Structure of the zodiacal cloud: new analytical and numerical solutions

N. Gorkavyi; L. Ozernoy; J. Mather; T. Taidakova

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Structure of the zodiacal cloud: new analytical and numerical solutions

机译：黄道云的结构：新的解析和数值解

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Recent results of analytical and numerical modelling of the interplanetary dust (IPD) distribution are described. They have been obtained with a new techniques employing the continuity equation written in the space of orbital coordinates. A 3-D structure and the corresponding 2-D slices for the IPD cloud governed by the Poynting-Robertson drag are computed in the framework of our 'reference model', accounting for almost all of the known major sources of dust (5000 asteroids and 217 comets). We discuss also the origin and structure of the 'dust bands' and the resonant ring near Earth.

机译：描述了行星际尘埃（IPD）分布的解析和数值模拟的最新结果。它们是通过使用在轨道坐标空间中编写的连续性方程的新技术获得的。由Poynting-Robertson阻力控制的IPD云的3-D结构和相应的2-D切片是在我们的“参考模型”框架内计算的，几乎涵盖了所有已知的主要尘埃来源（5000个小行星和217颗彗星）。我们还将讨论“尘埃带”的起源和结构以及地球附近的共振环。

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《Earth, planets and space: EPS》 |1998年第7期|共页
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N. Gorkavyi; L. Ozernoy; J. Mather; T. Taidakova;
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中图分类地球物理学;
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Structure of the zodiacal cloud: new analytical and numerical solutions

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