Dynamical simulation of the motion of Leonid meteoric stream
Li, GY; Zha, HB
刊名INTERNATIONAL JOURNAL OF MODERN PHYSICS D
2002-08-01
卷号11期号:7页码:1021-1034
关键词COMET TEMPEL-TUTTLE
ISSN号0218-2718
英文摘要The Leonid meteoric shower has been the most famous meteoric shower. The main characteristics of the stream are well known, being very spectacular displays in recent years. In this paper, the authors aim at searching the dynamic origin of the second peak of Leonids 1998. Firstly a dynamic model of the solar system is constructed, considering the perturbations of the nine major planets and the Moon, Post-Newtonian effects and the figure effect of the Earth. For the motions of comet and meteoroid, the non-gravitational effect and radiation pressure effect are taken into account separately. Secondly, the orbit of Comet Tempel-Tuttle is determined by using the observation data of this apparition. Finally, assuming an isotropic ejection model of comet, the authors simulate the motion of the meteoric stream and discover that the particles aged 2-revolutions erupted with velocity 50 m/s can befall Earth at 20h37m UT of Nov. 17, 1998, which form the main part of the second peak of Leonids 1998.
学科主题Astronomy & Astrophysics
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]COMET TEMPEL-TUTTLE
收录类别ISTP ; SCI
语种英语
WOS记录号WOS:000178117100007
公开日期2013-01-29
内容类型期刊论文
源URL[http://libir.pmo.ac.cn/handle/332002/7794]  
专题紫金山天文台_盱眙天文观测站
作者单位1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
推荐引用方式
GB/T 7714
Li, GY,Zha, HB. Dynamical simulation of the motion of Leonid meteoric stream[J]. INTERNATIONAL JOURNAL OF MODERN PHYSICS D,2002,11(7):1021-1034.
APA Li, GY,&Zha, HB.(2002).Dynamical simulation of the motion of Leonid meteoric stream.INTERNATIONAL JOURNAL OF MODERN PHYSICS D,11(7),1021-1034.
MLA Li, GY,et al."Dynamical simulation of the motion of Leonid meteoric stream".INTERNATIONAL JOURNAL OF MODERN PHYSICS D 11.7(2002):1021-1034.
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