漂移扫描太阳直径测量中0.1赫兹以下的大气涨落
天体物理仪器与方法
2015-06-03 v1 太阳与恒星天体物理
摘要
为了理解凌星法监测太阳直径的关键性，我们测量了0.001-1赫兹范围内视宁度的功率谱。
引用
@article{arxiv.1112.6187,
title = {Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter measurements},
author = {Costantino Sigismondi and Andrea Raponi and Giulia De Rosi and Michele Bianda and Renzo Ramelli and Massimo Caccia and Matteo Maspero and Loretta Negrini and Xiaofan Wang},
journal= {arXiv preprint arXiv:1112.6187},
year = {2015}
}
备注
3 pages, 3 figures, proc. of the Fourth French-Chinese meeting on Solar Physics Understanding Solar Activity: Advances and Challenges, 15 - 18 November, 2011 Nice, France