| Preface |
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xiii | |
| Participants |
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xvii | |
| Conference Photograph |
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xxiii | |
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Session
1. Photospheric Magnetism |
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Signatures of Penumbral Magnetic Fields at Very High Spatial Resolution |
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3 | (10) |
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The Micro-Structure of a Sunspot Penumbra |
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13 | (6) |
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19 | (6) |
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Inversion of Visible and IR Stokes Profiles in Sunspots |
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25 | (6) |
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Penumbral Moving Magnetic Features |
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31 | (5) |
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Internetwork Magnetic Field Distribution from Simultaneous Fe I 1.5 μm and Fe I 630 nm Observations |
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36 | (6) |
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On the Determination of Magnetic Field Strength and Flux in Inter-Network |
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42 | (6) |
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Magnetic Fields of the Quiet Sun: Distribution of Field Strengths |
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48 | (6) |
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Quiet-Sun Magnetism Seen with a Mn Line: Km-Sized Magnetic Structures |
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54 | (7) |
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G-Band Bright Points and Photospheric Magnetic Fields |
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61 | (7) |
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Multi-Line Spectro-Polarimetry of Filaments |
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68 | (4) |
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Polarimetric Observations of the Formation of a G-Band Bright Point |
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72 | (4) |
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Photospheric Dynamic Model of Magnetic Reconnection |
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76 | (4) |
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Proper Motions in Sunspot Penumbrae: Signs of Convection |
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80 | (4) |
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3D Reconstruction of Photospheric Velocity Fields Inside a Magnetic Network Cell |
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84 | (4) |
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Quiet-Sun Magnetic Fields: Simultaneous Inversion of Visible and IR Spectro-Polarimetric Observations |
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88 | (4) |
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SOLIS-VSM Solar Vector Magnetograms |
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92 | (4) |
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The Evershed Effect with 0``.2 Angular Resolution |
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96 | (4) |
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Systematic Errors in Dopplergrams of Active Regions and Their Correction |
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100 | (7) |
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Session
2. Radiative Transfer Methods and Inversion Techniques |
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Stokes Inversion Techniques: Recent Advances and New Challenges |
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107 | (12) |
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UNNOFIT Inversion of Spectro-Polarimetric Maps Observed with THEMIS |
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119 | (1) |
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Interpretation of the Second Solar Spectrum of the Sr I 4607 A Line Observed at THEMIS and Pic-du-Midi |
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120 | (6) |
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Polarized Spectral Line Formation in Turbulent Magnetic Fields: The Zeeman and Hanle Effects |
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126 | (6) |
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Major Effects of Line Asymmetries in Solar Magnetic Field Measurements from Simultaneous Multi-Wavelength Observations |
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132 | (5) |
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The Characteristic Length Scale of the Magnetic Fluctuation in a Sunspot Penumbra: A Stochastic Polarized Radiative Transfer Approach |
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137 | (7) |
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Magnetic Field Vector Retrieval with HMI |
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144 | (4) |
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Multigrid Methods for Polarized Radiative Transfer |
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148 | (7) |
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Session
3. New Solar Polarimeters and Techniques |
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Tunable Narrow-Band Filter for Imaging Polarimetry |
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155 | (6) |
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The Solar Ultraviolet Magnetograph Investigation: Polarization Properties |
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161 | (6) |
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Solar Spectro-Polarimetry at Pic-du-Midi/LJR |
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167 | (6) |
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Magnetic Field Measurements in Flare Loops and CMEs |
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173 | (4) |
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First Steps Towards the Electronic Inversion of the Radiative Transfer Equation |
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177 | (4) |
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Vacuum Ultraviolet Fabry-Perot Interferometers for Transition-Region Magnetography |
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181 | (4) |
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High-Precision Imaging Polarimetry in the Hα line |
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185 | (4) |
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Magnetic Field Diagnostic Capability of Solar-B/SOT: Filtergraph Instrument |
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189 | (4) |
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Spectral Line Selection for HMI |
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193 | (4) |
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Milne-Eddington Response Functions and Their Applications |
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197 | (4) |
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The Diffraction Limited Spectro-Polarimeter |
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201 | (4) |
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The Ba II 4554 / Hβ Imaging Polarimeter for the Dutch Open Telescope |
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205 | (4) |
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Large Field-of-View KD*P Modulator for Solar Polarization Measurements |
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209 | (6) |
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Session
4. Atomic Spectro-Polarimetry |
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Second Solar Spectrum: A Brief Overview |
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215 | (10) |
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Polarimetry of the Second Solar Spectrum in the UVB |
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225 | (6) |
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Second Spectrum of Na I D1 Observed with THEMIS |
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231 | (6) |
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Polarized Scattering in Strong Chromospheric Lines: Theory and Its Confrontation with Observations |
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237 | (8) |
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Session
5. Theory of Collisional Polarization |
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Semi-Classical Collision Formalism with Energy and Momentum Transfer |
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245 | (11) |
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Calculation of Depolarization and Polarization Rates by Isotropic Collisions with Neutral Hydrogen |
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256 | (13) |
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Session
6. Laboratory Experiments and Molecular Spectro-Polarimetry |
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The Hanle Effect in Atomic and Molecular Lines: A New Look at the Sun's Hidden Magnetism |
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269 | (24) |
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Polarizability Factors for Molecular Bands |
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293 | (8) |
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Theory, Observation, and Modeling of the Zeeman and Paschen-Back Effects in Molecular Lines |
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301 | (10) |
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Hanle Effect in the Paschen-Back Regime |
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311 | (6) |
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Multi-Line Determination of the Turbulent Magnetic Field from the Second Solar Spectrum of MgH |
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317 | (1) |
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Three-Dimensional Radiative Transfer Modeling of the Scattering Polarization in MgH Lines |
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318 | (1) |
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Spectro-Polarimetry of a Sunspot in Atomic and Molecular Lines with THEMIS |
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319 | (4) |
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Laboratory Experiment for Polarized Scattering at Potassium Vapor |
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323 | (6) |
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The Molecular Paschen-Back Effect |
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329 | (6) |
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Session
7. Stellar Spectro-Polarimetry |
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Spectro-Polarimetry of Cool Stars |
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335 | (10) |
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Spectro-Polarimetry of Magnetic Hot Stars |
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345 | (10) |
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Multi-Line Spectro-Polarimetry of Stellar Magnetic Fields Using Principal Components Analysis |
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355 | (7) |
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ESPaDOnS: The New Generation Stellar Spectro-Polarimeter. Performances and First Results |
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362 | (7) |
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Investigation of the Magnetic Field Characteristics of Herbig Ae/Be Stars: Discovery of the Pre-Main Sequence Progenitors of the Magnetic Ap/Bp Stars |
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369 | (6) |
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Molecular Diagnostics of the Internal Structure of Starspots and Sunspots |
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375 | (6) |
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Detection of the Molecular Zeeman Effect in Circular Polarization on Cool Active Stars |
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381 | (4) |
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Applied Doppler Imaging: Can Magnetic Activity of IM Pegasi Affect the Gravity Probe B Mission? |
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385 | (4) |
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Rotation and Chemical Abundances of Magnetic Ap/Bp Members in the Open Cluster NGC 6475 |
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389 | (4) |
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A Spectro-Polarimetric Survey of the Coolest Magnetic Ap Stars |
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393 | (4) |
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Magnetic Field Modeling of 78 Vir from the Analysis of Cr II Lines |
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397 | (4) |
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The Magnetic Activity of Young Suns: Magnetic Topologies and Differential Rotation of F- and G-Dwarfs |
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401 | (4) |
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PCA Technique Applied to the Detection of ZDI Circular Polarization in Solar-Type Stars |
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405 | (4) |
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An Evolutionary Study of Magnetic Ap Stars in 4 Northern Open Clusters |
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409 | (4) |
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Possible Detection of Weak Magnetic Fields in Two White Dwarfs, Including the Pulsating WD 1647+591 |
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413 | (6) |
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Session
8. Chromospheric Electro-Magnetism |
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419 | (10) |
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The Effect of Turbulent Electric Fields on the Scattering Polarization of Hydrogen Lines |
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429 | (2) |
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Measuring the Magnetic Vector with the He I 10830 A Line: A Rich New World |
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431 | (6) |
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Supersonic Downflows in the Vicinity of a Solar Pore |
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437 | (6) |
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Inference of the Magnetic Field in Spicules from Spectro-Polarimetry of He I D3 |
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443 | (5) |
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The Hanle and Zeeman Effects in Solar Spicules |
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448 | (6) |
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Spectro-Polarimetric Observations of Filaments in Hα and He 1 D3 |
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454 | (5) |
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The Hanle and Zeeman Effects in the Ba II D2 line |
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459 | (6) |
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Oscillations and Wave Propagation in Different Solar Magnetic Features |
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465 | (6) |
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Spectro-Polarimetry of Solar Prominences |
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471 | (4) |
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| Author Index |
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475 | |
