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	Introduction Physical Models Assumptions of Simulations Coronal Seismology Energy Input Non-LTE Diagnostics Chromospheric/Coronal Spectropolarimetry Magnetic Fields Energy Transport and Dissipation Tutorial: Non-LTE Diagnostics Made Fun! Coupling on Large Scales		Invited Talks at the SDO-4/IRIS/Hinode Workshop - March 2012 • Schedule • All Invited Talks (zip file) Introduction • Hansteen: Overview of Simulations and Observations of the Coupling Between Solar Regions • Tarbell: How to Exploit Current and Future Instrumentation to Understand the Coupled Solar Atmosphere • Young: Doing Science with IRIS - Experience Learned from Hinode/EIS (poster) Physical Models • Gudiksen: State-of-the-Art of Single Fluid MHD Numerical Modeling of the Coupled Solar Atmosphere • Khomenko: Beyond Single Fluid MHD: Multi-fluid Modeling of the Coupled Solar Atmosphere • Van Ballegooijen: The Role of Magnetic Braiding and MHD Wave Dynamics in the Heating of the Sun's Outer Atmosphere Assumptions of Simulations • Judge: Key- or Tomb- stones in the Bridge from Photosphere to Corona? • Klimchuk: The Pros and Cons of 1D vs 3D Modeling Strengths and Limitations of Coronal Seismology • De Moortel: What We Can and Cannot Learn from Seismology of the Solar Atmosphere • van Doorsselaere: What We Can and Cannot Learn from Seismology of the Solar Atmosphere • McIntosh: What We Can and Cannot Learn from Seismology of the Solar Atmosphere Energy Input • Cameron: Observational/Modeling Constraints of Magneto-convective Energy into Photosphere • Fisher: Electric Fields and Poynting Fluxes from Vector Magnetograms and Doppler Shifts Non-LTE Diagnostics • Rutten: Graphical Introduction to NLTE Chromospheric Line Formation • Carlsson: State-of-the-art of non-LTE Diagnostics: Observations and Simulations • Mason: IRIS: Transition Region and Coronal Diagnostics Chromospheric/Coronal Spectropolarimetry • Asensio-Ramos: Inversion Tools for Chromospheric Lines • Centeno: Opportunities and Challenges in Determining the Chromospheric Magnetic Field Using He I 10830 • Harvey: Opportunities and Challenges in Determining the Chromospheric Magnetic Field • de la Cruz Rodriguez: NLTE Inversions from a 3D MHD Chromospheric Simulation • Tomczyk: Constraints on Coronal Magnetic Fields from Observations of Visible and IR Emission Lines Magnetic Fields • Moreno-Insertis: Magnetic Flux Emergence into the Atmosphere: 3D Numberical Models • DeRosa: The Impact of the Chromosphere of Magnetic Fields: Field Exptrapolations • Abbett: The Impact of the Chromosphere on Numerical Models of the Convection Zone-to-Corona Energy Transport and Dissipation • Isobe: Observations and Modeling of Magnetic Reconnection in the Solar Atmosphere • McIntosh: Observational Evidence of Magnetic Waves in the Solar Atmosphere • De Moortel: Coupling, Damping and Dissipation of Magnetic Waves in the Chromosphere and Corona • Nordlund: Beyond Single Fluid MHD: Modeling Kinetic Effects in the Coupled Solar Atmosphere • Tian: The Mass Cycle Between the Chromosphere and the Corona/Solar Wind Tutorial: Non-LTE Diagnostics Made Fun! • Uitenbroek: How to Calculate non-LTE Diagnostics using RH • Leenaarts: How to do 3D Radiation • Uitenbroek: Problems with 1D Semi-emperical Modeling • Uitenbroek: NLTE Discussion of Response Funcitions/Contribution Functions/Formation Height • Leenaarts: Basic Properties of the Mg II h & k Line Formation Coupling on Large Scales & Into the Solar Wind • Antiochos: The Role of Topology in the Energetics of the Couple Solar Atmosphere • Mikic: Global MHD Models of the Corona and Solar Wind
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