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1.
Zhang Qing Wang Li-fan Hu Jing-yao P. A. Mazzali Wang Zhen-ru 《Chinese Astronomy and Astrophysics》1995,19(4):426-431
We present the modeling of the ultraviolet and optical spectra obtained simultaneously on 1993 April 15 with the HST and at Lick Observatory. A Monte Carlo code is employed in the modeling and a comparison is made between models reported by different groups. With an atmosphere similar to the Sun in chemical composition, the observed spectral lines are well reproduced by a power law density structure of index around 20 except the strong H and HeI λ5876 lines which have peculiar absorption profiles. The photospheric velocity is found to be 9500 km/s and the blackbody temperature of the spectrum is 7990 K. For H and HeI λ5876, we suggest a two-component density structure which has a smoother layer located immediately outside the steeply decreasing inner envelope. The power law indices are most probably 20 and 3, respectively, with the transition point at about 13 000 km/s. In addition, this outer smooth layer serves to flatten the far UV spectrum as observed. 相似文献
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In an attempt to elucidate the mechanics of deep-water wave breaking, a variety of breaking waves, including spilling and plunging waves, of different length scales and geometries was studied. The waves were generated through wave-wave interactions using wave packets with constant-steepness components, constant-amplitude components, and also components following the Pierson-Moskowitz distribution. Wave steepening prior to breaking were found to cause an increase in the high frequency spectral slope of the wave spectrum. The slopes were correlated to the type of breaking and the intensity of the breaking. The energy loss through breaking varied with the spectral characteristics of the wave packet. On the other hand, it was also noted that, irrespective of the wave packet, the losses were from the higher frequency end of the first harmonics. 相似文献
4.
This study investigates the effect of non-linear soil deformation on the displacement interaction among energy piles. The work is based on interaction factor analyses of full-scale pile group tests, whose results are compared with experimental evidence. The results presented highlight the tendency of interaction factor analyses that ignore non-linear soil deformation to overestimate the interaction and the displacement of energy pile groups. This outcome, in accordance with previous studies for conventional pile groups subjected to mechanical loads, may be considered in the analysis and design of energy pile groups subjected to thermal (and mechanical) loads through the interaction factor method. 相似文献
5.
Two meteor events which were sighted in the Gujarat skies of India, were accompained by the visibility of sporadicE ionization on the ionograms recorded at Ahmedabad (Geog. Lat. 23·2°N, long. 72·30°E). The first event was the Dhajala fireball
which flashed into the geoatmosphere along an E-N to W-S trail at about 20·40 h IST on 28 January 1976; the closest distance
of the ground projection of meteor trail from Ahmedabad was 50km. The other event was a possible meteor group sighted over
Ahmedabad on 28 May 1978, at about 21·10 h IST. This work describes the nature of the sporadicE ionization observed on Ahmedabad ionograms during the two events. Features of theEs echo during the Dhajala event which indicate that it could be of meteoric origin are discussed. Meteor theory is used to
relate the observed ionization with the physical dimensions of the Dhajala meteorite as obtained by other workers. 相似文献
6.
结合西安至宝鸡客运专线XBZQ-2标段施工实践,主要介绍了客运专线CPⅢ建网与施测的技术,实践结果表明工程所采用的CPⅢ施测技术具有精度高、安全可靠等优点,对类似工程具有一定的参考价值。 相似文献
7.
为保留等高线群简化过程中的地形特征信息,研究了一种等高线群渐进式简化方法。首先,从等高线数据中提取地形特征点及地形特征线;将提取的地形特征点和特征线作为约束条件予以量化,并作为控制变量;再依据渐进式图形简化的思想,利用控制变量对等高线上的非特征点、特征点、特征线及其关联的弯曲进行渐进式取舍,从而实现等高线群的动态简化。实验结果表明,该方法能够有效地保持地貌形态特征,同时提高了简化过程的智能化程度。 相似文献
8.
彩色扫描地图中背景色的等高(等深)线矢量化研究 总被引:1,自引:0,他引:1
在介绍矢量化方式的基础上,根据国外地图的特点,选择了基于全要素地图的矢量化方式。通过综合利用多义点及方向信息,对等高线矢量化的追踪过程控制,不仅避免了误追踪等特殊情况,且减少了人机交互,实现了有背景色区域等高(等深)线的半自动矢量化。 相似文献
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