The Hinode Mission

The Solar-B satellite was launched in the morning of 23 September 2006 (06:36 Japan time) by the Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA), and was renamed to Hinode (‘sunrise’ in Japanese). Hinode carries three - struments; the X-ray telescope (XRT), the EUV imaging spectrometer (EIS), and the solar optical telescope (SOT). These instruments were developed by ISAS/JAXA in cooperation with the National Astronomical Observatory of Japan as domestic partner, and NASA and the Science and Technology Facilities Council (UK) as international partners. ESA and N- wegian Space Center have been providing a downlink station. All the data taken with Hinode are open to everyone since May 2007. This volume combines the ?rst set of instrumental papers of the Hinode mission (the mission overview, EIS, XRT, and the database system) published in volume 243, Number 1 (June 2007), and the second set of papers (four papers on SOT and one paper on XRT) published in Volume 249, Number 2 (June 2008). Another SOT paper cited as Tarbell et al. (2008) in these papers will appear later in Solar Physics.

The Solar-B satellite was launched in the morning of 23 September 2006 (06:36 Japan time) by the Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA), and was renamed to Hinode (‘sunrise’ in Japanese). Hinode carries three - struments; the X-ray telescope (XRT), the EUV imaging spectrometer (EIS), and the solar optical telescope (SOT). These instruments were developed by ISAS/JAXA in cooperation with the National Astronomical Observatory of Japan as domestic partner, and NASA and the Science and Technology Facilities Council (UK) as international partners. ESA and N- wegian Space Center have been providing a downlink station. All the data taken with Hinode are open to everyone since May 2007. This volume combines the ?rst set of instrumental papers of the Hinode mission (the mission overview, EIS, XRT, and the database system) published in volume 243, Number 1 (June 2007), and the second set of papers (four papers on SOT and one paper on XRT) published in Volume 249, Number 2 (June 2008). Another SOT paper cited as Tarbell et al. (2008) in these papers will appear later in Solar Physics.

This book provides the latest scientific understanding of the Sun, sharing insights gleaned from the international solar physics project Hinode. The authors (who are the main project contributors) review, from the various viewpoints, the discoveries and advances made by the on-orbit operations of the Hinode spacecraft in its first decade. Further, they present a wealth of scientifically important photographs and data from Hinode. Launched in September 2006, Hinode is the third Japanese solar observatory on orbit, and employs three highly advanced telescopes jointly developed and operated with international partners. The book describes the background of these research topics, how the Hinode telescopes have tackled various challenges, and the scientific achievements and impacts in the first 10 years. Furthermore, it explores future perspective of researches in Japan. The book will benefit undergraduate students interested in recent advance in the solar research, as well as graduate students and researchers working in solar physics, the space sciences, astronomy, and plasma physics.

SOHO, the Solar and Heliospheric Observatory, is a project of international cooperation between ESA and NASA to study the Sun, from its deep core to the outer corona, and the solar wind. To achieve its scientific goals it carries a complement of twelve sophisticated, state-of-the-art instruments. Three helioseismology instruments are expected to provide unique data for the study of the structure and dynamics of the solar interior, from the very deep core to the outermost layers of the convection zone. A set of five complementary remote sensing instruments, consisting of EUV and UV imagers, spectrographs and coronagraphs, will give us our first comprehensive view of the outer solar atmosphere and corona, leading to a better understanding of the enigmatic coronal heating and solar wind acceleration processes. Finally, three experiments will complement the remote sensing observations by making in-situ measurements of the composition and energy of the solar wind and charged energetic particles. This volume contains detailed descriptions of all the twelve instruments on board SOHO. Also included are an overview paper and a description of the SOHO ground system, science operations and data products. The aim of these papers is to make the broader scientific community, and in particular potential guest investigators, aware of the scientific objectives and capabilities of the SOHO payload and to provide a reference document for the various instruments.

Advances in Geosciences is the result of a concerted effort to bring together the latest results and planning activities related to earth and space science in Asia and the international arena. The volume editors are all leading scientists in their research fields covering six sections: Atmospheric Science (AS), Hydrological Science (HS), Ocean Science (OS), Solid Earth (SE), Solar Terrestrial (ST) and Planetary Science (PS). The main purpose is to highlight the scientific issues essential to the study of earthquakes, tsunamis, atmospheric dust storms, climate change, drought, flood, typhoons, monsoons, space weather, and planetary exploration. This volume is abstracted in NASA''s Astrophysics Data System: http: //ads.harvard.edu. Sample Chapter(s). Chapter 1: Ulf Waves: Exploring the Earth''s Magnetosphere (1,240k). Contents: ULF Waves: Exploring the Earth''s Magnetosphere (B J Fraser); Spectrum of Density Fluctuations in the Solar Wind (V Krishnan); Polarization Properties of the Ultra-Low Frequency Waves in Non-Axisymmetric Background Magnetic Fields (K Kabin et al.); and other papers. Readership: Academics, researchers and postgraduate students in geosciences

Advances in Geosciences is the result of a concerted effort to bring together the latest results and planning activities related to earth and space science in Asia and the international arena. The volume editors are all leading scientists in their research fields covering six sections: Atmospheric Science (AS), Hydrological Science (HS), Ocean Science (OS), Solid Earth (SE), Solar Terrestrial (ST) and Planetary Science (PS). The main purpose is to highlight the scientific issues essential to the study of earthquakes, tsunamis, atmospheric dust storms, climate change, drought, flood, typhoons, monsoons, space weather, and planetary exploration. This volume is abstracted in NASA's Astrophysics Data System: http://ads.harvard.edu Contents:Volume 10: Atmospheric Science (AS) Rainfall over Thailand during ENSO (1997–2000) (Wonlee & Prungchan)Formation of Tropical Cyclone Concentric Eye Walls by Wave–Mean Flow Interactions (J-Y Peng et al.)Anthropogenic Aerosol Radiative Forcing in the INDO-Gangetic Basi (S Dey & S N Tripathi)and other papersVolume 11: Hydrological Science (HS)Study for the Fresh Ground Water Resources, Neil, Island, India (V K Saxena)Emerging Concepts in Hydrology for Tropical Pacific Regimes (J Terry)Analysis of Monami Waves in Aquatic Vegetation (S Patil et al.)and other papersVolume 12: Ocean Science (OS)3D Current Characteristics Simulation with ANN (C Z Chew et al.)Classification of Ocean Waves from the Data Buoy Measurements (R Balaji et al.)Intercomparison of Various Latent Heat Flux Products in the South China Sea (Zhen et al.)and other papersVolume 13: Solid Earth (SE)The International Laser Ranging Service (M Pearlman et al.)Numerical Modeling of the 2006 Java Tsunami Earthquake (N R Hanifa et al.)Statistical Properties and Time Trend in the Number of Holocene Volcanic Eruptions. (A N Zemtsov & A A Tron)and other papersVolume 14: Solar Terrestrial (ST)ULF Waves: Exploring the Earth's Magnetosphere (B J Fraser)Spectrum of Density Fluctuations in the Solar Wind (V Krishnan)Polarization Properties of the Ultra-Low Frequency Waves in Non-Axisymmetric Background Magnetic Fields (K Kabin et al.)and other papersVolume 15: Planetary Science (PS)X-Rays from Nonmagnetic Planets (K Dennerl)Clouds, Clumps, Cores, and Comets — A Cosmic Chemical Connection? (S B Charnley & S D Rodgers)Comparative X-Ray Studies of Planetary Aurorae (G Branduardi-Raymont)and other papers Readership: Academics, researchers and postgraduate students in geosciences. Key Features: Provides an important source of new and not-yet-published results from the growing Asian and international geoscience community Presents a unique view of the rapid scientific progress made by Asian researchers in topics crucial to the future of the global environment Highlights a first-hand description of how the largest scientific population in the world is working together to manage the environmental problems which will determine the economic and social growth of the world itselfKeywords:Planetary Science;Atmosphere;Ionosphere;Magnetosphere “This set is the result of an effort to bring together the latest results and planning activities related to earth and space science in Asia and the international arena. The main purpose of this set is to highlight the scientific issues essential to the study of earthquakes, tsunami, atmospheric dust storms, climate change, drought, floods, typhoons, monsoons, space weather, and planetary exploration.” Bulletin of the American Meteorological Society

The international Hinode mission was launched from Japan on 23 September 2006. The spacecraft carries a suite of instruments that permit observations of the Sun and its atmosphere with unprecedented resolution and precision. During its first two years of operation, Hinode has enabled numerous breakthroughs in our understanding of magnetic fields within the solar atmosphere and their relationship to the energetic solar phenomena that affect the Earth's space environment. Some of those breakthroughs were presented at the First Hinode Science Meeting held in Dublin, Ireland, in August 2007 (ASPCS Volume 397). By the time the Second Hinode Science Meeting was held in Boulder, Colorado, 29 September-3 October 2008, researchers had been able to subject Hinode data to in-depth, quantitative analyses and to make comparisons with detailed numerical and analytic models of solar phenomena. This volume presents brief summaries of work presented at the Second Hinode Science Meeting.