Morphological characters of the two-ribbon flare of 1981 May 13 and their explanation

We give a summary of the morphology of the two-ribbon flare of 1981 May 13. One striking feature is that the Ha flare began at about 0338' UT and the double-ribbon structure was formed about 0346, $\text{before}$ the impulsive phase of the radio 3 cm burst at 04 11 UT. The 3 cm radio burst flux beginning at 03 33 UT showed only slow, stepwise increases lasting half an hour until the impulsive phase and this type of increase is usually regarded to be a typical thermal process. Each step in the radio flux corresponded to a variation in the Ha flare, showing that the radio and Hα emissions during this period came from the same thermal source. In this paper, we explain this behaviour in terms of Hyder's model: we think that the magnetic trough supporting the solar prominence rose for some reason, causing the prominence matter (the dark filaments) to fall along the magnetic lines and to hit the chromosphere and trigger off the flare. We give rough estimates of the energy density, the height of prominence and the infall matter at the different radio increments. We also give a qualitative explanation for the appearances of the single-peak structure in the radio burst at 0411 and the covering of the sunspot shortly after at 04 13 and propose several possible mechanisms.     

壳聚糖/α,β-甘油磷酸凝胶微球的制备及性质研究

以液体石蜡为油相,以壳聚糖/α,β-甘油磷酸凝胶溶液为水相,用乳化法制备了壳聚糖/α,β-甘油磷酸凝胶微球,并对微球形态、粒径分布、溶胀性、蛋白吸附率、溶血率、体外降解率进行了分析。光学显微镜下显示,微球形态圆整,粒径主要分布在100～400μm;扫描电镜显示,微球内部为三维网络状结构,骨架清晰;pH=7.4的PBS缓冲液中干凝胶微球的溶胀率为218.08%,普通壳聚糖微球为70.98%;1和24h测得凝胶微球的蛋白吸附量分别为13.21和15.68μg/g,普通壳聚糖微球分别为3.71×103和4.83×103μg/g;微球的溶血率小于5%,血液相容性良好;体外降解实验显示,壳聚糖的脱乙酰度、黏度以及溶菌酶浓度对壳聚糖/α,β-甘油磷酸凝胶微球的降解性质产生影响。     

The mechanism for the impact of sea surface temperature anomaly on the ridgeline surface of Western Pacific

Based on the atmospheric circulation data provided by ECMWF and the sea surface temperature data by NOAA, we studied the mechanism for the impact of sea surface temperature anomaly on the ridgeline surface of western Pacific using an improved high truncated spectral model. Our results show that the wave-wave interaction and the wave-mean flow interactions are weaker in the inner dynamic process of atmospheric circulation, when atmospheric circulation is forced by the sea surface temperature of El Niño pattern. With the external thermal forcing changed from winter to summer pattern, the range of ridgeline surface of western Pacific moving northward is smaller, which causes the ridgeline surface of western Pacific on south of normal. On the contrary, the wave-wave interaction and the wave-mean flow interaction are stronger, when atmospheric circulation is forced by the sea surface temperature of La Niña pattern. With the external thermal forcing turning from winter to summer pattern, the ridgeline surface of western Pacific shifts northward about 19 latitude degrees, which conduces the ridgeline surface of western Pacific on north of normal. After moving to certain latitude, the ridgeline surface of western Pacific oscillates with the most obvious 30–60 d period and the 4°–7° amplitude. It is one of the important reasons for the interannual variation of ridgeline surface of Western Pacific that the atmospheric inner dynamical process forced out by different sea surface temperature anomaly pattern is different.     

奥陶系岩溶古地貌恢复及对气藏分布的控制作用——以鄂尔多斯盆地苏里格东区41-33区块为例

苏东41-33区块位于鄂尔多斯盆地中央古隆起的北部南缘,长期沉积间断的风化壳不整合面形成复杂的岩溶古地貌,属苏里格气田东部奥陶系碳酸盐岩气藏的重要勘探区。研究基于钻井、测井、地震及生产动态资料分析,综合运用地球物理法、残厚法和印模法,优选本溪组顶9号煤层和马家沟组马五5灰岩为标志层,深入探讨古地貌单元的恢复依据和划分标准,精细恢复岩溶古地貌形态,并明确岩溶古地貌特征及其对气藏分布的影响。研究表明:苏东41-33区块整体处于二级地貌单元岩溶斜坡之上,奥陶系古风化壳上下地层厚度可划分出上薄下薄、上薄下厚、上厚下薄等5种组合类型,细分古坡地、残丘和沟槽3个三级地貌单元;古地貌总体趋势走向为北高南低,出露层位展布由马五4过渡到马五1。中南部发育连片残丘,北部见小型零星残丘,恢复厚度低于15m,残留厚度超过85m;北部发育2条侵蚀沟槽带,充填厚度大于20m,残留厚度小于45m;古坡地分布范围广泛,周围被古残丘与沟槽所分割,残留厚度介于45m^85m之间,恢复厚度大于10m。古地貌类型对风化壳气藏分布具有明显的控制作用,岩溶残丘及残丘边缘带的古坡地储层叠合厚度增大,溶蚀孔洞充填程度低,主力含气层保存完整且连通性较好,是寻找高产井的目标区,而岩溶古沟槽相对不利于天然气富集,所钻遇气井多为低产或无产能。     

基于ArcIMS的农业立体污染空间信息网

针对农业立体污染及时发布和数据共享的需求,运用ArcIMS建立了农业立体污染空间信息网,以达到农业立体污染防治的现代化、信息化、规范化和高效化。     

青藏高原植被垂直带与气候因子的空间关系

集成了青藏高原气候区149个山地植被垂直带数据,利用国家基本气象台站自建站以来到2001年的地面观测日气象数据,计算了地面的温暖(WI)、寒冷(CI)、湿润(MI)、吉良龙夫(Kira)干湿指数、干燥度(Idm)等水热指数,运用GIS的空间分析模块,模拟了青藏高原水热条件的空间分布形势,探讨山地植被垂直带谱分布规律与制约因子的定量指标.结果表明:在高原的东北部、西北边缘,以荒漠、荒漠草原、山地森林、山地草原、灌丛、草甸为组合的半干旱、干旱结构向高原腹地以高寒草原、高山草甸、荒漠带组合的高寒干旱带谱结构的变化;东南、南部边缘,以温暖湿润为特征的以森林带为优势带谱组合结构逐渐向寒冷的高原中心变化;高原的地势效应,致使的水热形势旱现从中央向边缘变化的趋势是致使青藏高原植被垂直带谱分布的重要原因.     

Observation and Research of the Transits of Extrasolar Planets

In order to make more accurate estimates of the physical parameters of extrasolar planets, the observation and research on the phenomena of transits of the 7 known stars with the planetary systems TrES-1, TrES-3, XO-2, WASP-1, WASP-2, WASP-3 and HAT-P-7 are carried out with the 1-m reflecting telescope at Shandong University Weihai Astronomical Observatory/Weihai Municipal Astronomical Observatory. The fundamental conditions of the observation and data processing are introduced, and the transit light curves as well as the parameters of some planets derived from them are given. At the same time, when the results are summarized and analyzed, the prospects for the more in-depth and detailed researches which will be further carried out are also described.