| Project/Area Number |
03452065
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| Research Category |
Grant-in-Aid for General Scientific Research (B)
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| Allocation Type | Single-year Grants |
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| Research Field |
Space and upper atmospheric physics
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| Research Institution | KYOTO UNIVERSITY |
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Principal Investigator |
FUKAO Shoichiro Kyoto Univ./RASC,Professor, 超高層電波研究センター, 教授 (30026249)
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| Co-Investigator(Kenkyū-buntansha) |
YAMAMOTO Mamoru Kyoto Univ./RASC,Instructor, 超高層電波研究センター, 助手 (20210560)
YAMANAKA Manabu Kyoto Univ./RASC,Lecturer, 超高層電波研究センター, 講師 (30183982)
SATO Toru Kyoto Univ./Dept.Eng., Lecturer, 工学部, 講師 (60162450)
KIKUCHI Takashi Ministry of Posts and Telecommunications/CRL,Head, 通信総合研究所, 研究室長
菊地 崇 郵政省, 通信総合研究所, 研究室長
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| Project Period (FY) |
1991 – 1992
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| Project Status |
Completed (Fiscal Year 1992)
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| Budget Amount *help |
¥5,600,000 (Direct Cost: ¥5,600,000)
Fiscal Year 1992: ¥1,700,000 (Direct Cost: ¥1,700,000)
Fiscal Year 1991: ¥3,900,000 (Direct Cost: ¥3,900,000)
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| Keywords | Ionospheric structure / Thermospheric structure / Seasonal variation / Solar activity dependence / Ion drift velocity / Thermospheric meridional circulation / Gravity waves / F-region peak / 中緯度電離圏F領域 / ISレ-ダ-観測 / 電子密度勾配 / TID / 内部重力波 / 地磁気擾乱 |
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| Research Abstract |
The principal results are summarized as follows. (i) Ionospheric/thermospheric seasonal behavior-four years of MU radar data are analyzed to understand the seasonal variations, solar activity dependence, and magnetic activity behavior of the electron and ion density and temperature. Based on these data, the thermospheric temperatures and densities are derived. The temperatures are consistently lower than existing model values by 2-156 K,depending upon solar activity and season. (ii) The seasonal behavior of F-region electron density is investigated in detail. (iii) Seasonal behavior of ion-drift velocities-MU radar observations of electric fields during September 1986 to January 1991 are investigated in the form of time-of-day variations for several different seasonal and solar-activity cases. The maximum daily amplitudes and the time-of-day and solar activity trends at the MU and the Arecibo radar locations have strong resemblances. However the seasonal trends in the MU data, the Arec
… More
ibo data, and existing radar models disagree strongly. Currently, the thermospheric meridional winds are being investigated from these results. (iv)Mid-latitude ionospheric disturbances-over 500 hours of multiple-beam radar observations are analyzed. During magnetically disturbed times the traveling disturbances are very predominantly equatorward, indicating an auroral wave source, while during quiet times all wave directions are observed, indicating a local, lower-atmosphere source. (v) Ionospheric structure during the low-latitude auroral event of 20-23 October 1989-during the first auroral display over Japan since 1960, extreme spatial and temporal gradients are observed in four oblique beams. This observation calls into doubt the validity of the monostatic, sequential-three-position, vector velocity measurement often made by radars.
All of these results are essentially "local" investigations overhead from the MU radar. It strongly hoped that further efforts will be made in the near future to expand these studies to consider "non-local" phenomena related to global forcing mechanisms. Less
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