Site-testing at the Muztagh-ata Site.V. Nighttime Cloud Amount during the Last Five Years

Abstract

The clarity of nights is the major factor that should be carefully considered for optical/infrared astronomical observatories in site-testing campaigns. Cloud coverage is directly related to the amount of time available for scientific observations at observatories. In this article, we report on the results of detailed night-time cloud statistics and continuous observing me derived from ground-based all-sky cameras at the Muztagh-ata site from 2017 to 2021. Results obtained from acquisition data show that the proportion of the annual observing me at the Muztagh-ata site is 65%, and the best period with the least cloud coverage and longer continuous observing time is from September to February. We made a comparison of the monthly mean observing nights obtained from our all-sky cameras and CLARA dataset, results show that the discrepancy between them may depend on the cloud top heights. On average, this site can provide 175 clear nights and 169 nights with at least 4 hours of continuous observing time per year.

11 pages, 9 figures

References in corpus (3)

• Sky Quality Meter and satellite correlation for the night cloud cover analysis at astronomical sites
• Long-term trends of light pollution assessed from SQM measurements and an empirical atmospheric model
• New analysis of the fraction of observable nights at astronomical sites based on FengYun-2 satellite data