排序方式： 共有24条查询结果，搜索用时 15 毫秒
11.
本文针对Groom-Bailey分解法在消除地表电性不均匀体对MT数据的畸变效应时存在的问题引入遗传算法,对基于传统线性最优化方法的GB分解算法进行改进,提出基于遗传算法的大地电磁阻抗张量分解方法.通过对理论合成数据以及三维/二维模型正演数据的分解试验,并且对青藏高原北缘阿尔金断裂地区实际MT数据进行分解处理,证明了基于遗传算法的GB分解能够更加有效地校正三维/二维情况下近地表三维电性不均匀体所造成的畸变影响.最后,在已有算法基础上,研究了基于遗传算法的多频率GB分解算法和MT数据静校正算法,并通过实际MT数据的处理证明了这些算法的有效性. 相似文献
12.
《世界地质(英文版)》2012,(3):210-215
Based on China National Standard of Soil Engineering Classification (GB/T 50145-2007) and the Unified Soil Classification System of American Society for Testing Materials (ASTM D-2478), two kinds of soil laboratory engineering classification methods were discussed and analyzed from the aspects of the definition in particle fraction, classification of soil type and evaluation standard for soil gradation. There is a same limit of fine grains fraction in the two standards, and there are three main types of soil in GB/T 50145-2007 and two in ASTM D-2487. Different evaluation standards of gradation are put forward for gravels and sands in ASTM D-2487. Same criteria of A line, B line and controlling value of plastic index are in the plasticity chart of both standards. 相似文献
13.
精确计算设计洪水值对水利水电工程规划设计至关重要,其关键问题之一是选择合适的分布函数。目前多数研究仅选取单一的频率分布线型进行洪水频率分析,其设计洪水结果具有较大的不确定性。研究引入一种新的广义分布函数,即第二类beta分布(Generalized beta distribution of the second kind,GB2),进行洪水频率分析。该四参数分布具有较好的灵活性,基本可拟合任何偏度和峰度的曲线。采用最大熵原理推求分布函数的参数。研究利用科罗拉多河流域数据检验广义第二类beta分布函数的拟合效果,并将所提分布与水文中的其它传统分布进行比较分析。结果表明:四参数的广义第二类beta分布非常适于水文频率分析,其拟合效果基本优于水文中的其它传统分布。 相似文献
14.
15.
A.C. Fabian A. Celotti K. Iwasawa G. Ghisellini 《Monthly notices of the Royal Astronomical Society》2001,324(3):628-634
BeppoSAX observations of the high-redshift ( z =4.72) blazar GB 1428+4217 confirm the presence of a complex soft X-ray spectrum first seen with the ROSAT PSPC. Flattening below a rest-frame energy of 5 keV can be accounted for by absorption from an equivalent column density of (cold) gas with N H ∼8×1022 cm−2 . Below 2 keV a (variable) excess of a factor of ∼20 above the extrapolated absorbed spectrum is also detected. These findings are consistent with and extend to higher redshifts the correlation between increasing soft X-ray flattening and increasing z , previously pointed out for large samples of radio-loud quasars. We propose that such features, including X-ray absorption and soft excess emission as well as absorption in the optical spectra, can be satisfactorily accounted for by the presence of a highly ionized nuclear absorber with column N H ∼1023 cm−2 , with properties possibly related to the conditions in the nuclear regions of the host galaxy. High-energy X-ray emission consistent with the extrapolation of the medium-energy spectrum is detected up to ∼300 keV (rest frame). 相似文献
16.
17.
TH. Boller A. C. Fabian W. N. Brandt M. J. Freyberg 《Monthly notices of the Royal Astronomical Society》2000,315(2):L23-L28
We report on a ROSAT PSPC observation of the highly luminous z =4.72 radio-loud quasar GB 1428+4217 obtained between 1998 December 11 and 17, the final days of the ROSAT satellite. The low-energy sensitivity of the PSPC detector was employed to constrain the intrinsic X-ray absorption of the currently most distant X-ray detected object. Here we present the detection of significant soft X-ray absorption towards GB 1428+4217, making the absorbing material the most distant matter yet probed with X-ray spectroscopy. X-ray variability by 25±8 per cent is detected on a time-scale of 6500 s in the rest frame. The X-ray variation requires an unusually high radiative efficiency of at least 4.2, further supporting the blazar nature of the source. 相似文献
18.
We report on an examination of two geodemographic classification systems based on an analysis of 1991 census variables, for districts, wards and census enumeration districts in England and Wales. We also review the associations among the variables examined, the extent to which certain underlying components might account for the overall variation and the types of areas that are least typical. The results show that small areas are different in many different ways; a few dimensions cannot provide enough information to describe an area fully. Diversity on most scales remains even after geodemographicclassification, emphasizing the advantages of task-specific classification. 相似文献
19.
Isobel M. Hook & Richard G. McMahon 《Monthly notices of the Royal Astronomical Society》1998,294(1):L7-L12
We report the discovery of two radio-loud quasars with redshifts greater than 4: GB1428+4217, with z =4.72, and GB1713+2148 with z =4.01. This doubles the number of published radio-selected quasars with z >4, bringing the total to 4. GB1428+4217 is the third most distant quasar known and the highest redshift radio and X-ray source currently known. It has a radio flux density at 5 GHz of 259±31 mJy and an optical magnitude of R ∼20.9. The rest frame absolute UV magnitude, Mv (1450 Å), is −26.7, similar to that of the archetypal radio-selected quasar 3C273 [ z =0.158; Mv (1450 Å)=−26.4]. GB1428+4217 is tentatively detected in ROSAT PSPC observations, which has been confirmed by more recent ROSAT observations described in a companion paper by Fabian et al. Both quasars were discovered during the CCD imaging phase of an investigation into the evolution of the space density of radio-loud quasars at high redshift. Combined with our earlier survey results, these objects give a lower limit on the space density of quasars with radio power P 5 GHz >5.8×1026 W Hz−1 sr−1 between z =4 and z =5 of 1.4±0.9×10−10 Mpc−3 . This can be compared to 2.9±0.2×10−10 Mpc−3 at z =2 from Dunlop & Peacock for flat-spectrum sources of the same luminosity. 相似文献
20.
A. C.Fabian K.Iwasawa A.Celotti W. N.Brandt R. G.McMahon I. M.Hook 《Monthly notices of the Royal Astronomical Society》1998,295(1):l25-l28
The X-ray-luminous quasar GB 1428+4217 at redshift 4.72 has been observed with ASCA . The observed 0.5–10 keV flux is 3.2 Å– 10−12 erg cm−2 s−1 . We report here on the intrinsic 4 − 57 keV X-ray spectrum, which is very flat (photon index 1.29). We find no evidence for flux variability within the ASCA data set or between it and ROSAT data. We show that the overall spectral energy distribution of GB 1428+4217 is similar to that of lower redshift MeV blazars, and present models that fit the available data. The Doppler beaming factor is likely to be at least 8. We speculate on the number density of such high-redshift blazars, which must contain rapidly formed massive black holes. 相似文献