Statistical Study of Solar X-Ray Jets Observed with the Yohkoh Soft X-Ray Telescope
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概要
- 論文の詳細を見る
- Astronomical Society of Japanの論文
- 1996-02-25
著者
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Hudson H
Institute For Astronomy University Of Hawaii
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HUDSON Hugh
Institute for Astronomy, University of Hawaii
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HASHIMOTO Shizuyo
Department of Physics, Faculty of Science, Tokai University
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SHIBATA Kazunari
National Astronomical Observatory
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SHIMOJO Masumi
Department of Physics, School of Science, Tokai University
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HIRAYAMA Tadashi
National Astronomical Observatory
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ACTON Loren
Montana State University
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Acton L
Montana State University
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Hudson Hugh
Institute For Astronomy University Of Hawaii
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Shimojo Masumi
Department Of Physics School Of Science Tokai University
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Hashimoto S
Department Of Physics School Of Science Tokai University
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Hashimoto Shizuyo
Department Of Physics Faculty Of Science Tokai University
関連論文
- The Solar Flare of 1992 August 17 23 : 58 Ut
- Magnetic Reconnection as the Origin of Galactic-Ridge X-Ray Emission
- Statistical Study of Solar X-Ray Jets Observed with the Yohkoh Soft X-Ray Telescope
- Disk Accretion onto a Magnetized Young Star and Associated Jet Formation
- Hard X-Ray Sources and the Primary Energy-Release Site in Solar Flares
- Coronal X-Ray Jets Observed with the Yohkoh Soft X-Ray Telescope
- Dynamics of Local Isolated Magnetic Flux Tubes in a Rapidly Rotating Stellar Atmosphere
- Linear and Nonlinear Evolution of the Parker Instability of Magnetic-Flux Sheets in Co-Rotating Coordinates
- Measurement of Electron Temperature and Density in Laser-Produced Al Plasma
- Numerical Simulation of Solar Coronal X-Ray Jets Based on the Magnetic Reconnection Model
- Preflare Heating and Mass Motion in a Solar Flare Associated with Hot Plasma Ejection : 1993 November 11 C9.7 Flare
- Measurement of Electron Densities of Hydrogen and Helium Plasmas
- Measurements of Line Profiles of Argon Plasma withe Self-Absorption in Vacuum Ultraviolet Region
- Stark Shifts of Ionized Helium Lines
- Measurements of the Stark Shifts of Singly Ionized Argon Lines
- Calculation of the Line-Positions and the Relative Intensities of Fine-Structure Components for HeII 3s, p, d-5s, p, d. f Line Complex