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作 者:段辑 刘煜[2] 申远灯[2] 宋腾飞[2] 刘顺庆[2] 张雪飞[2] 温骁[2] 杨磊[2] 林隽[2] 刘忠[2] 王建成[2]
机构地区:[1]云南省昭通市昭阳区气象局,云南昭通657000 [2]中国科学院国家天文台/云南天文台,云南昆明650011
出 处:《天文研究与技术》2012年第2期184-202,共19页Astronomical Research & Technology
基 金:国家自然科学基金(11078004;10933003;11073050);科技部973项目(MOST 2011CB811400);中国科学院方向性项目(KJCX2-EW-T07);国家天文台天文专项基金(西部太阳选址)资助
摘 要:采用云南省昭通市昭阳区气象局1960年到1988年间在大山包实地采集的气象数据资料,并根据优良太阳观测台址所要求的各项参数指标,对大山包29年来的气象资料进行了系统的统计分析,发现该候选址点在干季(10月到次年4月)具有年日照时间增长、云量减少、相对湿度降低、风速较小且风向稳定、气候变化具有明显的周期性等特征。考虑到交通条件便利,初步判定它是一个具有潜力的优良太阳观测候选址点。This paper statistically analyzes the meteorological conditions of Mt. Dashanbao by using the meteorological data from the year 1960 to the year 1988, which were collected by the Meteorologic Bureau of the Zhaoyang District, Zhaotong City, Yunnan Province. We focus on meteorological parameters particularly relevant to the selection of an excellent solar observation site. We investigate the annual variation patterns of the parameters with wavelet analysis. We have found that the monthly relative humidity, average sunshine time, and average temperature all have nearly-fixed variation cycles of about one year, which is very important for ground-based solar observation. In addition, these parameters show two distinct steady stages in each year, and we call them the dry season (from November to April of next year ) and wet season (from May to October). In the dry season, the monthly relative humidity, mean temperature, and average cloud amount are low, while the montly average sunshine-time and wind-speed values are relatively large. The average wind speed over a long time is still low, even though at some occasions high wind speed can influence observation. In addition, the wind direction is very stable there, so we can easily overcome the drawback of the occurrences of high wind speeds. In the wet season, the site does not fit well for solar observation due to the poor meteorological conditions. However, we do not rule out short-lasting meteorological conditions for observation in the wet season. Moreover, the site on Mt. Dashanbao is not far from the Yunnan Observatory, Chinese Academy of Sciences, Kunming, China. The convenient transportation can save a significant amount of financial resources in the installation, operation, and maintenance of telescope (s). Based on our statistical results, we conclude that Mt. Dashanbao is a potentially excellent solar observation site in the west China. In summary the site has long sunshine time, low coverage of clouds, low wind speed, steady wind direction, good s
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