Dust Properties in the Local Interstellar Medium

被引：0
|
作者：
Ingrid Mann
Hiroshi Kimura
机构：
[1] ESA Space Science Department-ESTEC,Institut für Planetologie
[2] Westfälische Wilhelms-Universität,undefined
[3] Max-Planck-Institut für Aeronomie,undefined
来源：
Space Science Reviews | 2001年 / 97卷
关键词：
Dust; Amorphous Carbon; Radiation Pressure; Interstellar Dust; Local Interstellar Medium;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
Ulysses measurements yield reliable in-situdetection of large dust particles which stem from the interstellar medium (ISM) and which are not observed in interstellar extinction data. Both current models of large grains in the ISM: core-mantle grains as well as composite grains, are in agreement with dust properties implied by the Ulysses results. However, the size of particles detected by Ulysses still exceeds the size of the large grains that are predicted for the ISM.
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页码：389 / 392
页数：3
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