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The remote response of the East Asian summer monsoon(EASM)to European black carbon(EUBC)aerosols was studied by using an ensemble of sensitivity experiments with the Geophysical Fluid Dynamics Laboratory(GFDL)atmospheric general circulation model(AGCM)Atmospheric Model version 2.1(AM2.1).The results show that EUBC causes an enhanced EASM.The resulted enhanced southwesterly brings more moisture supply from the Bay of Bengal,which causes an increase in precipitation over the Yangtze River valley,northeastern China,the eastern part of the Yellow River valley,and the Tibetan Plateau.Diagnostic examination suggests that EUBC induces enhanced tropospheric heating over most of the Eurasian Continent through a propagating wave train and horizontal air temperature advection.This phenomenon results in intensified thermal contrast between land and ocean,which accounts for the enhanced EASM.Moreover,reductions in EUBC emission in 1992 may have contributed to decadal weakening of the EASM in the early 1990s. 相似文献
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秋季黄河口附近海域沉积物反硝化速率及影响因素研究 总被引：2，自引：0，他引：2
用乙炔抑制法和现场静态箱法对黄河口附近海域秋季的反硝化速率进行了研究,该海域反硝化速率在3.8~19.3μmol/(m2.h)之间,平均10.27μmol/(m2.h)。影响其反硝化速率的主要因素为反硝化细菌的数量。黄河口的反硝化速率低于珠江口和长江口海域。 相似文献
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Yu Bai Yang Chen Xiang-Tao He Jiang-Hua Wu Qing-Kang Li Richard F.Green Wolfgang Voges 《中国天文和天体物理学报》2007,7(3):375-379
This is the third paper in a series connected with our Multiwavelength Quasar Survey. The survey is aimed to provide a quasar sample more complete than any previous survey by using a combined selection technique to reduce selection effects. We present the observational results for the X-ray candidates in field f836. We found 15 X-ray AGNs in this field of which eight are new discoveries. The X-ray data and optical spectra of these AGNs are given. We give the X-ray candidate selection criteria, which proved to be highly efficient in isolating X-ray AGNs. 相似文献
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Jiang-Hua Wu Xiang-Tao He Yang Chen Wolfgang Voges National Astronomical Observatories Chinese Academy of Sciences Beijing jhwu Department of Astronomy Beijing Normal University Beijing Max-Planck-Institut fur Extraterrestrische Physik D- Garching Germany 《中国天文和天体物理学报》2003,(5)
We report the discovery of five Narrow-Line Seyfert 1 galaxies (NLSls) identified from the ROSAT All-Sky Survey bright sources. One of them has a quasar-like luminosity and two, including the quasar-like one, have close companions and/or show interacting features. We calculate the central black hole masses and Eddington ratios for the five NLSls. In combination with the objects of Kaspi et al., we find that NLSls have smaller central black hole masses and higher accretion rate than normal Seyfert 1s. 相似文献
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Shun-Fang Liu Zhen-Yu Wu Xiao-Bin Zhang Jiang-Hua Wu Jun Ma Zhao-Ji Jiang Jian-Sheng Chen Xu Zhou 《天体物理学报》2009,(7):791-802
We report the results of a time-series CCD photometric survey of variable stars in the field of open cluster NGC 2126. In about a one square degree field covering the cluster, a total of 21 variable candidates are detected during this survey, of which 16 are newly found. The periods, classifications and spectral types of 14 newly discovered variables are discussed, which consist of six eclipsing binary systems, three pulsating variable stars, three long period variables, one RS CVn star, and one W UMa or δ Scuff star. In addition, there are two variable candidates, the properties of which cannot be determined. By a method based on fitting observed spectral energy distributions of stars with theoretical ones, the membership probabilities and the fundamental parameters of this cluster are determined. As a result, five variables are probably members of NGC 2126. The fundamental parameters of this cluster are determined as： metallicity to be 0.008 Z, age log（t） = 8.95, distance modulus （m - M）0 = 10.34 and reddening value E（B - V） = 0.55 mag. 相似文献
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Xu Zhou Zhen-Yu Wu Zhao-Ji Jiang Xiang-Qun Cui Long-Long Feng Xue-Fei Gong Jing-Yao Hu Qi-Sheng Li Gen-Rong Liu Jun Ma Jia-Li Wang Li-Fan Wang Jiang-Hua Wu Li-Rong Xia Jun Yan Xiang-Yan Yuan Feng-Xiang Zhai Ru Zhang Zhen-Xi Zhu National Astronomical Observatories Chinese Academy of Sciences Beijing China Nanjing Institute of Astronomical Optics & Technology National Astronomical Observatories Nanjing China Purple Mo... 《中国天文和天体物理学报》2010,10(3)
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安徽省西北部储藏有丰富的低温地热资源。NNE向与近EW向断裂是区内主要控热、导热断裂,第三纪馆陶组为主要热储层。可分为亳州第三纪热储异常区和太和～阜阳第三纪热储异常区。现状开采量较小,具有较大的开发利用前景。 相似文献