The late-Paleozoic mafic volcanic rocks occurring in the surrounding areas of the Gonghe basin are distributed in the A’nyêmaqên ophiolite zone, Zongwulong tectonic zone and Kuhai-Saishitang volcanic zone. The mafic volcanics in the A’nyêmaqên zone formed an ancient ridge-centered hotspot around the Majixueshan OIB, the Kuhai-Saishitang mafic rocks consist of E-MORB and continental rift basalts and the Zongwulong volcanic rocks are enriched N-MORB. The regionally low Nb/U and Ce/Pb ratios reflect the influence of the OIB material on the mafic magma source. From geochemistry, spatial distribution and tectonic relationship of the mafic rocks, an ancient triple-junction centered at the Majixueshan can be inferred. The existence of the Kuhai-Saishitang aulacogen may have provided a tectonic channel for the Majixueshan OIB materials metasomatizing the magma source for the Zongwulong rocks. The formation of the triple-junction and the rifting of the Zongwulong zone have separated the orogens and massifs in the region.
结合JPL和GFZ的中性大气标准反演算法,发展了上海天文台中性大气掩星标准反演算法流程.对CHAMP观测资料进行中性大气反演,并将反演结果与ECMWF(the European Center for Medium Range Weather Forecasting)的预报大气数据进行比较.作为讨论,指出将来的发展方向. 相似文献
Remote sensing technique has played an important role in land use dynamic monitoring, but as for the land use dynamic monitoring
at county level, traditional remote sensing methods such as satellite imagery visual interpretation and computer classification
can not meet its demand for accuracy. The result of 1: 10 000 land use investigation map has high accuracy, but this method
can not be used to dynamically monitor the land use because of its big expenses, long period and difficulty in updating data.
In this paper, the characteristics of physiognomy, climate and the status of land use in Dehui County are taken into consideration
and a set of method, which takes use of 3S techniques and applies to Northeast China Plain, is come up with. When the land
use type of a land parcel changed as a whole, the date updating can be make by changing its land type ID in the attribute
table in a GIS. When the land use type of an irregular area changed, GPS receivers are used to position its border. This set
of method is characteristic of high accuracy and low expenses. It gets the information of land use change timely and can be
used to dynamically monitor the land use.
Foundation item: Under the auspices of the key project of the National Ninth Five-year Plan (96-B02-01-07).
Biography: LI Lin-yi (1968 —), female, a native of Jilin, Ph. D. candidate of Changchun Institute of Geography, the Chinese
Academy of Sciences. Her research interest includes land use change monitoring and crop yield estimation using “3S” techniques. 相似文献
For the 3 : 1 Jovian resonance problem, the time scales of the two degrees of freedom of the resonant Hamiltonian are well-separated [5]. With the adiabatic approximation, the solution for the fast oscillations can be found in terms of the slowly varying variables. Thus the rapidly oscillating terms in the slow oscillation equations can be treated as forced terms. We refer to the resonance between the forcing and intrinsic frequencies as a forced secondary one in this paper. We discuss the forced secondary resonances in asteroidal motion at the 3 : 1 commensurability by using Wisdom's method. The results show that the orbits situated originally near the resonance will leave the neighbourhood of resonance and tend to the separatrices and critical points for different energies, respectively. We have not found any stochastic web as expected in this case. Moreover, we study the problem of validity on the approximation of a system.The Project Supported by the National Natural Science Foundation of China. 相似文献
We study the relation between the infrared colors[ OⅢ] emission lines,gaseous absorbing column density(NH) ,and the detectability of the polarized (hidden)broad-line region(HBLR) in a large sample of 75 Seyfert 2 galaxies(Sy2s).From the indicators of star-formation activity,f60/f100 and LFIR/LB,we find some evidence that the Sy2s without HBLR show higher star-formation activities than those with HBLR,in agreement with previous prediction.Also,we confirm that the HBLR Sy2s tend to have a larger luminosity ratio of the core to the host galaxy,suggesting that the HBLR Sy2s display more powerful AGN activity.Howerver,the level of obscuration found in previous papers in nearly indistinguishable between the two types of Sy2s.The results support the statement that the non-HBLR Sy2s,with a weaker core component and a stronger star-formation activity component,are intrinsically different from the HBLR Sy2s,which are Sy1 systems with a hidden powerful AGN core and a low star-formation activity.The indications are that the non-HBLR Sy2s might be at an earlier evolutionary phase than the HBLR Sy2s. 相似文献