Development of comet nucleus simulation experiments
彗核模拟实验进展
基本信息
- 批准号:10554027
- 负责人:
- 金额:$ 9.79万
- 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:1998
- 资助国家:日本
- 起止时间:1998 至 1999
- 项目状态:已结题
- 来源:
- 关键词:
项目摘要
We have developed new methods for making amorphous icy grains:1 ) CO sublimation-induced disruption methodFirst, we deposited CO sample of 10 mm thickness. Second, thin film of amorphous water ice was deposited on the CO. After deposition, the substrate was heated by turning off the helium refrigerator. At temperatures around 30 K, corresponding to CO sublimation temperatures, the sublimation of CO occurred violently, and this caused the disruption of the thin film of amorphous water ice.2) Continuous production method by fast codeposition of HィイD22ィエD2O and COィイD22ィエD2.We found that continuous disruption of ice film occurred during the deposition , when deposition rate is larger than 3x10ィイD1-9ィエD1 m/s and when thickness of the film is larger than critical thickness.In both method, we collected amorphous icy grains falling from the substrate using grain collector. These methods enables us to perform better comet nucleus simulation experiments than hitherto performed.
我们发展了制备非晶冰粒的新方法:1)CO升华诱导破裂法首先,我们沉积了10 mm厚的CO样品。其次,在CO上沉积无定形水冰薄膜。沉积后,通过关闭氦制冷机来加热衬底。在30 K左右,CO升华温度附近,CO发生剧烈的升华,导致非晶水冰薄膜的破裂; 2)H_(22)O_(22)的快速共沉积连续制备方法。当沉积速率大于3 × 10 ~(-1)D_1 -9 × 10 ~(-1)D_1 m/s和薄膜厚度大于临界厚度时,两种方法都是利用颗粒收集器收集从衬底上脱落的非晶冰粒。这些方法使我们能够进行更好的彗星核模拟实验比迄今为止进行。
项目成果
期刊论文数量(18)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
Jepiskinns,P.,D.F.Blake and A.Kouchi: "Amorphous water ice- A solar system material" Solar System Ices. 139-155 (1998)
Jepiskinns,P.,D.F.Blake 和 A.Kouchi:“非晶水冰 - 太阳系材料”太阳系冰。
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- 影响因子:0
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- 通讯作者:
Arakawa, M.: "Collisional disruption of ice by high velocity impact" Proc.31th ISAS Lunar and Planetary Symp.13-16 (1998)
Arakawa, M.:“高速撞击对冰的碰撞破坏”Proc.31th ISAS Lunar and Planetary Symp.13-16 (1998)
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- 影响因子:0
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Kouchi, A., et al.: "Crystallization Heat of Impure Amorphous H_20 Ice"Geophys. Res. Lett. in press
Kouchi, A. 等人:“不纯非晶态 H_20 冰的结晶热”Geophys。
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Kouchi A.et al.: "New methods for making amorphous icy grains for comet nucleus simulation experiments"Proc.32nd ISAS Lunar and Planetary Symp.. 121-124 (1999)
Kouchi A.等人:“为彗星核模拟实验制作非晶冰粒的新方法”Proc.32nd ISAS Lunar and Planetary Symp.. 121-124 (1999)
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- 影响因子:0
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香内晃: "宇宙のアモルファス物質"応用物理. 68. 1179-1180 (1999)
Akira Kanai:“宇宙中的无定形物质”应用物理学 68. 1179-1180 (1999)。
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KOUCHI Akira其他文献
KOUCHI Akira的其他文献
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{{ truncateString('KOUCHI Akira', 18)}}的其他基金
Observation of surface structure of amorphous ice and role of amorphous ice in surface atomic reactions at low temperatures
非晶冰表面结构观察及非晶冰在低温表面原子反应中的作用
- 批准号:
22340157 - 财政年份:2010
- 资助金额:
$ 9.79万 - 项目类别:
Grant-in-Aid for Scientific Research (B)
Evaluation of catalytic effect of amorphous ice on the surface atomic reactions
非晶冰对表面原子反应的催化效果评价
- 批准号:
17104006 - 财政年份:2005
- 资助金额:
$ 9.79万 - 项目类别:
Grant-in-Aid for Scientific Research (S)
UV-induced diamond formation in interstellar clouds
星际云中紫外线诱导钻石形成
- 批准号:
15340180 - 财政年份:2003
- 资助金额:
$ 9.79万 - 项目类别:
Grant-in-Aid for Scientific Research (B)
Collisional sticking of organic grains in the solar nebula
太阳星云中有机颗粒的碰撞粘附
- 批准号:
12440142 - 财政年份:2000
- 资助金额:
$ 9.79万 - 项目类别:
Grant-in-Aid for Scientific Research (B)
Chemical reaction mechanism on the surafce of interstellar icy grains
星际冰粒表面化学反应机制
- 批准号:
07454128 - 财政年份:1995
- 资助金额:
$ 9.79万 - 项目类别:
Grant-in-Aid for Scientific Research (B)
Material evolution simulator
材料演化模拟器
- 批准号:
05554013 - 财政年份:1993
- 资助金额:
$ 9.79万 - 项目类别:
Grant-in-Aid for Developmental Scientific Research (B)
相似海外基金
Participation in the CONSERT instrument on Rosetta in order to inform the science team of up-to- date cometary nucleus models.
参与罗塞塔上的 CONSERT 仪器,以便向科学团队通报最新的彗星核模型。
- 批准号:
ST/G002045/1 - 财政年份:2010
- 资助金额:
$ 9.79万 - 项目类别:
Research Grant
Physico-Chemical Phenomena Near the Cometary Nucleus
彗核附近的物理化学现象
- 批准号:
7033934 - 财政年份:1970
- 资助金额:
$ 9.79万 - 项目类别: