教員・研究者情報
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袴田 和幸 HAKAMADA Kazuyuki

プロフィール

生年 1947
出身 静岡県
職名 教授
所属 工学部 共通教育科 教養課題教育(科学技術リテラシー)担当
最終学歴 神戸大学大学院理学研究科
学位 理学博士(名古屋大学)
所属学会・役職 地球電磁気・地球惑星圏学会
American Geophysical Union
専門分野 宇宙空間物理学、太陽圏物理学
研究テーマ コロナ磁場の三次元構造と太陽風の加速機構、宇宙天気予報の基礎研究
授業科目 基礎物理学、基礎電磁気学、力学、物理の世界、自然科学分野ゼミナール

学術論文、評論

Resolving the enigmatic solar wind disappearance event of 11 May 1999, Journal of Geophysical Research(学術雑誌), Vol.110, No.A8, A08101, 2005

Correlation between Expansion Rate of the Coronal Magnetic Field and Solar Wind Speed in a Solar Activity Cycle, Solar Physics(学術雑誌), Vol.227, No.2, pp.387-399, 2005

Origin of the slow solar wind, Adv. Space Research(学術雑誌), Vol.33, PP.689-695, 2004

Polar low-speed solar wind reappeared at the solar activity maximum of cycle 23, Geophysical Research Letters(学術雑誌), Vol.30, No.7, pp.62-1 - 62-4, 2003

太陽風速度とコロナ磁場膨張率の長周期変動、情報科学リサーチジャーナル(大学・研究所等紀要), Vol.10, pp.57-66, 2003

Solar wind speed and expansion rate of the coronal magnetic field in solar maximum and minimum phases, Solar Physics(学術雑誌), Vol.207, pp.173-185, 2002

太陽風加速機構の解明―太陽風速度とコロナ磁場膨張率との相関―、情報科学リサーチジャーナル(大学・研究所等紀要), Vol.9, pp.49-64, 2002

Polar low-speed solar wind at the solar activity maximum, Journal of Geophysical Research(学術雑誌), Vol.106, No.A11, pp.24923-24935, 2001

Latitudinal vecocity structures up to the solar poles estimated from interplanetary scintillation tomography analysis, Journal of Geophysical Research(学術雑誌), Vol.106, No.A8, pp.15677-15686, 2001

太陽活動極大期および極小期における太陽風速度とコロナ磁場膨張率、情報科学リサーチジャーナル(大学・研究所等紀要), Vol.8, pp.67-76, 2001

Low-speed solar wind associations with active regions near solar minimum, Advanced Space Research(学術雑誌), Vol.25, No.9, pp.1893-1896, 2000

太陽風の加速機構の解明-トモグラフィーによる太陽風速度分布の推定とポテンシャルモデルを用いた太陽表面への射影、情報科学リサーチジャーナル(大学・研究所等紀要), Vol.7, pp.27-38, 2000

コンピュータリテラシー教育の現状、情報リサーチジャーナル(大学・研究所等紀要), Vol.7, pp.73-78, 2000

Solar wind speed and expansion rate of the coronal magnetic field during Carrington rotation 1909, Solar Physics(学術雑誌), Vol.187, pp.115-122, 1999

The highest solar wind veolocity in a polar region estimated from IPS tomography analysis, Space Science Review(学術雑誌), Vol.87, pp.237-239, 1999

Low-speed solar wind from the vicinity of solar active regions, Journal of Geophysical Research(学術雑誌), Vol.104, No.A8, pp.16993-17003, 1999

Comparison of solar wind speed with coronagraph data analyzed by tomography, Solar Wind Nine(その他), pp. 565-567, 1998

Radial variation of solar wind velocity near the Sun, Solar Wind Nine(その他), pp. 313-316, 1998

Solar wind measured by interplanetary scintillation method, Solar Wind Nine(その他), pp.29-34, 1998

Three dimensional geometry of planar magnetic structure in the corona, Solar Physics(学術雑誌), Vol.181, pp.73-85, 1998

Low-speed solar wind within streamer belt form active regions, The 32nd Scientific Assembly of COSPAR(その他), 1998

Planar magnetic structures in the corona, Solar-Terrestrial Predictions V(その他), pp.650-653, 1996

A Simple method to compute spherical harmonic coefficients for the potential model of the coronal magnetic field, Solar Physics(学術雑誌), Vol.159, pp.89-96, 1995

The solar wind speed weighted along the line of sight and the intensity of He I (1083 nm) absorption line, Proceedings of the Second SOLTIP Symposium(その他), pp.117-120, 1994

Time profile of solar wind acceleration estimated by the IPS observations, Proceedings of eighth International Symposium on Solar and Terrestrial Physics(その他), 22-1 - 22-4, 1994

Solar wind speed and its acceleration inferred using the interplanetary scintillation method in carrington rotation 1753, Solar Physics(学術雑誌), Vol.153, pp.419-435, 1994

コロナ磁場の三次元構造と太陽風加速の状態、情報科学リサーチジャーナル(大学・研究所等紀要), Vol.1, pp.35-43, 1994

Solar wind observed within 0.3 AU with interplanetary scintillation, Solar Wind Seven(その他), pp.201-204, 1991

Solar wind observed within 0.3 AU using interplanetary scintillation at 327 MHz, Proceedings of the Pacific Regional STEP Conference(その他), pp.23-26, 1991

Solar wind speed and He I (1083 nm) absorption line intensity, Journal of Geophysical Research(学術雑誌), Vol.94, No.A4, pp.5397-5403, 1991

Three-dimensionla structure of the coronal magnetic field, Science Form(学術雑誌), Vol.3, pp.57-58, 1988

Three-dimensional structure of the coronal magnetic field and the solar wind speed distribution projected on the photosphere in 1974, Journal of Geophysical Research(学術雑誌), Vol.92, No.A5, pp.4339-4348, 1987

The three-dimensional geometry of the heliospheric current sheet, Planetary and Space Science(学術雑誌), Vol.33, No.8, pp.915-923, 1985

Spatial variation of the solar wind speed in 1976 and 1977, Memoirs of Nationa Institute of Polar Research Special Issue No.36(大学・研究所等紀要), pp.232-237, 1985

Three-dimensional structure of the solar wind in 1974, Proceedings of the US-Japan Seminor(その他), pp.19-24, 1984

Influence of the heliospheric current sheet on the Swinson's type north-south anisotropy of cosmic rays, Proceedings of the International Symposium on Cosmic Ray Modulation in the Heliosphere(その他), pp.1-7, 1984

A Cause of the solar wind speed variations : An Update, Journal of Geophysical Research(学術雑誌), Vol.89, No.A1, pp.357-361, 1984

Solar wind disturbances caused by solar flares: equatorial plane, Planetary and Space Science(学術雑誌), Vol.31, No.12, pp.1435-1458, 1983

Cosmic ray north-south asymmetry related with the latitudinal angular distance of the Earth from the heliospheric current sheet, Proceedings of the 18th International Cosmic Ray Conference(その他), Vol.3, pp.358-361, 1983

Solar wind distrubances in the outer heliosphere, caused by six successive solar flares from the same active region, Geophysical Research Letters(学術雑誌), Vol.10, No.7, pp.577-579, 1983

Simulation of three-dimensional solar wind disturbances and resulting geomagnetic storms, Space Science Reviews(学術雑誌), Vol.31, pp.3-70, 1982

Magnetic field configuration of the heliosphere and spiral galaxies, The Astrophysical Journal(学術雑誌), Vol.253, pp.552-555, 1982

A cause of solar wind speed variations observed at 1 A.U., Journal of Geophysical Research(学術雑誌), vol.86, No.A3, pp.1290-1298, 1981

Geomagneitc activity at the time of heliospheric current sheet crossings, Geophysical Research Letters(学術雑誌), Vol.7, No.9, pp.653-656, 1980

Empirical formula to relate the auroral electrojet intensity with interplanetary parameters, Planetary and Space Science(学術雑誌), Vol.28, pp.803-813, 1980

Influence of the east-west component of the interplanetary magnetic field on the intensity of the auroral electrojet, Planetary and Space Science(学術雑誌), Vol.28, pp.29-39, 1980

Time profile of Forbush decreases and their relation to the structure of the interplanetary magnetic filed, Proceedings of the 16th International Cosmic Ray Conference(その他), MG4-7, Vol.3, pp.146-151, 1979

Effect of the north-south component of the interplanetary magnetic field on the solar diurnal variation of the cosmic ray intensity, Memoirs of Chubu Institute of Technology(大学・研究所等紀要), Vol.13-A, pp.177-181, 1977

North-south asymmetry of the diurnal variation of the geomagnetic disturbance and the polarity of the interplanetary magnetic field, Memoirs of Chubu Institue of Technology(大学・研究所等紀要), Vol.11-A, pp.121-126, 1975

Effects of solar wind parameters on the development of magnetospheric substorms, Planetary and Space Science(学術雑誌), Vol.23, pp.75-91, 1975

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