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Theoretical and numerical study on Jovian atmospheres:their dynamics, matetialtrensport, and energetics.

Theoretical and numerical study on Jovian atmospheres:their dynamics, matetialtrensport, and energetics.
木星大气的理论和数值研究:它们的动力学、物质运动和能量学。
批准号:
16204036
负责人:
HAYASHI Yoshi-yuki
金额:
$29.37万
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (A)
财政年份:
2004
资助国家:
日本
项目状态:
已结题
起止时间:
2004 至 2007

项目摘要

项目成果

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中文摘要
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英文摘要
For the purpose of investigating the interplay among dynamical, thermal, and compositional structures of the atmospheres of Jovian planets, we compiled the current status of corresponding knowledge, developed a hierarchical modeling system, and conducted numerical experiments with those hierardical modeling systems. The main findings of our investigations are summarized as follows:1. We developed a vertical one-dimensional equilibrium cloud condensation model, which enable us to cover possible atmospheric compositional varieties of the Jovian planets. We found that the contributions to the intensity of stability by the cloud layers associated with the condensation of NH_3 and formation of NH_4SH are not negligible compared with that of H_2O.2. We developed a two-dimensional cloud convection model incorporating the condensation of NH_3 and H_2O and formation of NH_4SH. We conducted a series of numerical experiments, and found that the H_2O condensation level acts as a distinct dynamical … More boundary that separates the convective motions above and below it. The stable layers due to NH_3 and NH_4SH clouds cannot suppress the cloudy plumes driven by H_2O condensation healing, resulting in the mixing over the full depth of the atmosphere above the H_2O condensation level.3. With the application to the Jovian atmosphere in mind, we performed a series of numerical studies on the equatorial acceleration using the three dimensional Bousinesq spherical shell convection model. We found that a strong stable layer in the outer layer helps the development of equatorial retrograde jet. This result may raise a question about the theory where rotating spherical thermal convection explains the cause of the equatorial westerly jets of Jupiter and Saturn.4. A common software infrastructure, over which those numerical models were constructed, was developed. It contains "gt4f90io" which is a library for I/O of numerical data, and "Rdoc" which is an automatic documentation generator for numerical model codes. We also organized a standard style of Fortran90 programming and constructed a library of Fortran90 functions for basic mathematical manipulations, with which we developed 'Spmodel" which is a set of spectral models. All of the softwares mentioned are open to public on our web site. Less
期刊论文(50)
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Meteorology of Jupiter
木星的气象学
DOI: --
发表时间: 2005
期刊: Astronomical Herald 98
影响因子: --
作者: [Nakajima, K]
通讯作者: K
Monitoring of Atmospheric Dynamics by Jupiter Orbiter
木星轨道飞行器监测大气动力学
DOI: --
发表时间: 2007
期刊:
影响因子: --
作者: [Takahashi, Y., Nakajima, K., Sakanoi, T., Sugiyama, K., Takeuchi, S., Imamura, T., Satoh, T.]
通讯作者: T.
Design and implementation test of a general circulation model with flexible and readable code: design of physical process module
代码灵活可读的总体循环模型的设计与实现测试:物理过程模块设计
DOI: --
发表时间: 2007
期刊:
影响因子: --
作者: [Morikawa,Y., Ishiwatari,M, Takahashi, Y.-O-, Odaka, M., Hayashi, Y.-Y]
通讯作者: Y.-Y
Rossby waves and jets in a two-dimensional decaying turbulence on a rotating sphere.
旋转球体上二维衰减湍流中的罗斯贝波和射流。
DOI: --
发表时间: 2007
期刊: Journal of the Atomospheric Sciences 64-12
影响因子: --
作者: [Y. Saiki, M. Yamada, 田中勝, M. Yamada, 内田真勝, Y. -Y. Hayashi]
通讯作者: Y. -Y. Hayashi
43
    Research on the representation of precipitation structure in general circulation models based on the results of the Aqua-Planet Experiment Project
    • 批准号:
      21340139
    • 项目类别:
      Grant-in-Aid for Scientific Research (B)
    • 资助金额:
      $7.49万
    • 财政年份:
      2009
    • 负责人:
      HAYASHI Yoshi-yuki
    • 依托单位:
    海外基金