› Buoyant Rise of Active Region Flux Tubes in a Solar-like Convective Envelope - Yuhong Fan, National Center for Atmospheric Research
09:00-09:35 (35min)
› Global dynamics of subsurface active regions - Laurène Jouve, IRAP
09:35-10:10 (35min)
› Multi-parametric study of rising 3D buoyant flux tubes in an adiabatic stratification using AMR - Juan Martinez-Sykora, Lockheed Martin Solar and Astrophysics Laboratory
10:10-10:45 (35min)
› Flux emergence in the solar global convection calculation with the reduced speed of sound technique. - Hideyuki Hotta, University of Tokyo
11:15-11:50 (35min)
› Probing Emerging Magnetic Flux and the Nature of Detected Pre-emergence Signatures - Stathis Ilonidis, Stanford University
11:50-12:25 (35min)
› Observations of the Magnetic Flux Approaching the Visible Surface - Shin Toriumi, University of Tokyo
12:25-13:00 (35min)
› Active Region Emergence, a New Paradigm - Robert Stein, Michigan State University
14:30-15:05 (35min)
› Modeling the Origin of Tilt, Twist, Active Longitudes, and More: Buoyant Loops in Global Convective Dynamos - Nicholas Nelson, University of Colorado
15:05-15:40 (35min)
› Flux emergence in a magnetized convection zone - Rui Pinto, LESIA - Observatoire de Paris & AIM/SAP - CEA Saclay
15:40-16:15 (35min)
› Magnetic helicity properties of emerging active regions determined from longitudinal photospheric magnetograms. - Mariano Poisson, Instituto de Astronomía y Física del Espacio, Facultad de Ciencas Exactas y Naturales
17:20-17:55 (35min)
› Photospheric injection of magnetic helicity during AR 11158 emergence - Kevin Dalmasse, LESIA - Observatoire de Paris
17:55-18:30 (35min)
› Collective Solar Behavior - Alan Title, LM Space Astrophysics Laboratory
09:00-09:35 (35min)
› The role of preexisting magnetic environment with newly emerging flux in flares - Brigitte Schmieder, LESIA - Observatoire de Paris
09:35-10:10 (35min)
› Condition for arcade field eruption triggered by a flux emergence event - Takaaki Yokoyama, University of Tokyo
10:10-10:45 (35min)
› Structures of Emerging Flux Triggering Solar Eruptions - Kanya Kusano, Solar-Terrestrial Environment Laboratory, Nagoya University
11:15-11:50 (35min)
› Flux emergence and solar eruptive events - Vasilis Archontis, University of St Andrews
11:50-12:25 (35min)
› Chromospheric Canopy Fields over a Flux Emerging Region as a Key Condition for Formation of the Sunspot Penumbra - Eunkyung Lim, Korea Astronomy and Space Science Institute
16:45-17:20 (35min)
› High resolution spectro-polarimetric observations of the formation of a penumbra - Paolo Romano, INAF - Catania Astrophysical Observatory
17:20-17:55 (35min)
› The Magnetic Flux History of a Quiet-Sun Supergranular Cell - Luis Bellot Rubio, Instituto de Astrofísica de Andalucía-CSIC
09:00-09:35 (35min)
› High resolution analysis of a magnetic bubble emerging through the solar atmosphere - Ada Ortiz Carbonell, Institute of Theoretical Astrophysics
09:35-10:10 (35min)
› Signatures of small-scale magnetic field emergence as seen from the New Solar Telescope in Big Bear - Vasyl Yurchyshyn, Big Bear Solar Observatory
10:50-11:25 (35min)
› Small-scale flux emergence from the photosphere to the corona - Fernando Moreno-Insertis, Instituto de Astrofísica de Canarias
11:25-12:00 (35min)
› A Detailed Comparison Between The Observed and Synthesized Properties of a Simulated Type II Spicule. - Viggo Hansteen, Institute of Theoretical Astronomy, University of Oslo
09:00-09:35 (35min)
› Recurrent Coronal Jets Induced by Magnetic Emergence - Pascal Démoulin, LESIA - Observatoire de Paris
09:35-10:10 (35min)
› Jets and eruptions following magnetic flux emergence into the corona - Fernando Moreno-Insertis, Instituto de Astrofísica de Canarias
10:10-10:45 (35min)
› Energy Buildup in Active Regions: A Comparison of AR11158 with a Simulation of Magnetic Flux Emergence - Ward Manchester, Center for Space Environment Modeling, University of Michigan
11:15-11:50 (35min)
› Evolution of electric currents during active region formation - Tibor Torok, Predictive Science Inc.
11:50-12:25 (35min)
› Magnetic topology, the key to understanding the jets and eruptions following magnetic flux emergence into the corona !? - Klaus Galsgaard, Niels Bohr Institute & University of Copenhagen
14:30-15:05 (35min)
› Time-Dependence of Topological Features of PFSS Models of the Solar Corona - Marc DeRosa, Lockheed Martin Solar and Astrophysics Laboratory
15:05-15:40 (35min)
› Nonlinear force-free extrapolation of emerging flux - Gherardo Valori, LESIA - Observatoire de Paris
15:40-16:15 (35min)
Data-Driven Modeling of Emerging Flux and Active Regions
Chairperson : Etienne Pariat
› Estimating flare's free energy using Poloidal-Toroidal Decomposition method. - Maria Kazachenko, Space Sciences Laboratory
16:45-17:20 (35min)
› A Magnetofrictional Method for Data-driven Simulations of Evolving Solar Coronal Fields - Mark Cheung, Lockheed Martin Solar and Astrophysics Laboratory - DeRosa Marc, Lockheed Martin Solar & Astrophysics Laboratory
17:20-17:55 (35min)
