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Serial optical observation of Jovian plasma processes at the summit of Mauna Kea in Hawaii

Serial optical observation of Jovian plasma processes at the summit of Mauna Kea in Hawaii
在夏威夷莫纳克亚山山顶对木星等离子体过程的连续光学观测
批准号:
11691115
负责人:
MORIOKA Akira
金额:
$4.22万
依托单位:
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (B).
财政年份:
1999
资助国家:
日本
项目状态:
已结题
起止时间:
1999 至 2000

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中文摘要
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英文摘要
The study, 2-dimensional imaging observations of the D-line emission distribution of logenic sodium atoms, which is regarded as a tracer of logenic volcanic gases, were performed with two field of views (FOV), namely±20Rj (narrow FOV ; Rj : Jovian radius), and ±400Rj (wide FOV). From the observational results, the following characteristics of emission distribution were obtained. In the narrow FOV observation, two different types of distribution extending to〜20Rj, that is, the band-shaped distribution and the spray-shaped distribution, were observed simultaneously. In the wide FOV observation, the elongated oval-like emission distribution extended to as much as 400Rj along the equatorial plane was observed. The east-west intensity asymmetry was also observed, with a dependence on the Io phase angle.Based on the observed images , we then made model analyses to investigate supply processes of sodium atoms and time variation of sodium distribution, and presented the comprehensive source process which can consistently reproduce the observed characteristics both in the narrow and wide FOV observation.From the model analysis for the narrow FOV observational results, it is concluded that the band-shaped distribution is attributed to the molecular ion destruction process, and the typical gyrovelocity of the molecular ions is estimated to be 20km/sec. It is also concluded that the spray-shaped distribution is produced through the charge exchange process. Then a combination of the two processes was examined for the wide FOV observational results. The combined model analysis could fairly reproduce the observed features of the wide extended sodium distribution. In the course of the model analysis, some important physical processes and related parameters are suggested.
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Nozawa, H.: "Variability of SII emission from the Io plasma torus"Adv.Space Res.. Vol.26, No.10. 1529-1532 (2000)
Nozawa, H.:“Io 等离子体环面 SII 发射的变化”Adv.Space Res.。第 26 卷,第 10 期。
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Takahashi,S.: "Distribution of sodium cloud near Io and in the inner Jovian magnetosphere"Advanced Space Research. 26. 1529-1532 (2000)
Takahashi,S.:“木卫一附近和木星内部磁层中钠云的分布”高级空间研究。
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Sakanoi, T.: "Observations of Vertical Winds in the Thermosphere with a Fabry-Perot Doppler Imager at Syowa Station, Antarctica"Adv.Space Res.. Vol.24, No.11. 1439-1442 (2000)
Sakanoi, T.:“在南极洲昭和站使用法布里-珀罗多普勒成像仪观测热层中的垂直风”Adv.Space Res.。第 24 卷,第 11 期。
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Nakagawa,F.: "On the sources of Jovian hectometric radiation"Advanced Space Research. 26. 1525-1528 (2000)
Nakakawa,F.:“关于木星百米辐射源”高级空间研究。
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28
    Acceleration and dynamics of energetic particles in the Jovian magnetosphere
    • 批准号:
      12440129
    • 项目类别:
      Grant-in-Aid for Scientific Research (B)
    • 资助金额:
      $8.06万
    • 财政年份:
      2000
    • 负责人:
      MORIOKA Akira
    • 依托单位:
    Study on Jupiter's inner magnetosphere by the observation of Jovian synchrotron radiation
    • 批准号:
      09440171
    • 项目类别:
      Grant-in-Aid for Scientific Research (B)
    • 资助金额:
      $7.36万
    • 财政年份:
      1997
    • 负责人:
      MORIOKA Akira
    • 依托单位:
    海外基金