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371.
作为基层气象部门,文化建设对于一个单位强化内部管理、谋划科学发展,重塑价值体系具有重要意义。为此对基层气象台站文化建设情况开展了问卷调查,分析了基层台站气象文化建设的现状。在此基础上,探讨了气象文化的重要作用、气象文化建设的阻碍因素和气象文化建设的措施。 相似文献
372.
Xinhui Bi Bernd R.T. Simoneit Guoying Sheng Shexia Ma Jiamo Fu 《Atmospheric Research》2008,88(3-4):256-265
Total suspended particles (TSP), collected during June 2002 to July 2003 in Guangzhou, a typical economically developed city in South China, were analyzed for the organic compound compositions using gas chromatography–mass spectrometry (GC/MS). Over 140 organic compounds were detected in the aerosols and grouped into different classes including n-alkanes, hopanoids, polycyclic aromatic hydrocarbons, alkanols, fatty acids, dicarboxylic acids excluding oxalic acid, polyols/polyacids, lignin products, phytosterols, phthalates and water-soluble sugars. The total amounts of the identified organic compounds including unresolved complex mixture (UCM) ranged from 3112 ng/m3 in spring to 5116 ng/m3 in winter, comprising on seasonal average 2.8% of TSP. Primary organic compounds peaked in winter although there are no heating systems burning fuels in Guangzhou. The highest saccharide levels occurred in fall due to agricultural activities. This study demonstrated that utilization of fossil fuels, biomass burning, soil resuspension and plastic/refuse burning are the major contributors to the identified organic compounds in the urban atmosphere of South China. 相似文献
373.
Trends in graded precipitation in China from 1961 to 2000 总被引:3,自引:0,他引:3
Daily precipitation rates observed at 576 stations in China from 1961 to 2000 were classified into six grades of intensity, including trace (no amount), slight (≤ 1 mm d^-1), small, large, heavy, and very heavy. The last four grades together constitute the so called effective precipitation (〉 1 mm d^-1). The spatial distribution and temporal trend of the graded precipitation days are examined. A decreasing trend in trace precipitation days is observed for the whole of China, except at several sites in the south of the middle section of the Yangtze River, while a decreasing trend in slight precipitation days only appears in eastern China. The decreasing trend and interannual variability of trace precipitation days is consistent with the warming trend and corresponding temperature variability in China for the same period, indicating a possible role played by increased surface air temperature in cloud formation processes. For the effective precipitation days, a decreasing trend is observed along the Yellow River valley and for the middle reaches of the Yangtze River and Southwest China, while an increasing trend is found for Xinjiang, the eastern Tibetan Plateau, Northeast China and Southeast China. The decreasing trend of effective precipitation days for the middle- lower Yellow River valley and the increasing trend for the lower Yangtze River valley are most likely linked to anomalous monsoon circulation in East China. The most important contributor to the trend in effective precipitation depends upon the region concerned. 相似文献
374.
一个区域地气耦合柱状模式的发展及其对半干旱区的模拟 总被引:1,自引:0,他引:1
在现有的区域气候模式的基础上构建了用于研究地气耦合模拟的区域柱状模式,其中包括了详细的物理过程,可以作为研究半干旱区地气相互作用过程的工具。通过区域柱状模式与不同陆面模式的耦合,检验了不同陆面模式在非耦合和耦合两种情况下对半干旱区的模拟性能。结果表明,陆面模式在耦合后对感热的模拟偏差放大,而潜热的模拟效果得到了改进,不同的陆面模式对区域柱状模式的模拟性能影响较大,耦合了CoLM后的区域柱状模式对地表气象要素的模拟得到了较大的改进。 相似文献
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Pin Zhang Zai-Qi Fu 《天体物理学报》2009,(7):770-776
The Infrared Space Observatory (ISO) Short-Wavelength Spectrometer (SWS) spectra of 10 Be stars are presented. It can be seen that the Be stars show a diversity in their ISO SWS01 spectral classifications by Kraemer et al., from naked stars, stars associated with dust, stars with warm dust shells, stars with cool dust shells to very red sources. In addition, the Brα/HI(14-6) line flux ratio derived for the sample stars is compared with that of P Cyg, and it is found that the line ratio of Be stars which were investigated show not only lower values as suggested by Waters et al., but also larger values. Therefore, the line ratio cannot be used to judge whether a star is a Be star or not. 相似文献
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On 13 December 2006, some unusual radio bursts in the range 2.6?–?3.8 GHz were observed during an X3.4 flare/CME event from 02:30 to 04:30 UT in active region NOAA 10930 (S06W27) with the digital spectrometers of the National Astronomical Observatories of China (NAOC). During this event many spikes were detected with the high temporal resolution of 8 ms and high frequency resolution of 10 MHz. Many of them were found to have complex structures associated with other radio burst types. The new observational features may reflect certain emission signatures of the electron acceleration site. In this paper, we present the results of the analysis of the new observational features of the complex spikes. According to the observed properties of the spikes, we identify five classes. Their observational parameters, such as duration, bandwidth, and relative bandwidth, were determined. Most spikes had negative polarization, but spikes with positive polarization were observed during a short time interval and were identified as a separate class. Based on the analysis of observations with Hinode/SOT (Solar Optical Telescope) we suggest that the sources of the spikes with opposite polarizations were different. Combined observations of spikes and fiber bursts are used to estimate the magnetic field strength in the source. 相似文献