Mathematical modelling of the Geminid meteoroid stream

被引：51
|
作者：
Ryabova, G. O. [1 ]
机构：
[1] Tomsk VV Kuibyshev State Univ, Res Inst Appl Math & Mech, Tomsk 634050, Russia
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2007年 / 375卷 / 04期
关键词：
meteors; meteoroids;
D O I：
10.1111/j.1365-2966.2007.11392.x
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Geminid meteoroid stream formation and evolution were studied by the method of nested polynomials. The stream has two layers formed due to differences in orbital parameters of particles ejected from the cometary nucleus before and after perihelion. The shape of the model activity profiles depends on the place where the Earth passes the stream. The importance of observations for calibration of the model is discussed.
引用
收藏
页码：1371 / 1380
页数：10
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