First Ten Years of Hinode Solar On-Orbit Observatory

<p>Part I Reviews on 10 Years of Hinode</p><p><br/></p><p>A Brief History of Hinode – Toward the Success in Orbit</p><p>1 Birth of Hinode</p><p>2 Instrument Overview</p><p>3 Science Achievements</p><p>4 International Collaboration</p><p>5 As On-Orbit Solar Observatory</p><p>6 Ups and Downs in Operations</p><p>7 Future Prospects</p><p>References</p><p><br/></p><p>Hinode’s Contributions to Solar Physics</p><p>1 High Resolution Observation of the Sun in the Visible Wavelengths</p><p>2 Discovery of Various Waves and Corona Heating</p>3 Active Region Outflows and the Solar Wind<p></p><p>4 Outlook for the Future</p><p>References</p><p><br/></p><p>Ten-Year Results of Solar Optical Telescope (SOT) Onboard Hinode</p><p>1 Scientific Objectives of Solar Optical Telescope</p><p>2 Resolution of Photospheric Magnetic Structures in Quiet Sun</p>3 Resolution of Dynamical Phenomena in the Chromosphere<p></p><p>4 Summary</p><p>References</p><p><br/></p><p>X-ray Telescope (XRT) aboard Hinode: Key instrumental features and scientific highlights</p><p>1 Scientific Background of XRT and Key Instrumental Features</p><p>2 Some Scientific Highlights from XRT</p>3 Summary<p></p><p>References</p><p><br/></p><p>Solar Extreme Ultraviolet Spectroscopy: zur NachEISzeit</p><p>1 EISberg before Hinode (“Sunrise”)</p><p>2 Ice-breaking (EISbrechend) scientific problems</p><p>3 Scientific objectives for post-gracial age (NachEISzeit)</p><p>References</p><p><br/></p><p>Part II Coronal Heating and Solar Wind</p><p><br/></p><p>Coronal Heating: issues revealed from Hinode observations</p><p>1 Introduction</p><p>2 Before the birth of Hinode</p><p>3 From Yohkoh to Hinode</p>4 Achievements by Hinode on Coronal Heating<p></p><p>5 Concluding Remarks</p><p>References</p><p><br/></p><p>Importance of MHD Waves Observed with Hinode</p><p>1 Introduction</p><p>2 Discoveries of waves</p><p>3 Energy flux estimation using numerical simulation</p><p>4 Estimation of magnetic field using MHD waves</p><p>5 Waves or mass loss?</p><p>6 Summary</p><p>References</p><p><br/></p><p>Hinode Investigations of Microflares and Nanoflares</p><p>1 Small flares in the Sun</p><p>2 Physical processes of microflares and nanoflares</p><p>3 Investigating signatures of unresolved nanoflares</p><p>4 Summary and future observations</p><p>References</p><p><br/></p><p>The Origin of the Solar Wind</p><p>1 Introduction</p><p>2 Fast Wind</p><p>3 Slow Wind</p><p>4 Future Prospects</p><p>References</p><p><br/></p><p>Part III Magnetism of Solar Atmosphere</p><p><br/></p><p>New Insights into Sunspots through Hinode Observations</p><p>1 Sunspot Studies before Hinode</p><p>2 Sunspot Fine-scale Structures</p><p>3 Sunspot Formation</p><p>4 Sunspot Decay</p><p>5 Future Works</p><p>References</p><p><br/></p><p>Three-Dimensional Coronal Magnetic Field Based on the Photospheric Magnetic Field by Hinode/SP Observation</p><p>1 Introduction</p>2 Nonlinear Force-Free Field Extrapolation<p></p><p>3 NLFFF Extrapolation Based on the Observed Magnetic Field</p><p>4 Current State and Future</p><p>References</p><p><br/></p><p>New Approach to Solar Flare Trigger Process with Hinode/Solar Optical Telescope</p><p>1 Solar Flare Trigger Problem</p>2 Flare-triggering Structure Observed by Hinode/SOT<p></p><p>3 Future Direction</p><p>References</p><p><br/></p><p>Hinode Observations of Flows and Heating Associated with Magnetic Reconnection during Solar Flares</p><p>1 Introduction</p><p>2 Flows</p><p>3 Heating</p><p>4 Conclusions and Future Prospects</p><p>References</p><p><br/></p><p>The First Decade of Hinode: understanding Coronal Mass Ejections</p><p>1 Introduction</p><p>2 The build-up to a CME</p><p>3 Observations of the CME</p><p>4 Propagation of the CME</p><p>5 Summary</p><p>References</p><p><br/></p><p>Understanding Magneto-Convection on Solar Surface with Hinode Satellite Observation</p><p>1 Why do we prefer smaller scale?</p><p>2 Observational results and new knowledge obtained by Hinode</p><p>3 Future tasks in the following 10 years</p><p>References</p><p><br/></p><p>Hinode Observation of the Sun’s Polar Magnetic Field and Solar Cycle Variation</p><p>1 Introduction</p><p>2 Polar region monitoring by Hinode</p><p>3 Future solar cycle variation and polar region monitoring</p><p>References</p><br/><p></p><p>Local Helioseismology Analyses with Hinode/SOT Datasets</p><p>1 Introduction</p><p>2 Advantages of SOT Local Helioseismology</p><p>3 Significant Results of SOT Helioseismology</p><p>4 Outlook</p><p>References</p><p><br/></p><p>Part IV Newly Opened Physics and Future Observations</p><p><br/></p><p>Penumbral Microjets in Sunspot Chromospheres: Evidence of Magnetic Reconnection</p><p>1 Dynamic Chromosphere Revealed by Hinode</p><p>2 Discovery of Penumbral Microjets</p><p>3 Influence on Heating of the Transition Region and Corona</p><p>4 Summary and Future Direction</p><p>References</p><p><br/></p><p>Physics of Partial Ionization in the Solar Chromosphere Revealed by the Solar Optical Telescope on board Hinode</p><p>1 Introduction</p><p>2 Plasma parameters and theoretical treatments</p><p>3 Brief overview of the SOT results</p><p>4 Concluding Remark</p>References<p></p><p><br/></p><p>Thermal Non-equilibrium Plasma Observed by Hinode</p><p>1 Introduction</p><p>2 Ion Temperature in a Solar Active Region</p><p>3 Non-equilibirum Ionization During a Solar Flare</p><p>4 Summary and Future Perspectives</p><p>References</p><p><br/></p><p>From Hinode to the Next-Generation Solar Observation Missions</p><p>1 Introduction</p><p>2 The SOLAR-C Project</p><p>3 Small Size Space Missions</p><p>4 Ground-based Observations</p><p>5 Summary</p><p>References </p><p><br/></p><p>Part V Science Center and Public Outreach</p><p><br/></p><p>Hinode Science Center at NAOJ - from the preparations of the establishment to the issues for the future -</p><p>1 Particularity of solar observation data in astrophysical studies</p><p>2 Data analysis system for solar observing satellites</p><p>3 Preparation for establishing the Hinode Science Center</p><p>4 10 years of Hinode Science Center</p><p>5 Issues for the future</p><p>References</p><p><br/></p><p>Public Outreach and Education Activities of Solar Mission Hinode in Japan</p><p>1 Introduction</p><p>2 Working Group for Public Use of Hinode Data</p><p>3 Let’s look at the Sun with Hinode!</p><p>4 A Lot of Thought into Our Outreach Activities</p><p>5 Conclusion</p><p>References</p><p><br/></p><p>A Hinode Image Gallery</p><p>A.1 Quiet Sun</p><p>A.2 Sunspots</p><p>A.3 Chromosphere</p><p>A.4 Corona</p><p>A.5 Flares and Eruptions</p><p>A.6 Astronomical Events</p><p><br/></p><p>Index</p><div><br/></div>