丽江与纳木错天光背景亮度在一天中的不同变化过程
he sky brightness is an important parameter to evaluate the excellence of a coronal observatory, which directly determines whether the coronagraph can measure and monitor the coronal activity for a long time. The Sky Brightness Moniter (SBM) is a precision instrument for accurately measuring important atmospheric parameters such as the sky brightness, water vapor content, and atmospheric extinction. It is also an universal instrument for coronagraph site selection and an important equipment for solar site selection in western China. Before conducting statistical analysis on the accumulated data from Namco and Lijiang, this paper first performs an in-depth analysis using representative data from Namco and Lijiang. The aim is to preliminarily study and understand the characteristics of the sky brightness at the site based on the profiles of the representative data. Firstly, by considering the actual climatic characteristics and the normalized sky brightness, the paper gradually explains the different variations of the sky brightness throughout the day. Secondly, we establish an effective calculation method to measure and reveal the evolution characteristics of the sky brightness. The results show: (1) the sky brightness (green line, 530 nm) at the Lijiang station with an altitude of 3200 meters and the Namco site with an altitude of 4700 meters are both relatively good. The minimum values can reach the order of $10 \times 10-6$, ensuring the feasibility of regular corona observations; (2) the sky brightness at the Namco site and the Lijiang station evolves differently over time. The Lijiang station is not suitable for all-day observations, with morning conditions being far superior to those in the afternoon. In contrast, the Namco site has a longer observation time (from 9:00 AM to 4:00 PM), and its cooperation with the observation equipment of other stations can significantly improve the efficiency of space weather ground monitoring. The analysis results not only provides a sample analysis for subsequent statistics on the sky brightness at Namco but also demonstrates the expected characteristics of the sky brightness at Namco.
刘强、刘煜、宋腾飞、任安炳、赵明宇、张雪飞、李小波、祝凤荣、沙飞扬、OLOKETUYIJacobOladeji、王新建、段晓梅、罗启旺
LIU Yu;LIU QiangLIU Yu;SONG Teng-feiSONG Teng-feiLIU QiangSONG Teng-feiSONG Teng-feiSONG Teng-feiLIU YuLIU Yu;SONG Teng-feiLIU YuLIU YuLIU YuLIU Yu
天文学
望远镜: 选址 天文仪器 方法: 数据分析 技术: 图像处理
telescopes: site testing astronomical instrumentation methods: data analysis techniques: image processing
刘强,刘煜,宋腾飞,任安炳,赵明宇,张雪飞,李小波,祝凤荣,沙飞扬,OLOKETUYIJacobOladeji,王新建,段晓梅,罗启旺.丽江与纳木错天光背景亮度在一天中的不同变化过程[EB/OL].(2025-04-08)[2025-08-16].https://chinaxiv.org/abs/202504.00159.点此复制
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