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Fracture Research Institute Graduate School Of Engineering Tohoku University | 論文
- Assessment of Effects of Pipe Surface Roughness and Pipe Elbows on the Accuracy of Meter Factors Using the Ultrasonic Pulse Doppler Method
- Substellar Companions to Evolved Intermediate-Mass Stars : HD 145457 and HD 180314
- Development of Iodine Cells for the Subaru HDS and the Okayama HIDES : I. Instrumentation and Performance of the Spectrographs
- Iodine-Cell Spectroscopy at Okayama Astrophysical Observatory : First Results
- Planetary Companions to Evolved Intermediate-Mass Stars : 14 Andromedae, 81 Ceti, 6 Lyncis, and HD 167042
- Planetary Companions around Three Intermediate-Mass G and K Giants : 18 Delphini, ξ Aquilae, and HD 81688
- Stellar Parameters and Photospheric Abundances of Late-G Giants : Properties of the Targets of the Okayama Planet Search Program
- Radial-Velocity Variability of G-Type Giants : First Three Years of the Okayama Planet Search Program
- High-Dispersion Spectra Collection of Nearby F-K Stars at Okayama Astrophysical Observatory : A Basis for Spectroscopic Abundance Standards
- Development of Iodine Cells for the Subaru HDS and the Okayama HIDES : II. New Software for Precise Radial Velocity Measurements
- Development of Pulse Ultrasonic Doppler Method for Flow Rate Measurement in Power Plant Multilines Flow Rate Measurement on Metal Pipe
- ICONE11-36615 DEVELOPMENT OF PULSE ULTRASONIC DOPPLER METHOD FOR FLOW RATE MEASUREMENTS OF POWER PLANT : Multiline flow rate measurement on metal wall pipe flow
- Measurement System of Bubbly Flow Using Ultrasonic Velocity Profile Monitor and Video Data Processing Unit, (III) Comparison of Flow Characteristics between Bubbly Cocurrent and Countercurrent Flows
- Measurement System of Bubbly Flow Using Ultrasonic velocity Profile Monitor and Video Data Processing Unit, (II) Flow Characteristics of Bubbly Countercurrent Flow
- Measurement System of Bubbly Flow Using Ultrasonic Velocity Profile Monitor and Video Data Processing Unit
- Photometric Observations of an Extreme ER UMa Star, RZ Leonis Minoris
- Chemical Evolution of Zinc in the Galaxy
- Non-LTE Line-Formation and Abundances of Sulfur and Zinc in F, G, and K Stars
- Sulfur Abundances in Metal-Poor Stars Based on OAO-1.88m/HIDES Spectra
- Photospheric Abundances of Volatile and Refractory Elements in Planet-Harboring Stars
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