首页 | 本学科首页   官方微博 | 高级检索  
文章检索
  按 检索   检索词:      
出版年份:   被引次数:   他引次数: 提示:输入*表示无穷大
  收费全文   92篇
  免费   2篇
测绘学   4篇
大气科学   2篇
地球物理   19篇
地质学   39篇
海洋学   3篇
天文学   20篇
自然地理   7篇
  2022年   1篇
  2021年   1篇
  2020年   4篇
  2019年   1篇
  2018年   1篇
  2017年   2篇
  2016年   1篇
  2015年   1篇
  2014年   2篇
  2013年   9篇
  2012年   5篇
  2011年   1篇
  2010年   2篇
  2009年   5篇
  2008年   4篇
  2007年   4篇
  2006年   3篇
  2005年   4篇
  2004年   5篇
  2003年   1篇
  2002年   4篇
  2000年   2篇
  1999年   5篇
  1998年   1篇
  1997年   1篇
  1995年   3篇
  1991年   1篇
  1990年   1篇
  1987年   1篇
  1986年   1篇
  1984年   1篇
  1983年   2篇
  1981年   1篇
  1979年   1篇
  1975年   2篇
  1974年   2篇
  1972年   2篇
  1971年   2篇
  1959年   1篇
  1955年   1篇
  1939年   1篇
  1920年   1篇
排序方式: 共有94条查询结果,搜索用时 15 毫秒
91.
Local policies can play an important role in establishing a context that shapes vulnerability and influences subsequent recovery of lifelines under the natural hazards of extreme wind and seismic events. External factors, such as access availability, have long been known to influence the rate of restoration of utility systems following blackouts. Thus, since system performance takes place within a socio-technical-political context, it can be anticipated that selected local policies may also influence either the geographic extent of damage or the rate of restoration or both. This project empirically validates the assumption that selected local non-design policies establish a context that significantly (measurably) influences system functionality in terms of spatial extent and duration of outage.  相似文献   
92.
We present an improved technique for calculating bulk densities of low-mass (<1 g) meteoroids using a scattering model applied to the high-density plasma formed around the meteoroid as it enters Earth’s atmosphere. These plasmas, referred to as head echoes, travel at or near the speed of the meteoroid, thereby allowing the determination of the ballistic coefficient (mass divided by physical cross-section), which depends upon speed and deceleration. Concurrently, we apply a scattering model to the returned signal strength of the head echo in order to correlate radar-cross-section (RCS) to plasma density and meteoroid mass. In this way, we can uniquely solve for the meteoroid mass, radius and bulk density independently. We have applied this new technique to head echo data collected in 2007 and 2008 simultaneously at VHF (160 MHz) and UHF (422 MHz) at ALTAIR, which is a high-power large-aperture radar located on the Kwajalein Atoll. These data include approximately 20,000 detections with dual-frequency, dual-polarization, and monopulse (i.e. angle) returns. From 2000 detections with the smallest monopulse errors, we find a mean meteoroid bulk density of 0.9 g/cm3 with observations spanning almost three orders of magnitude from 0.01 g/cm3 to 8 g/cm3. Our results show a clear dependence between meteoroid bulk density and altitude of head echo formation, as well as dependence between meteoroid bulk density and 3D speed. The highest bulk densities are detected at the lowest altitudes and lowest speeds. Additionally, we stipulate that the approximations used to derive the ballistic parameter, in addition to neglecting fragmentation, suggest that the traditional ballistic parameter must be used with caution when determining meteoroid parameters.  相似文献   
93.
94.
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号