爆炸影响降水的观测分析

本文对“炮响雨落”的现象进行了实验验证。初步结果表明:在一定云雨条件下,炮击后可能促使未降水积状云产生降水,也可能促使已降水云的降水参量增大,这些变化发生迅速,但维持时间不长。并指出炮击促进云体降水的作用可能是通过改变支托水滴的气流造成的。在适当条件下,通过炮击影响气流的瞬时作用,可能触发云内不稳定能量释放,造成持续下沉,破坏云的发展,从而防止冰雹灾害。     

一次雹暴的特征随时间演变的分析

冰雹通常由强烈的积雨,即所谓雹暴中形成。在雹暴的整个生命过程中,无论是外观还是内部特征,都在不停地发生着变化。由于这种变化十分激烈和迅速,大冰雹往往就在某一短时间内(通常不超过30分钟)生长并危害农业。加上此时伴随着闪电大风大雨,要观测它甚为困难。因此,人们至今对其演变的许多方面还缺乏详细和确切的的认识。     

一次渤海气旋发生的初步分析

一九七五年五月四日晨开始,在河北省东部、渤海海面、辽东半岛、山东半岛、黄海北部海面先后出现9—10级西北大风。掖县、羊角沟、招远、海阳、蓬莱等地区阵风达12级,并伴有阵性降雨过程。由于风的来势很猛,使沿海部分地区的人民生命财产受到了一定程度的损失。     

夏季青藏高原流场三维结构的模拟实验

本文用流体模拟实验的方法,研究了我国夏季青藏高原及邻近地区环流的三维结构和成因,主要结果为: 无转动因素时,高原加热作用能引起流体在低层径向地朝高原辐合,在高原上层放射状向周围辐散.高层辐散流体的一部分在高原内部开始下沉,形成高原上空的对流环,在有转动的实验中也观察到.辐散流体中还出现波动. 高原内部经常出现两个对流上升中心,中心附近的温度有较大脉动,两个对流上升区之间有时为下沉运动,构成高原内部独特的对流环. 通过高原中部的南北垂直剖面上,可观察到方向相反的两个对流环,流体在高原中部上升,在南北高原范围内下沉.在高原外部为高原加热引起的下沉运动. 实验表明,包括基本东西风和高原以外热源的环境背景条件,对高原流场有重要作用. 实验结果为解决夏季青藏高原环流的三维结构提供了依据,文中列举了一些说明的现象。     

广西天气分析

广西地处祖国南疆,属低纬地区,山丘起伏,地形复杂,天气多变,每年都有不同程度的灾害,给发展农业生产带来不利的影响。在“农业学大寨”、“工业学大庆”的运动中,我们在自治区党委的领导下,进一步明确了气候为农业服务的方向,天气预报为灾害性天气和农事活动关键性天气为主攻方向,开展气象科研,大搞业务基本建设,对广西的主要灾     

Complementary Notes on a ‘Well-known’ Marine Heterotrichous Ciliate, Folliculinopsis producta (Wright, 1859) Frauré-Fremiet, 1936 (Protozoa, Ciliophora)

1　Introduction　Folliculina likeciliatesarecommonlyfoundinlit toralzonesandareeasilyrecognizedbytheirlargesi zesandspecialstructures (i.e.vase shapedloricaandperistomiallobe) .Tillnow ,dozensofspecieshavebeenreportedworldwide (Kahl,1 932 ;Faur啨Fremiet,1…     

Land cover change detection in West Jilin using ETM ＋ images

In order to assess the information content and accuracy of Landsat ETM digital images in land cover change detection,change-detection techniques of image differencing, normalized difference vegetation index,principal components analysis and tasseled-cap transformation were applied to yield 13 images. These images were thresholded into change and no change areas. The thresholded images were then checked in terms of various accuracies. The experiment results show that kappa coefficients of the 13 images range from 48.05-78.09. Different images do detect different types of changes. Images associated with changes in the near-inflared-reflectance or greenness detects crop-type changes and changes between vegetative and non-vegetative features. A unique means of using only Landsat imagery without reference data for the assessment of change in arid land are presented. Images of 12t June, 2000 and 2‘d June, 2002 are used to validate the means. Analyses of standard accuracy and spatial agreement are performed to compare the new images (hereafter called “change images” ) representing the change between the two dates. Spatial agreement evaluates the conformity in the classified “change pixels” and “no-change pixels” at the same location on different change images and comprehensively examines the different techniques. This method would enable authorities to monitor land degradation efficiently and aeculately.     

Star formation and figure rotation in the early-type galaxy NGC 2974

We present Galaxy Evolution Explorer ( GALEX ) far-ultraviolet (FUV) and near-ultraviolet (NUV) imaging of the nearby early-type galaxy NGC 2974, along with complementary ground-based optical imaging. In the ultraviolet, the galaxy reveals a central spheroid-like component and a newly discovered complete outer ring of radius 6.2 kpc, with suggestions of another partial ring at an even larger radius. Blue FUV–NUV and UV-optical colours are observed in the centre of the galaxy and from the outer ring outwards, suggesting young stellar populations (≲1 Gyr) and recent star formation in both locations. This is supported by a simple stellar population model which assumes two bursts of star formation, allowing us to constrain the age, mass fraction and surface mass density of the young component pixel by pixel. Overall, the mass fraction of the young component appears to be just under 1 per cent (lower limit, uncorrected for dust extinction). The additional presence of a nuclear and an inner ring (radii 1.4 and 2.9 kpc, respectively), as traced by [O  iii ] emission, suggests ring formation through resonances. All three rings are consistent with a single pattern speed of  78 ± 6  km s⁻¹ kpc⁻¹, typical of S0 galaxies and only marginally slower than expected for a fast bar if traced by a small observed surface brightness plateau. This thus suggests that star formation and morphological evolution in NGC 2974 at the present epoch are primarily driven by a rotating asymmetry (probably a large-scale bar), despite the standard classification of NGC 2974 as an E4 elliptical.