The CODAG sounding rocket experiment to study aggregation of thermally diffusing dust particles

被引：8

作者：

Blum, J

Wurm, G

Poppe, T

机构：

[1] Univ Jena, Inst Astrophys, D-07745 Jena, Germany

[2] Univ Jena, Observ, D-07745 Jena, Germany

来源：

EXPLORATION OF SMALL BODIES IN THE SOLAR SYSTEM: RELATED LABORATORY AND MODELLING STUDIES | 1999年 / 23卷 / 07期

关键词：

D O I：

10.1016/S0273-1177(99)00195-7

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The initial step of planetesimal formation in the solar nebula is due to a low velocity, Brownian motion induced aggregation process of the pre-planetary dust particles. Tn order to reveal the physics of such agglomeration processes, e.g. sticking efficiency, temporal evolution of cluster mass distribution, and morphology of the (fractal) dust aggregates, we developed the simulation experiment CODAG-SRE for ESA's MASER 8 sounding rocket flight (launch April/May 1999) which is described in this article. (C) 1999 COSPAR. Published by Elsevier Science Ltd.

引用

页码：1267 / 1270

页数：4