MoLLIST: Molecular Line Lists, Intensities and Spectra
MoLLIST: Molecular Line Lists, Intensities and Spectra
复制标题
DOI：
10.1016/j.jqsrt.2019.106687
复制
发表时间：
2020-01-01
影响因子：
2.3
通讯作者：
Bernath, Peter F.
中科院分区：
文献类型：
--
作者：
Bernath, Peter F.
冷星、棕矮星和系外行星的天文光谱的模拟需要高分辨率的线表和许多分子的吸收截面。地球大气层和太阳系中的其他行星也需要类似的数据集。回顾了线条列表的要求，并讨论了创建线条列表的方法。提供了要在不同单位之间转换的方程式。介绍了MOLLIST(分子线表、强度和光谱)数据的编制方法，并以此为例进行了说明。(C)2019爱思唯尔有限公司。保留所有权利。
The simulation of astronomical spectra of cool stars, brown dwarfs and exoplanets requires high resolution line lists and absorption cross sections of many molecules. Similar data sets are needed for the Earth's atmosphere and other planets in our solar system. The requirements for line lists are reviewed and methods used to create them are discussed. Equations to convert between different units are provided. The MoLLIST (Molecular Line Lists, Intensities and Spectra) data compilation is presented and used as an example. (C) 2019 Elsevier Ltd. All rights reserved.