精密定轨用地球大气模型误差的补偿方法

本文提出了一种用于精密轨道确定的地球大气模型误差的补偿方法，这种方法采用改进 大气周日峰角的技术，有效地补偿了大气密度模型的误差，并具有较好的物理意义．与传统 的每圈改进一次加速度的方法比较，轨道确定达到了相当的径向精度，且避免了轨道改进参 数间的相关性，同时解算参数的数量也少了一半．     

Statistical analysis of the optical variability of QSO's

For 34 QSOs and 9 active galaxies with known optical variation and measured redshifts, the rate of optical variation appears to be positively correlated with the age: older quasars vary more violently than younger ones and active galaxies are the most violent of all.     

兰州台潮汐形变观测结果与景泰6.2级地震

本文介绍了兰州形变台水管倾斜仪和石英伸缩仪1987年初至1990年底观测资料的调和分析结果和各分量的年变化,分析了M_2波γ和α因子的月重复精度及其对非潮汐变化的监测能力和本区当前的构造活动特征,对异常变化与1990年10月20日甘肃景泰Ms6.2级地震之关系作了初步探讨。     

On the origin of δ spots

Mount Wilson sunspot drawings from 1966 through 1980 were used in conjunction with Hα filtergrams from Big Bear Solar Observatory to examine the origin of δ spots, spots with bipolar umbrae within one penumbra. Of the six cases we studied, five were formed by the union of non-paired spots. They are either shoved into one another by two neighboring growing bipoles or by a new spot born piggy-back style on an existing spot of opposite polarity. Proper motions of the growing spots take on curvilinear paths around one another to avoid a collision. This is the shear motion observed in δ spots (Tanaka, 1979). In the remaining case, the δ spot was formed by spots that emerged as a pair. Our findings indicate no intrinsic differences in the formation or the behavior between δ spots and spots of normal magnetic configuration.     

On the dynamic activity in sheared corridors of large delta spots

In the extraordinarily flare-prolific region of March 1989, NOAA region No. 5395, unusual dynamic activity in the photosphere was observed for the first time inside the large delta spot (Wanget al., 1991). Analyses of two additional large delta spots with sheared penumbral fibrils revealed that what occurred in the March 1989 delta spot is not an isolated case; similar complex dynamic activity was observed in the August and October 1989 delta spots. Both are flare-prolific regions as well, each producing 5 X-class flares. As in the March 1989 case, registered and highly time-compressed white-light movies were made from digital data obtained at Big Bear Solar Observatory. The new evidence confirmed the unusual activity: (1) penumbral motions in the directions of sheared penumbral fibrils near the inversion line as well as elsewhere in the delta complex, and (2) new spots emerging in the midst of penumbral motions. The manner and place of emergence are different from those in ordinary emerging flux regions, and often the spots are without observable opposite polarity flux. It is easy to see how the emergence of new spots in the midst of strong fields as well as the shear motions near the inversion line further enhance the flare productivity of the large delta spot regions. But we have yet to understand the origin of the dynamic activity observed.     

湖北省棉花产量的变化与棉田布局的战略调整*

本文揭示了湖北省棉花亩产的增长具有北高南低的特点,分析了鄂北地区种植棉花的自然优势和经济效盆大于江汉平原,从而提出湖北省棉花北移的战略调整的设想。     

推覆构造的特征及其与油气的关系

推覆构造是地壳中广泛发育的一种构造型式。逆冲断层常成带地平行排列,形成逆冲带和叠瓦构造。断层多呈上陡下缓或阶梯状,底部常有滑脱构造,并在深处常收敛在一个基底逆冲断层上。推覆构造还常与飞来峰、构造窗、叠瓦构造、牵引褶皱、后冲断层和平移断层等构造现象一起产出。推覆构造不仅扩大了找油的领域,它本身对油气的生成、储集、运移、圈闭和保存条件都有着重要的影响。虽然它们有时可造成某些对油气藏不利的因素,但更经常地则是造成油气藏形成的有利条件。当然,影响油气藏形成的因素十分广泛,它不仅限于推覆构造本身的某些特征,同时还决定于许多其它地质条件。因此,不同推覆构造或同一推覆构造的不同部位,其含油气远景也是很不相同的。     

攀枝花市大气污染物降水清除机制的研究

本文采用了主成份分析及因子分析的方法,研究了影响降水pH值的主要源及其贡献和这些源被降水清除的机制。分析结果表明:大气中一次污染物是影响降水pH及各种成分浓度的主要因素。人为污染源包括高排放源、低排放源和汽车源,它们的排放物以碱性物质为主;自然污染源包括输送物、腐烂物、自然NOx等,它们的排放物主要是酸性物质;在一般情况下,降水的pH值取决于高、低排放源排放的碱性物质的多寡;降水量越大,清除的污染物越多,在雨季各测点降水平均pH值为6.31～7.10。在高排放源影响小的地方,对持续时间长的大雨,降水后期的pH能反映自然源的影响,其值小于5.60。可见,攀枝花市酸雨几率极低甚至降水呈碱性,     

昆仑山玉龙喀什河最大洪峰出现日期的灰色预测

玉龙喀什河是昆仑山北坡最大的河流——和田河的主要支流。玉龙喀什河同古孜洛克水文站夏洪严重。因此预测最大洪峰出现日期是十分有意义的。用灰色系统理论来预测最大洪峰出现日期,是以原始数据为基础,按累加生成,建立GM(1,1)模型,并通过模型求出平滑度,进而作相对误差检验,合格后再作预测。经过检验,预测基本上符合实际。     

The relation of the average sound intensity to range in homogeneous shallow-water

Using a “three parameters” bottom model, the average sound intensity in homogeneous shallow water with constant depth is found by a better expression to be finite for normal mode number of water layer. The space structure of the sound field and some factors controlling the near, middle and far fields are discussed with this expression. This paper was published in Chinese inOceanologia et Limnologia Sinica 14 (2): 198–202, 1983.