Photometric and Polarimetric Opposition Phenomena Exhibited by Solar System Bodies
Photometric and Polarimetric Opposition Phenomena Exhibited by Solar System Bodies
复制标题
太阳系天体表现出的光度和偏振对立现象
DOI：
10.1007/978-94-010-0628-6_13
复制
发表时间：
2002
影响因子：
4.8
通讯作者：
M. Mishchenko
中科院分区：
文献类型：
--
作者：
V. Rosenbush;N. Kiselev;V. Avramchuk;M. Mishchenko
对无大气层的太阳系天体（行星、卫星、行星环和小行星）以及彗星和行星际尘埃粒子的地面和航天器观测提供了大量新的相位角和波长范围内的光度和偏振数据。本章回顾了近冲观测到的光度和偏振相位效应的研究进展。我们还提出了最近的偏振观测结果的伽利略卫星的木星，Iapetus，和小行星64安吉丽娜在非常小的相位角。现有数据的分析，使我们能够确定的亮度和偏振反对的影响和调查它们之间的相关性的参数。所获得的结果可以形成详细的理论建模和解释的相位效应的观测基础。
Ground-based and spacecraft observations of atmosphere less solar system bodies (planets, satellites, planetary rings, and asteroids) and cometary and interplanetary dust particles have provided a wealth of new photometric and polarimetric data over a wide range of phase angles and wavelengths. This chapter reviews the progress in the study of the photometric and polarimetric phase effects observed near opposition. We also present the results of recent polarimetric observations of the Galilean satellites of Jupiter, Iapetus, and the asteroid 64 Angelina at very small phase angles. Analyses of the available data allow us to determine the parameters of the brightness and polarization opposition effects and investigate correlations between them. The results obtained may form the observational basis for detailed theoretical modeling and interpretation of the phase effects.