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301.
Activities to provide energy for an expanding population are increasingly disrupting and changing the concentration of atmospheric gases that increase global temperature. Increased CO2 and temperature have a clear effect on growth and production of rice as they are key factors in photosynthesis. Rice yields could be increased with increased levels of CO2, however, the rise of CO2 may be accompanied by an increase in global temperature. The effect of doubling CO2 levels on rice production was predicted using rice crop models. They showed different effects of climate change in different countries. A simulation of the Southeast Asian region indicated that a doubling of CO2 increases yield, whereas an increase in temperature decreases yield.Enhanced UV-B radiation resulting for stratographic ozone depletion has been demonstrated to significantly reduce plant height, leaf area and dry weight of two rice cultivars under glasshouse conditions. Data are still insufficient, however, for conclusive results on the effect of UV-B radiation on rice growth under field conditions.Rice production itself has a significant effect on global warming and atmospheric chemistry through methane emission from flooded ricefields. Water regime, soil properties and the rice plant are major factors controlling the flux of methane in ricefields. Global and regional estimates of methane emission rates are still highly uncertain and tentative. Integration of mechanistic modeling of methane fluxes with geographic information systems of factors controlling these processes are required to improve estimates and predictions. 相似文献
302.
近年来湖南省在地勘行业管理上开展了法规法制建设、规划计划编制、勘查秩序维护、勘查成果管理、勘查外部环境改善等方面的工作,“八五”后3年继续开展法制建设、勘查登记管理、勘查成果管理、建立行业统计系统、做好服务协调工作,推广改革经验等。 相似文献
303.
戴振学 《吉林大学学报(地球科学版)》1993,(1)
抽水试验最优化设计,是指针对一个具体的地下水系统优选出一个抽水试验设计,它使抽水试验的费用最小化,而试验所获资料能满足识别参数所要求的可靠性,它可以概化为一个非线性的混合整数规划问题,其决策变量是确定抽水井和观测井的位置及井数、抽水量和观测频率等,采用搜索算法求解了这一优化问题,得到了理论最优解,并进行了实例演算。 相似文献
304.
谭山复式岩体位于江南过渡带北缘,是该区出露面积较大的复式岩体。本文对谭山复式岩体开展了地质调查、岩浆岩锆石U-Pb年代学和全岩地球化学分析。地质特征显示谭山复式岩体沿杨美桥背斜轴部侵入,根据岩性分析划分为碱长花岗岩、正长花岗岩和二长花岗岩。LA-ICP-MS锆石U-Pb定年结果显示,碱长花岗岩和正长花岗岩分别为128.9±1.6 Ma~128.8±2.5 Ma和129.8±2.6 Ma~129.2±1.8 Ma;结合前人已获得二长花岗岩成岩时代(128.5±1.7 Ma~126.7±1.7 Ma),谭山复式岩体形成于128.9±1.6 Ma~126.7±1.7 Ma之间,对应于皖南地区燕山期 3阶段岩浆活动(早阶段:153~146 Ma,中阶段:143~136 Ma,晚阶段:135~121 Ma)的最晚阶段(135~121 Ma)。该复式岩体碱长花岗岩、正长花岗岩和二长花岗岩的地球化学特征均表现为:富碱,高Ga/Al比值,强烈亏损Ba、Sr、P、Ti,富集 Rb、Th、Nd、Ce,显著的Eu负异常,均为碱性过铝质特征的A型花岗岩。谭山复式岩体起源于下地壳物质部分熔融,为陆内拉张环境背景下同源岩浆多期次上升侵位的产物。 相似文献
305.
综述了亚洲中部干旱气候若干研究进展,并对亚洲中纬度干旱区形成机理进行了深入分析。依据大尺度气候分类法将全球陆地划分为季风、地中海及西风带气候区,分别对应于年内季节循环中多雨—高温的同位相、反位相及不相关等类型水—热配置特征。亚洲中部干旱区南北部分属地中海和西风带气候区,其不同水—热位相配置又对应于不同的水汽通量及其散度等特征。研究揭示了欧亚大陆中部干旱区形成于降水不足且季节性水—热配置不当,起因于大气环流平均槽脊季节变化引起的大气动力—热力配置,其根源是海陆热力差异及大地形对大气环流强迫的结果。本文还讨论了季风区与非季风区之间平均气流水汽散度的季节性互动,以及行星尺度上不同气候区之间平均气流与瞬变涡动水汽散度之间的配置等问题。 相似文献
306.
在吕梁造山旋回期间(1900Ma)北瓦沟辽河群经受了多幕变质和多期变形的改造,可识别出三组皱褶构造:1.早期近东西向片内平卧褶皱,由固态流变机制形成(F_1);2.枢扭北北西—南南东向不对称褶皱(F_2);3.北东向开阔褶皱构造(F_3)。此外,还发育与褶皱构造相关的布丁构造和布丁褶皱。赋存在辽河群中的铅锌矿床遭受了强烈的改造作用并严格受构造控制。 相似文献
307.
In situ measurements of stratospheric H2SO4 and HSO3vapors using passive chemical ionization mass spectrometry were made in October 1982 after the eruption of volcano El Chichon. Data were obtained between about 20 and 41 km showing [H2SO4 + HSO3] sum concentrations between about 104 and 2 × 105 cm?3 below 29 km and a steep rise above this altitude. Maximum [H2SO4 + HSO3] values of about 3 × 106 cm?3 are reached above 35 km.Partial [HSO3] concentrations increase above 34 km reaching about around 40 km. From the measurements it is concluded that H2SO4 and probably HSO3photolysis have an important influence above 34 km leading to the observed increase of [HSO3] and a depletion of H2SO4vapor.It also seems that the data support the view of heterogeneous HSO3 removal. If correct, this would imply that stratospheric aerosols are formed primarily from HSO3 rather than H2SO4vapor. 相似文献
308.
Radium-226 (226Ra) activities were measured in the surface water samples collected from the Arctic Ocean and the Bering Sea during the First
Chinese National Arctic Research Expedition. The results showed that 226Ra concentrations in the surface water ranged from 0.28 to 1.56 Bq/m3 with an average of 0.76 Bq/m3 in the Arctic Ocean, and from 0.25 to 1.26 Bq/m3 with an average of 0.71 Bq/m3 in the Bering Sea. The values were obviously lower than those from open oceans in middle and low latitudes, indicating that
the study area may be partly influenced by sea ice meltwater. In the Bering Sea, 226Ra in the surface water decreased northward, probably as a result of the exchange between the 226Ra-deficient sea ice meltwater and the 226Ra-rich Pacific water. In the Arctic Ocean, 226Ra in the surface water increased northward and eastward. This spatial distribution of 226Ra reflected the variation of the 226Ra-enriched river component in the water mass of the Arctic Ocean. The vertical profiles of 226Ra in the Canadian Basin showed a concentration maximum at 200 m, which could be attributed to the inputs of the Pacific water
or/and the bottom shelf water with high 226Ra concentration. This conclusion was consistent with the results from 2H, 18O tracers. 相似文献
309.
Using data obtained with the 20-cm H full-disk telescope at Big Bear Solar Observatory and Fexii 195 Å EIT on SOHO, we analyze a sudden disappearance event of a quiescent filament in detail. The filament was located along the common boundary of the active regions NOAA 9672 (S19 E13) and NOAA 9673 (N03 E18). The filament disappeared during a time interval between 17:59 UT and 19:47 UT on 22 October 2001 immediately after the onset of a major flare, which occurred in the active region NOAA 9672. At about 23:23 UT of the same day, the filament began to reappear in H and, after about 15 hours, the filament recovered to its steady state with its size being slightly smaller than that before its disappearance. This filament disappearance event belongs to the thermal type of sudden filament disappearances, which is caused by an input of additional heat. The heating mechanism that leads to sudden thermal disappearances of quiescent filaments is still not well understood. This simple event, due to the explicit cause and effect relationship between the flare and the disappearance of the filament, shows us that the flare triggered some kind of heating mechanism which continued several hours. The heat may come from the flare via heat conduction from its ribbon or from the excitation of dissipating Alfvén waves. However, from the data analysis, we conclude that the flare triggered an in-situ heating, which is likely caused by magnetic reconnection. 相似文献
310.