张掖地区的光合有效辐射特征

光合有效辐射(PAR)是植物进行光合作用的重要能量来源。本文利用HEIFE期间在临泽(FOP)和张掖(BOP)取得的太阳分光辐射资料，分析研究了张掖地区的光合有效辐射。结果表明：张掖地区晴天PAR在太阳总辐射中所占的比例在0.419-0.426之间。季节变化不明显；多云天气条件下比值大于晴天，且有较明显的季节变化，夏季大。冬季小。文中还根据实际观测资料拟合得到了张掖地区PAR的经验公式，据此估算和讨论了张掖地区PAR的分布情况．     

农田近地面层CO2和湍流通量特征研究

利用１９８５年５月至６月在北京郊区中国科学院农业生态试验研究站的麦田中实测的小麦不同生长期的ＣＯ２浓度梯度、光合有效辐射、净辐射、土壤热通量和温度、湿度及风速梯度等量的数据，采用空气动力学方法，计算了ＣＯ２通量、感热通量、潜热通量和动量通量。并对观测场地、仪器设备、校准方法及误差分析进行了描述。结果表明：从５月１４日到６月１５日，在１ｍ，２ｍ和１０ｍ处，ＣＯ２浓度振幅的日变化分别为１０３．４到２７．５，８７．５到２７．３和６９．８到１１．５ｐｐｍ；光合型和呼吸型的平均ＣＯ２浓度分别为３４５．３，３５０．６，３５７．５ｐｐｍ和３７３．９，３６９．７，３６２．１ｐｐｍ。在白天，ＣＯ２通量和梯度的输送方向是从大气向植被，在中午（１１时到１３时）输送达到负的最大值。在夜间，ＣＯ２通量和梯度输送的方向与白天相反，并且，在早晨（４时到６时）达到正的最大值。ＣＯ２通量与净辐射（Ｒｎ）、可利用能（Ｈ＋ＬＥ）、光合有效辐射和动量通量之间有较好的相关关系     

关于光合有效辐射的新实验结果

通过成都、昆明、广州等地生长季节内对总日射（Q）和光合有效辐射（QPAR）的长期连续自动同步观测发现，以小时累计量为基础的QPAR/Q比值仍比较稳定，季节、云量以及太阳高度的日变化对其影响不大。这与我们以前在华北平原的研究结论是一致的。并有随纬度降低而略增的趋势。     

A practical model to estimate photosynthetically active radiation using general meteorological elements in a temperate humid area and comparison among models

Although accurately evaluating photosynthetically active radiation is important, much effort is required to measure this radiation using a quantum sensor. We develop a new model that makes estimates using only general meteorological data—solar radiation, atmospheric pressure, air temperature, and relative humidity. Root mean square deviations for eight datasets at five sites in Japan were smaller than 5.2 %, similar to error in other studies and to individual differences of quantum sensors. Most root mean square deviations of nine previous models and our eight datasets are larger than that of the new estimation model, which performed well. This suggests that the model is useful for estimating photosynthetically active radiation in a temperate, humid area of Japan.     

冬小麦生长和产量形成与气象条件关系及其动态模拟的研究——以河南省黄淮平原冬小麦中、低产地区为例

本文以能量转换和物质循环的观点,根据大量的田间试验及气象资料,对河南省黄淮平原中、低产地区冬小麦生长和产量形成与气象条件的定量关系及其时空变化特点作了分析,并指出了小麦群体内部光合有效辐射(PAR)的垂直分布特征;群体中存在着一个对PAR的强烈削弱层,它随着小麦生育期的后延而升高。依该地区小麦干物质积累不同特点,作者提出了早播、适播、迟播和受冻害四种生长型。 在前人研究的基础上,作者提出了“冬小麦农业气象计算机模拟模型”(WWACSM),它由发育期、叶面积系数及光合生产三个一级子模式和若干个二级子模式组成:并结合河南省黄淮平原小麦生产实践,对其中某些子模式作了探索和改进,为进一步发展该地区小麦的商品生产提供了气象依据。     

东亚地区的大气辐射能的收支(一)——地球和大气的太阳辐射能收支

本文是讨论东亚地区大气辐射能收支研究工作的第一部分,讨论了以下三个问题: (1)本文利用文献[1]的水汽各吸收带的吸收光谱实验资料,求得了一个适合于手算的水汽对太阳辐射的总吸收能量公式(公式(6))。并把式(6)与Mugge—Moller公式进行了比较。 (2)利用公式(6),计算了东亚地区39个测站1,7月自地面到100毫巴各气层对太阳辐射的吸收能量,及其对大气的加温率。本文还进一步考虑了云的订正、大气对地面反射辐射的吸收,而求得了东亚地区对流层大气吸收能量的分布。 (3)利用1958—1960年中国地区的一些地面总辐射和反射率观测资料,以及本文计算的大气中各种吸牧能量,讨论了中国地区行星反射率的分布和地球大气系统中各种太阳辐射能的收支。     

COMPREHENSIVE ANALYSIS OF THE MACRO- AND MICRO-PHYSICAL CHARACTERISTICS OF DENSE FOG IN THE AREA SOUTH OF THE NANLING MOUNTAINS

Using the composite field observational data collected in the area south of the Nanling Mts. and numerical modeling, the seasonal features of dense fog and visibility, fog drop spectrum and physical concept of fog forming have been analyzed. The occurring frequency of low visibility（≤200 m） is very high with a mean of 24.7%, a maximum of 41.8% from the end of autumn to winter and next spring. The fog processes that occur in the area south of the Nanling Mts. in spring and winter result from the interactions of complicated micro-physical processes, the local terrain, water vapor transportation and the influencing weather system. The fog processes are arisen from advection or windward slope, which is much different from the radiation fog. Cooling condensation due to the air lifted by the local mountain plays an important role in fog formation. Windward slope of the mountain is favorable to the fog formation. Dense fog can occur at lower altitudes in the windward slope of mountain, resulting in the lower visibility. The fog is mainly of small-drop spectrum with smaller number-density than that of urban fog, and its drop spectrum has descending trend in the section of smaller diameter. The inverse relationship between fog water content and visibility is the best among several relationships of micro-variables. In addition to micro-physical processes of fog body itself, the motion of irregular climbing and crossing over hillside while the fog body is being transported by the wind are also important reasons for the fluctuation of micro-physical parameters such as fog water content.     

RADIATION BUDGET OF THE TROPOSPHERE OVER CHINA

Based on the theory of the radiation transfer and some physical approximation techniques,a numericalclimatological method for the radiation budget in the troposphere over China is proposed.By utilizingten-year-averaged climatological data (1960—1969,1961—1970) from 104 stations,the radiation budgetand its components of the troposphere over China are calculated.In contrast with the satellite observationsand other computational results,the present results are satisfactory.The main factors which determine theradiation budget are also discussed briefly.     

THE CHARACTERISTICS OF LOW-FREQUENCY OSCILLATIONS OVER THE SOUTH CHINA SEA

Using 1975-1993 (with 1978 missing) data of the outgoing longwave radiation (OLR), characteristics of seasonal variation of low-frequency oscillations in the South China Sea and its relation to the establishment and activity of the summer monsoon there are studied. As is shown in the result, the low-frequency oscillation in the South China Sea is much stronger in the period of summer monsoon than in that of winter monsoon and the summer monsoon there usually begins to set up in a negative phase of the first significant low-frequency oscillation for the early summer. The study also reveals that the circulation for the low-frequency oscillation during the summer monsoon in the Sea is embodied as north-south fluctuations of the ITCZ and east-west shifts of western ridge point of the West Pacific subtropical high, suggesting close correlation between the low-frequency oscillation and the active and break (decay) of the South China Sea monsoon. In the meantime. the work illustrates how the low-frequency oscillation in the South China Sea are superimposed with the seasonal variation of the general circulation. so that the summer inonsoon covers the establishment of the I^st, intensification of the 2^nd and 3^rd the low-frequency oscillations and decay of the 4^th oscillation.