Dynamical response of the stratosphere to the solar forcing

平流层对太阳强迫的动态响应

• 批准号: 15340159
• 负责人: KODERA Kunihiko
• 金额: $ 6.78万
• 依托单位: Meteorological Research Institute, Japan Meteorological Agency (JMA)
• 依托单位国家: 日本
• 项目类别: Grant-in-Aid for Scientific Research (B)
• 财政年份: 2003
• 资助国家: 日本
• 起止时间: 2003 至 2004
• 项目状态: 已结题
• 来源: https://kaken.nii.ac.jp/en/grant/KAKENHI-PROJECT-15340159/
• 关键词: Solar influence; International cooperation; Climate chance; Solar UV; Ozone; Stratosphere; Meridional circulation; General circulation; 国際研究者交流; 中層大気

Total solar irradiance (TSI) measurements by satellites revealed that the variation in the TSI is only about 0.1%, which is too small to produce any meaningful climatic effects. The ultra-violet part of the solar spectrum shows larger (3-8%) variation and may possible to produce a change in stratospheric circulation. However, such processes involving highly non-linear responses are difficult to identify sole from the observation or by a particular general circulation model studies.Accordingly, the present study is conducted as a part of an international cooperative study "General Circulation Model Reality Intercomparison Project for SPARC (GRIPS)". In particular, comparison with the Free University of Berlin model as well as observational data, was conducted to elucidate the processes how the solar influence produced in the winter stratopause region can penetrate down to the Earth's surface.The solar heating in the stratosphere is closely related with the production and destruction of the ozone, so that it is also important to understand the variation of chemical species. To investigate the solar effect on ozone, we conducted a chemical climate model study by imposing the observed solar spectrum variation and wind field.The results of the present study demonstrate that the solar influence created in the stratopause region by change in solar irradiance and ozone concentration comes down to the troposphere by two processes through i) change in the wave mean-flow interaction in higher latitudes of the winter hemisphere and ii) change in mean meridional (or Brewer-Dobson) circulation induced by the abovementioned wave mean-flow interactions.From these two processes the mechanism of the solar influence on the North Atlantic Oscillation and the Indian Monsoon activity is explained.

卫星测量的太阳总辐照度（TSI）显示，TSI的变化只有0.1%左右，这是太小了，产生任何有意义的气候影响。太阳光谱的紫外线部分显示出较大的变化（3-8%），可能会引起平流层环流的变化。然而，这样的过程涉及高度非线性的响应是很难识别的观察或通过一个特定的大气环流模式研究，因此，本研究是作为一个国际合作研究的一部分“大气环流模式现实相互比较项目（GRIPS）”。特别是与柏林自由大学模式和观测资料的比较，阐明了冬季平流层顶产生的太阳影响如何向下穿透到地球表面的过程，平流层的太阳加热与臭氧的产生和破坏密切相关，因此了解化学物种的变化也很重要。为了研究太阳对臭氧的影响，利用观测到的太阳光谱变化和风场进行了一个化学气候模式的研究，结果表明，太阳辐射和臭氧浓度的变化在平流层顶产生的影响通过两个过程到达对流层：（1）波平均的变化，冬季半球高纬度气流相互作用和ii）平均纬向变化（或Brewer-Dobson）环流由上述波平均值引起-从这两个过程出发，分析了太阳对北大西洋涛动和印度季风活动的影响机制，解释道

项目成果

Simulation of radiative and dynamical resoponses of the middle atmosphere to the 11-year solar cycle

中层大气对11年太阳周期的辐射和动力学响应的模拟

• 发表时间: 2005
• 期刊: J. Atmos. Solar-Terr. Phys. 67
• 作者: Shibata;K.;K.Kodera
• 通讯作者: K.Kodera

Simulation of radiative and dynamical responses of the middle atmosphere to the 11-year solar cycle

中层大气对11年太阳周期的辐射和动力学响应的模拟

• 发表时间: 2005
• 期刊: J. Atmos. Solar-Terr. Phys. 67
• 作者: Shibata;K.;K.Kodera
• 通讯作者: K.Kodera

Matthes, Langematz, Gray, Kodera, Labitzke: "Improved 11-Year Solar Signal in the FUB-CMAM"Journal of Geophysical Research. 109(D6). 10.1029/2003JD004012 (2004)

Matthes、Langematz、Gray、Kodera、Labitzke：“FUB-CMAM 中 11 年太阳信号的改进”地球物理研究杂志。

Impact of the SH major stratospheric warming on the Hadley circulation : A case study

• DOI: 10.2467/mripapers.54.111
• 发表时间: 2004
• 期刊: Papers in Meteorology and Geophysics
• 作者: K. Kodera;Kazutaka Yamada

Possible solar modulation of the ENSO cycle

• DOI: 10.2467/mripapers.55.21
• 发表时间: 2005-03
• 期刊: Papers in Meteorology and Geophysics
• 作者: K. Kodera;邦彦 小寺