An incompressible stratified fluid model of Comet Shoemaker-Levy 9's collision with Jupiter
文献类型：期刊论文
| 作者 | Zhang, K ; Chen, DH; Jones, C
|
| 刊名 | CHINESE ASTRONOMY AND ASTROPHYSICS
 |
| 出版日期 | 2004-10-01 |
| 卷号 | 28期号:4页码:412-421 |
| 关键词 | comets : Shoemaker-Levy comet planets and satellite : Jupiter |
| ISSN号 | 0275-1062 |
| 英文摘要 | A linear model of Comet Shoemaker-Levy 9's collision with Jupiter is presented, in which the Jovian atmosphere is taken to be a stratified, incompressible and inviscid fluid layer and the gravity wave associated with the impacts is caused by an initial impulse. Instead of adopting an initial surface deformation, we take an initial impulsive pressure P(r, z, 0) as the initial condition. It is found that this approach is more convenient for the mathematical formulation of the problem, especially for the computation of the vertical displacement of the fluid particles and the perturbation potential energy which can then be expressed by finite Fourier sine and cosine transform of P(r, z, 0). |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | IMPACT ; WAVES |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000226493300005 |
| 公开日期 | 2012-12-22 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/7763]  |
| 专题 | 紫金山天文台_期刊（老文献） |
| 作者单位 | 1.Univ Exeter, Sch Math Sci, Exeter EX4 4QJ, Devon, England 2.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China |
| 推荐引用方式 GB/T 7714 | Zhang, K,Chen, DH,Jones, C. An incompressible stratified fluid model of Comet Shoemaker-Levy 9's collision with Jupiter[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2004,28(4):412-421. |
| APA | Zhang, K,Chen, DH,&Jones, C.(2004).An incompressible stratified fluid model of Comet Shoemaker-Levy 9's collision with Jupiter.CHINESE ASTRONOMY AND ASTROPHYSICS,28(4),412-421. |
| MLA | Zhang, K,et al."An incompressible stratified fluid model of Comet Shoemaker-Levy 9's collision with Jupiter".CHINESE ASTRONOMY AND ASTROPHYSICS 28.4(2004):412-421. |
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来源：紫金山天文台
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