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| The Solar-B EUV Imaging Spectrometer: An Overview of the EIS Instrument | p. 3 |
| The X-Ray Telescope for Solar-B: Calibration and Predicted Performance | p. 19 |
| Archiving, Distribution and Analysis of Solar-B Data | p. 31 |
| Application of CHIANTI to Solar-B | p. 35 |
| Calibration of the SOT Polarization | p. 39 |
| Calibration of SOT Dopplergrams | p. 43 |
| Examinations of the Relative Alignment of the Instruments on SOT | p. 47 |
| Estimate on SOT Light Level in Flight with Throughput Measurements in SOT Sun Tests | p. 51 |
| Performance Characteristics of the Solar-B Spectro-Polarimeter | p. 55 |
| The Solar-B Science Center in Japan | p. 59 |
| Temperature Analysis with the XRT | p. 63 |
| Recent High Resolution Observations and Interpretations of Sunspot Fine Structure | p. 71 |
| Solar Magneto-Convection Simulations | p. 87 |
| Helicity as the Ultimate Test to the Surface Dynamo Problem | p. 99 |
| What are 'Faculae'? | p. 103 |
| Supersonic Downflows in the Photosphere Discovered in Sunspot Moat Regions | p. 113 |
| Small Scale Energy Release Driven by Supergranular flows | p. 119 |
| The Quiet Sun Magnetic Field | p. 125 |
| What Can We Learn about Filaments from Vector Magnetograms | p. 137 |
| Magnetic Correspondence between Moving Magnetic Features and Penumbral Magnetic Fields | p. 145 |
| Formation of Magnetic Non-Potentiality in a Solar Active Region | p. 153 |
| Skew Angle and Magnetic Helicity in Solar Active Regions | p. 163 |
| Evolutionary Characteristics of Magnetic Helicity Injection in Active Regions | p. 167 |
| The Use of Spectro-Polarimetric Measurements to Determine the Plasma Heating | p. 171 |
| Determination of Magnetic Helicity of a Solar Active Region using the Linear Force-Free Field Model | p. 175 |
| Helicity Injection in Regions of Various Magnetic Fluxes | p. 179 |
| Calculations of Photospheric Plasma Velocity Fields using Photospheric Magnetic Field Measurements | p. 183 |
| Waves and Shocks in the Solar Atmosphere | p. 193 |
| Plans to Observe Flare-Associated Waves with Solar-B | p. 205 |
| Flare-Associated Oscillations in Coronal Multiple-Loops Observed with the Norikura Green-Line Imaging System | p. 213 |
| Solar-B as a Tool for Coronal Wave Studies | p. 221 |
| Observed Co-Temporal Oscillations by CDS and TRACE and the Implications for Solar-B Instrumentation | p. 225 |
| Chromospheric Dynamics: Spicules and Waves | p. 231 |
| Chromospheric Magnetic Reconnection | p. 243 |
| The Relationship between EUV Brightenings and Dark Mottles in the Quiet Sun | p. 257 |
| Towards Understanding the Solar Atmosphere | p. 263 |
| Topological Dissipation and The Solar Corona | p. 269 |
| Limb Prominences seen in UV, EUV and SXR | p. 279 |
| Observational Analysis of the Relation between Coronal Loop Heating and Photospheric Magnetic Fields | p. 287 |
| Magnetic Twist of EUV Coronal Loops observed by TRACE | p. 299 |
| Investigation of Coronal Loop Temperatures Using Three EUV Filters and Implications for Future Work with Solar-B | p. 303 |
| Studying Transition Region Phenomena with Solar-B/EIS | p. 307 |
| Local Helioseismology | p. 313 |
| Observations of Helioseismic Response to Flare Energy-release Events | p. 325 |
| Three-Dimensional Numerical Experiments of Flux Emergence into the Corona | p. 335 |
| Observation of Magnetic Field Reconnection at the Base of EFR Surges | p. 347 |
| Three-Dimensional MHD Simulations of Emerging Flux and Associated Magnetic Reconnection | p. 355 |
| Flux Cancellation Associated with Flux Emergence on the Sun | p. 367 |
| 3-D Magnetohydrodynamics Simulation of the Solar Emerging Flux | p. 371 |
| Magnetohydrodynamic Numerical Simulations of Emerging Flux Tube for Studying Effects of Twist Intensity | p. 377 |
| Three-dimensional Filament Eruption Driven by a Emerging Flux | p. 381 |
| Correlation between Increases of Magnetic Fluxes and Brightenings of Coronal Structures around Emerging Flux Regions | p. 385 |
| Recent Progress in Study of Magnetic Reconnection in a Laboratory Plasma and Possible Application to Space Astrophysical Plasmas | p. 391 |
| Investigation of Reconnection in the Solar Corona by Numerical Simulation Based on Solar-B Observations | p. 407 |
| Simulation Study of Three-Dimensional and Nonlinear Dynamics of Flux Tube in the Solar Corona | p. 421 |
| Low Atmosphere Reconnections Associated with a Filament Eruption | p. 425 |
| A Statistical Study of the Reconnection Rate in Solar Flares | p. 429 |
| Self-similar Reconnection : A new model for Astrophysical Application beyond the Petschek Model | p. 433 |
| XRT and EIS Observations of Reconnection Associated Phenomena | p. 439 |
| Oblique Shocks in the Reconnection Jet in Solar Flares | p. 443 |
| Structure and Evolution of Magnetic Fields Leading to Solar Flares | p. 449 |
| Evolution of H[alpha] Kernels and Energy Release in an X-Class Flare | p. 461 |
| Simulation Study of Transition Process from Long-Lived Sigmoid to Flare Eruption | p. 469 |
| Flare Energy Conversion due to Direct Electric Fields Resulting from the Sheared Reconnection | p. 477 |
| High Velocity Doppler shift Observations of 10 MK Flare Plasma | p. 481 |
| Observations of Simultaneous Coronal Loop Shrinkage and Expansion during the Decay Phase of a Solar Flare | p. 485 |
| Supra-Arcade Downflows: Results from Observational Analysis | p. 489 |
| Quantitative Analysis of Nonthermal Electrons in Impulsive Hard X-ray Flares | p. 493 |
| Electron Acceleration at the Earth's Bow Shock, Solar Flares and Interplanetary Shocks | p. 497 |
| Combining Hydrodynamics Modeling with Test Particle Tracking to Improve Flare Simulations | p. 501 |
| A Simulation of Flares in YSOs with Non-thermal Heating and Expected Hard X-ray Spectrum | p. 505 |
| Solar Origins of Interplanetary Coronal Mass Ejections | p. 511 |
| Multidimensional Simulations of Filament Channel Structure and Evolution | p. 525 |
| Origin of the Sheared Magnetic Fields that Explode in Flares and Coronal Mass Ejections | p. 539 |
| Observation of a Coronal Mass Ejection and its Source Region with NOrikura Green-line Imaging System (NOGIS) | p. 543 |
| What Coronal Parameters Determine Solar Wind Speed? | p. 549 |
| Self-consistent MHD Modeling of Solar Wind | p. 557 |
| The energetics of the Slow Solar wind | p. 569 |
| Study of Small-Scale Dynamics in Quiet Regions from TRACE/BBSO Observations | p. 573 |
| Summary Review: Science with the SOT | p. 579 |
| Two Fundamental MHD Problems in Solar Physics | p. 587 |
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