrosyan | Mean-Field Hydrodynamics For Turbulent Flows Subjected Rotation | 0230 | 81 |
| PT F2 | L.T.S. Mendes et al. | Theoretical Estimates of the Convective Turnover Time for Low-Mass, Rotating Pre-Main Sequence Stars | 0448 | 82 |
| PT F3 | O. Kuzmanovska | The Redistribution Of The Regions In Radiative And Convective Equilibrium Of The Stars Of The Main Sequence With Rotation | 0449 | 83 |
| PT F4 | G.J.J. Botha & E.A. Evangelidis | Differential Rotation And Angular Momentum | 1246 | 84 |
| Session G: MHD convection and dynamos |
| PT G1 | A.V. Getling & X.M. Bao | Is Solar Convection Responsible for the Local Amplification and Structuring of Magnetic Fields? | 0416 | 85 |
| PT G2 | A.V. Getling & A.A. Buchnev | Quasi-Regular Structures in the Solar Photosphere (Trenching in the Brightness Relief): Algorithmic Treatment | 0417 | 86 |
| PT G3 | V.N. Kryvodubskyj | "Negative Magnetic Buoyancy" Effects and Reconstruction of Toroidal Field in the Solar Convection Zone | 0515 | 87 |
| PT G4 | R. Samec et al. | Magnetic Activity In The Atmospheres of F-Type Binaries | 0837 | 88 |
| PT G5 | G.J.J. Botha et al. | Numerical Simulations Of Sunspots | 1247 | 89 |
| PT G6 | M.K. Browning et al. | Simulations of solar magnetic dynamo action in the convection zone and tachocline | 1607 | 90 |
| PT G7 | D. Skandera & W.-Ch. Müller | Spectral Properties of Magnetohydrodynamic Convection With a Horizontal Temperature Gradient | 1666 | 91 |
| PT G8 | P.J. Bushby | Super-equipartition fields in simulations of photospheric magnetoconvection | 1257 | |
