彗星尘埃颗粒偏振特性的建模
天体物理学
2007-05-23 v1
摘要
总结并系统化了含尘彗星的观测数据。分析了线偏振对各种参数（相位角、波长等）的依赖关系。使用一组具有不同大小和化学成分的定向排列椭球粒子来拟合哈雷彗星观测到的线偏振和圆偏振。
引用
@article{arxiv.astro-ph/0009146,
title = {Modelling of Polarization Properties of Cometary Dust Grains},
author = {D. A. Semenov and N. V. Voshchinnikov},
journal= {arXiv preprint arXiv:astro-ph/0009146},
year = {2007}
}
备注
4 pages, 5 figures, to be published in Proceedings of International Radiation Symposium IRS 2000: Current Problems in Atmospheric Radiation, St. Petersburg, July 24-29, 2000