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Kazunari Shibata
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Reizaburo Kitai
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Satoru UeNo
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Daisaku Nogami
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Takako T. Ishii
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Miwako Katoda
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Yoko Nasuji
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Mai Kamobe
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Naoki Kaneda
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Hiroyuki Komori
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Shozo Yagi
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Ayumi Asai
(Unit of Synergetic Studies for Space, Kyoto University)
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Reizaburo Kitai
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Satoru UeNo
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Daisaku Nogami
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Takako T. Ishii
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Miwako Katoda
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Yoko Nasuji
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Mai Kamobe
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Naoki Kaneda
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Hiroyuki Komori
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Shozo Yagi
(Kwasan & Hida Observatories, Graduate School of Science, Kyoto University)
Ayumi Asai
(Unit of Synergetic Studies for Space, Kyoto University)
Introduction
Chapter1 Solar Research and the Terrestrial Environment
1.1Basics of Solar Observation
1.2Impacts of the Sun on the Earth
Chapter2 Flare Monitoring Telescope
2.1Telescope Observation System and Public Data Release
2.2Photographic Records of the FMT Before and After its Relocation to Peru
Chapter 3 Solar Full-disk Hα Observations in the World
3.1Solar Hα Full-disk Observation
3.2Solar Full-disk Observation in Other Wavelengths
Chapter 4 Summary of the Observations Carried Out over a Period of 11 Years
4.1Flare
4.2Surge
4.3Prominence
4.4Filament Activity
4.5Moreton Waves
Chapter 5 Event Lists
5.1Active Phenomena in Hα−0.8Å(Disk Events)
5.2Active Phenomena in Prominence Images (Limb Events)
Chapter 6 Representative Events
6.1General Descriptions of the Illustrations
6.2Representative Disk Events
6.3Representative Limb Events (Prominences)
Appendix A Selected Papers Relating to FMT
A-1Morimoto & Kurokawa, “A Method for the Determination of 3-D Velocity Fields of Disappearing Solar Filaments,” 2003
A-2Morimoto & Kurokawa, “Eruptive and Quasi-Eruptive Disappearing Solar Filaments and Their Relationship with Coronal Activities,” 2003
A-3Eto et al., “Relation between a Moreton Wave and an EIT Wave Observed on 1997 November 4,” 2002
A-4Narukage et al., “SIMULTANEOUS OBSERVATION OF A MORETON WAVE ON 1997 NOVEMBER 3 IN Hα AND SOFT X-RAYS,” 2002
A-5Narukage et al., “X-Ray Expanding Features Associated with a Moreton Wave,” 2004
A-6Morimoto et al., “Energetic Relations between the Disappearing Solar Filaments and the Associated Flare Arcades,” 2010
Appendix B FMT-Related Papers
Appendix C FMT-Related Reports in Proceedings of the Symposiums of Solar-
Terrestrial Energy Program(STEP)
Afterword
INDEX
Chapter1 Solar Research and the Terrestrial Environment
1.1Basics of Solar Observation
1.2Impacts of the Sun on the Earth
Chapter2 Flare Monitoring Telescope
2.1Telescope Observation System and Public Data Release
2.2Photographic Records of the FMT Before and After its Relocation to Peru
Chapter 3 Solar Full-disk Hα Observations in the World
3.1Solar Hα Full-disk Observation
3.2Solar Full-disk Observation in Other Wavelengths
Chapter 4 Summary of the Observations Carried Out over a Period of 11 Years
4.1Flare
4.2Surge
4.3Prominence
4.4Filament Activity
4.5Moreton Waves
Chapter 5 Event Lists
5.1Active Phenomena in Hα−0.8Å(Disk Events)
5.2Active Phenomena in Prominence Images (Limb Events)
Chapter 6 Representative Events
6.1General Descriptions of the Illustrations
6.2Representative Disk Events
6.3Representative Limb Events (Prominences)
Appendix A Selected Papers Relating to FMT
A-1Morimoto & Kurokawa, “A Method for the Determination of 3-D Velocity Fields of Disappearing Solar Filaments,” 2003
A-2Morimoto & Kurokawa, “Eruptive and Quasi-Eruptive Disappearing Solar Filaments and Their Relationship with Coronal Activities,” 2003
A-3Eto et al., “Relation between a Moreton Wave and an EIT Wave Observed on 1997 November 4,” 2002
A-4Narukage et al., “SIMULTANEOUS OBSERVATION OF A MORETON WAVE ON 1997 NOVEMBER 3 IN Hα AND SOFT X-RAYS,” 2002
A-5Narukage et al., “X-Ray Expanding Features Associated with a Moreton Wave,” 2004
A-6Morimoto et al., “Energetic Relations between the Disappearing Solar Filaments and the Associated Flare Arcades,” 2010
Appendix B FMT-Related Papers
Appendix C FMT-Related Reports in Proceedings of the Symposiums of Solar-
Terrestrial Energy Program(STEP)
Afterword
INDEX
DVD-ROM