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汤宁宇 左沛 李菂 Lei Qian Tie Liu Yue-Fang Wu Marko Krco Meng-Ting Liu You-Ling Yue Yan Zhu Hong-Fei Liu Dong-Jun Yu Jing-Hai Sun Peng Jiang Gao-Feng Pan Hui Li Heng-Qian Gan Rui Yao Shu Liu FAST Collaboration 《天文和天体物理学研究(英文版)》2020,(5):181-192
We present a pilot HI survey of 17 Planck Galactic Cold Clumps(PGCCs)with the Five-hundred-meter Aperture Spherical radio Telescope(FAST).HI Narrow Self-Absorption(HINSA)is an effective method to detect cold HI being mixed with molecular hydrogen H2 and improves our understanding of the atomic to molecular transition in the interstellar medium.HINSA was found in 58%PGCCs that we observed.The column density of HINSA was found to have an intermediate correlation with that of 13CO,following log(N(HINSA))=(0.52±0.26)log(N13CO)+(10±4.1).HI abundance relative to total hydrogen[HI]/[H]has an average value of 4.4×10-3,which is about 2.8 times of the average value of previous HINSA surveys toward molecular clouds.For clouds with total column density NH>5×1020 cm-2,an inverse correlation between HINSA abundance and total hydrogen column density is found,confirming the depletion of cold HI gas during molecular gas formation in more massive clouds.Nonthermal line width of 13CO is about 0-0.5 kms-1 larger than that of HINSA.One possible explanation of narrower non-thermal width of HINSA is that HINSA region is smaller than that of 13CO.Based on an analytic model of H2 formation and H2 dissociation by cosmic ray,we found the cloud ages to be within 106.7-107.0 yr for five sources. 相似文献
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选取1990~1999年贵州省3个国家基准站(威宁、贵阳、三穗)气象观测数据,评估了逼近法在贵州不同海拔地区计算湿球温度的效果,对比了BP(Back Propagation)神经网络模型和逼近法在计算湿球温度方面的优劣。结果表明:(1)3站逼近法计算值与观测值之间平均绝对误差分别为0.059℃、0.046℃、0.042℃,误差<0.1℃的数据比例为83.91%、91.52%、92.76%;当气温低于0℃时,误差>0.2℃的频率呈增长趋势,其原因可能是逼近法中对结冰的判别和实际情况存在差异导致高海拔地区的计算效果差于低海拔地区。(2)3站BP神经网络模型计算精度比逼近法分别提高60.71%、57.45%、57.78%,误差<0.1℃的数据比例提高到97.38%、97.18%、97.44%,有效地解决了高海拔地区气温低于0℃频率较高而导致逼近法计算误差偏大的问题,在低海拔地区的计算结果也优于逼近法。(3)BP神经网络模型计算湿球温度需要对各测站进行单独拟合,在低海拔地区针对大量站点且计算精度要求不高时可用逼近法,反之则用BP神经网络建立单站模型。 相似文献