スポンサーリンク
Kwasan and Hida Observatories, Kyoto University | 論文
- Internal Fine Structure of Ellerman Bombs
- Energetic Relations between the Disappearing Solar Filaments and the Associated Flare Arcades
- Slow and Fast MHD Shocks Associated with a Giant Cusp-Shaped Arcade on 1992 January 24
- Suzaku Observation of the Ophiuchus Galaxy Cluster : One of the Hottest Cool Core Clusters
- HZE particle and neutron dosages from cosmic rays on the lunar surface (Proceedings of the international workshop on advances in cosmic ray science)
- Spatial Distribution of the Galactic Center Diffuse X-Rays and the Spectra of the Brightest 6.4keV Clumps
- Time Variability of the Neutral Iron Lines from the Sagittarius B2 Region and Its Implication of a Past Outburst of Sagittarius A
- Horizontal and Vertical Flow Structure in Emerging Flux Regions
- A Super Bubble Candidate in the Galactic Center and a Local Enhancement G359.77-0.09
- Three-Dimensional Simulation of Solar Emerging Flux Using the Earth Simulator : I. Magnetic Rayleigh-Taylor Instability at the Top of the Emerging Flux as the Origin of Filamentary Structure
- Three-Dimensional Magnetohydrodynamic Numerical Simulations of Coronal Loop Oscillations Associated with Flares
- Spectroscopic Studies of the Solar Corona : III. Density Diagnostics Using the Infrared Lines of Fe XIII
- Spectroscopic Studies of the Solar Corona : II. Properties of Green and Red Emission Lines in Open and Closed Coronal Structures
- Spectroscopic Studies of the Solar Corona I. Spatial Variations in Line Parameters of Green and Red Coronal Lines
- Ca II K Spectral Study of an Emerging Flux Region using the Domeless Solar Telescope in Hida Observatory
- Height Dependence of Gas Flows in an Ellerman Bomb
- X-Ray Expanding Features Associated with a Moreton Wave
- Real-Time Frame Selector and its Application to Observations of the Horizontal Velocity Field in the Solar Photosphere
- Eruptive and Quasi-Eruptive Disappearing Solar Filaments and Their Relationship with Coronal Activities
- Relation between a Moreton Wave and an EIT Wave Observed on 1997 November 4